Meteoritics & Planetary Science 38, Nr 7, Supplement, A189–A248 (2003)http://meteoritics.org
A189 © Meteoritical Society, 2003. Printed in USA.
The Meteoritical Bulletin, No. 87, 2003 July
Sara S. RUSSELL,1* Jutta ZIPFEL,2 Luigi FOLCO,3 Rhian JONES,4 Monica M. GRADY,1 Timothy McCOY,5 and Jeffrey N. GROSSMAN6
1Department of Mineralogy, The Natural History Museum, Cromwell Road, London SW7 5BD, United Kingdom2Max-Planck-Institut für Chemie, Postfach 3060, D-55020 Mainz, Germany
3Museo Nazionale dell’Antartide, Via Laterina 8, I-53100 Siena, Italy4Institute of Meteoritics, Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, New Mexico 87131, USA
5Department of Mineral Sciences, National Museum of Natural History, Smithsonian Institution, Washington DC 20560, USA6United States Geological Survey, MS 954, Reston, Virginia 20192, USA
*Corresponding author. E-mail: [email protected] supplemental maps and photographs, visit the Meteoritical Bulletin’s web site at http://www.meteoriticalsociety.org
(Received 16 May 2003)
Abstract–Meteoritical Bulletin No. 87 lists information for 1898 newly classified meteorites, com-prising 1048 from Antarctica, 462 from Africa, 356 from Asia (355 of which are from Oman), 18from North America, 5 from South America, 5 from Europe, and 3 from Australia. Information is pro-vided for 10 falls (Beni M’hira, Elbert, Gasseltepaoua, Hiroshima, Kilabo, Neuschwanstein, ParkForest, Pê, Pétèlkolé, and Thuathe). Two of these—Kilabo and Thuathe—fell on the same day. Orbitalcharacteristics could be calculated for Neuschwanstein. Noteworthy specimens include 8 Martianmeteorites (5 from Sahara, 2 from Oman and 1 from Antarctica), 13 lunar meteorites (all except onefrom Oman), 3 irons, 3 pallasites, and many carbonaceous chondrites and achondrites.
INTRODUCTION
The Meteoritical Bulletin is a compilation of announcementsby the Meteoritical Society’s Meteorite NomenclatureCommittee of newly described and classified meteorites.Several conventions are followed. Shock classification isafter Stöffler et al. (1991). The scale of Wlotzka (1993) isused for weathering grades, except as noted. For chondrites, aslash in petrologic type, shock stage or weathering grade,(e.g., H5/6) indicates a transitional assignment. A hyphen inpetrologic type assignment (e.g., H5–6) indicates the range oftypes observed in a breccia. Group names such as “L(LL)”indicate uncertain assignments, with the less probable groupin parentheses. “Ungrouped” indicates that a meteorite doesnot fit existing classifications. “Anomalous” is used if ameteorite can be assigned to an established class, but differsfrom other members of that class in a significant way. Allitalicized abbreviations refer to addresses tabulated at the endof this document.
NEWLY DESCRIBED METEORITES
Acfer 056–352, see Saharan meteorites from Algeria
Acfer 328 27°43′N, 4°13′EAlgeriaFound 2001 December 22Carbonaceous chondrite (CV3)
A dark-brown, 180.07 g, roundish stone lacking fusion crustwas found by F. Beroud and C. Boucher. Mineralogy andclassification (B. Devouard and J.-L. Devidal, UBP; B. Zandaand M. Denise, MNHNP): large chondrules (~1 mm indiameter), several small CAIs, plus a very large (10 mm)irregular, zoned one. Mean olivine, Fa16.3 (range Fa0.6–56.5);mean low-Ca pyroxene, Fs16.0 (range Fs0.8–60.2); shock stage,S3; weathering grade, W2/3. Specimens: type specimen, 20 g,MNHNP; main mass with finders.
A190 S. S. Russell et al.
Acfer 331 27°35′N, 4°01′EAlgeriaFound 2001 December 23Carbonaceous chondrite (CM2)
Many, black, soft, porous and friable fragments totalling750 g were found by F. Beroud and C. Boucher. Mineralogyand classification (B. Devouard and J.-L. Devidal, UBP; B.Zanda and M. Denise, MNHNP): matrix is abundant, andchondrules display large fine-grained rims; metal is virtuallyabsent, except for small grains inside chondrules; hydratedphases characteristic of CM2 chondrites, including Fe-richserpentine and tochilinite (PCPs), are ubiquitous within thematrix. Mean olivine, Fa9.5 (range Fa0.7–45.4); mean low-Capyroxene, Fs5.4 (range Fs1.4–20.9). Weathering grade, W0.Specimens: main mass with finders; type specimen, 22.6 g,MNHNP.
Acfer 332 27°44′N, 4°08′EAlgeriaFound 2001 December 23Carbonaceous chondrite (CO3)
A brown, compact stone of 115.02 g was found by F. Beroudand C. Boucher. Mineralogy and classification (B. Devouardand J.-L. Devidal, UBP; B. Zanda and M. Denise, MNHNP):sharply defined chondrules from 0.1 to 0.3 mm and rare metalgrains; olivine, mean Fa26.2 (range Fa2.9–74.0), low-Capyroxene, mean Fs6.6 (range Fs1.3–14.8), W2. Specimens: typespecimen, 20.1 g, MNHNP; main mass with finders.
Acfer 333 27°34′N, 4°04′EAlgeriaFound 2001 December 26Carbonaceous chondrite (CO3)
A dark-grey, slightly friable stone broken in 5 fragments andtotalling 489 g was found by F. Beroud and C. Boucher.Mineralogy and classification (B. Devouard and J.-L.Devidal, UBP; B. Zanda and M. Denise, MNHNP): sharplydefined chondrules from 0.1 to 0.3 mm and rare metal grains;olivine, mean Fa23.2 (range Fa0.7–81.7), low-Ca pyroxene, meanFs7.4 (range Fs1.1–37.6), W2. Specimens: type specimen, 25.4 g,MNHNP; main mass with finders.
Adrar Bous, see Saharan meteorites from Niger
Aguemour 017, see Saharan meteorites from Algeria
Al Huqf 001, see Oman meteorites
American meteorite finds(11 meteorites)North and South AmericaFound 1999–2002
Several ordinary chondrites have been found at various
locations in North and South America. Details are given inTable 1.
Antarctic ANSMET meteorites(724 meteorites)AntarcticaFound 1999–2001
Appendix 1 brings up to date the list of officially announcedmeteorites from the US Antarctic Meteorite Program. Some10192 ANSMET meteorites have been listed in previouseditions of the Meteoritical Bulletin; these meteorites bringthe total to 10916. Listed are the classifications, masses,degrees of weathering, olivine and pyroxene compositions,pairing information, ice fields upon which the meteoriteswere found, and bibliographic information, all sorted bysample name. Meteorites were recovered from Bates Nunatak(BTN), Mount Crean (CRE), Finger Ridge (FIN), MeteoriteHills (MET), O’Dell Glacier (ODE), Queen Alexandra Range(QUE), and Tentacle Ridge (TEN). The meteorites inAppendix 1 were published in the Antarctic MeteoriteNewsletter (AMN) issues 25(2) (2002) and 26(1) (2003).Brief descriptions of meteorites other than equilibratedordinary chondrites are published in AMN. Note meteoritepairings may be tentative.
Antarctic NIPR meteorites(170 meteorites)AntarcticaFound 1988, 1998
Appendix 2 describes 170 meteorites from the JapaneseNational Institute of Polar Research (NIPR) program. Themeteorites in Appendix 2 were published in the MeteoriteNewsletter of the Japanese Collection of Antarctic Meteoritesvolume 11(1) 2002. They include 169 of the Asuka (A-)meteorites collected during the 1988 field season, larger than10 g in mass, and a Yamato (Y-) Martian meteorite collectedduring the 1998 field season. Listed are the classifications,masses, degrees of weathering, olivine and pyroxenecompositions, and bibliographic information, all sorted bysample name. Additional information, including briefdescriptions of some achondrites, is given in the newsletter.
Antarctic PNRA meteorites(144 meteorites)AntarcticaFound 2001 December
Table 2 reports the classification of 144 meteorites recoveredfrom the Frontier Mountain (FRO) blue ice field by the ItalianProgramma Nazionale delle Ricerche in Antartide (PNRA) inDecember 2001. Mineralogy and classification by A. Burroni,C. Ferraris and L. Folco (MNA-SI), A. Maras and M. Macrì(URoma), and Raul Carampin and Anna Maria Fioretti (UPad).Main masses, type specimens, thin sections, MNA-SI.
Meteoritical Bulletin No. 87 A191
Antarctic PSF meteorites(10 meteorites)AntarcticaFound 2000 January
Table 3 reports ten meteorite specimens found in blue iceregions of Moulton Escarpment in the Thiel Mountains (TIL)region of Antarctica. Specimens were collected by variousmembers of the Planetary Studies Foundation’s Antarctica2000 expedition, 2000 January 12–15. TIL 99016 is classifiedas E6 based on pyroxene composition and texture. Pairingwith TIL 91714 is possible. Analyses by G. A. Jerman,MSFC; classification by Paul Sipiera, Harper. Main masses,reference specimens and probe sections reside at PSF.Representative specimens held by R. Hoover, MSFC.
Areshima, see Saharan meteorites from Niger
Asuka (A-), see Antarctic NIPR meteorites
Bacqueville 49°19′20′′N, 01°21′56′′EFranceFound 1999 August 15Ordinary chondrite (H6)
A 395 g single stone was found by Mr. Trehour, who waslooking for metallic and archaeological objects in a field closeto the forest of Bacqueville. A few weeks later, when he cutthe stone, he realized it might be a meteorite. Classification(M. Denise, MNHNP): olivine, Fo18.96; low Ca-pyroxeneFs17.26, shock stage S3, weathering grade W5. Specimens:main mass Thierry Tréhour (finder); type specimen 33.8 g,MNHNP.
Ballarat 37°34.25′S, 143°49.52′EVictoria, AustraliaFound between 1867 and 1874Iron (IAB)
The 15 g meteorite was found during mining operations bythe Park Company in deep lead placer deposits below basaltflows in the West Ballarat goldfield. The meteorite wasdonated by Henry Rosales to the University of Melbourne inthe 1890s. Classification and description (J. Wasson, UCLA;W. Birch, Vic; L. Samuels, Monash): Nickel 6.1–6.3%, Co0.36%, Ga 95 µg/g, Ge 480 µg/g, Ir 1.1 µg/g. The meteoriteconsists of subgrains of kamacite crossed by partiallyresorbed Neumann bands and contains abundantschreibersite. Specimens: main mass and type specimen Vic.
Bates Nunatak (BTN), see Antarctic ANSMET meteorites
Beni M’hira ~32°52′N, 10°48′ETataouine, TunisiaFell 2001 January 8, 3:00 hrs local timeOrdinary chondrite (L6)
A meteorite was seen to fall in the Beni M’hira region by the
inhabitants of Ksar Beni M’hira, a small village ~35 km E ofFoum Tataouine, (SE Tunisia). Three fragments weighing1720, 300, and 200 g were recovered after the fall by localsoldiers. An additional 7 pieces totalling >14 kg were laterrecovered by private finders. Classification (L. Folco, MNA-SI; N. Perchiazzi, MSNP; N. Laridhi Ouazaa, Tunis): olivineFa24.3, orthoenstatite Fs21.4, shock stage S5, weathering gradeW0. Magnetic susceptibility (P. Rochette, CEREGE),expressed as the decimal logarithm of apparent mass specificsusceptibility (χ; in 10−9m3kg−1), is log χ = 5.01 ± 0.02.Specimens: 2190 g Tunis; type specimen, 29.2 g, and two thinsections, MSNP, one thin section, MNA-SI; 467.7 g, MNHNP;remaining mass with private collectors.
Bluewing 008, see American meteorite finds
Camel Donga 040 30°19′S, 126°37′EWestern Australia, AustraliaFound 1988Carbonaceous chondrite (C3, ungrouped)
Two stones of 34.5 g and 20.6 g were found by Alex Bevan.Classification and mineralogy (Mike Zolensky, JSC): Themeteorite is a genomict mixure of two lithologies. Bothlithologies contain abundant chondrules up to 1 mm across,some with well-developed, fine-grained rims or igneous rims;abundant smaller fragments, abundant troilite and pentlandite,but no pyrrhotite. Metal (Fe49Ni51 to Fe63Ni37) is rare due tohigh weathering grade. No magnetite was observed.Lithology 1 olivine, Fa1–49 with peak at Fa3; low Ca-pyroxene, Fs2–11. Lithology 2 olivine, Fa23–42 with apronounced peak at Fa35; pyroxene, Fs2–25. Lithology 1 ispetrographic type 3, and lithology 2 has been heated briefly toas high as 1100°C. Oxygen isotopes (R. Clayton, UChi): bothlithologies are identical in oxygen isotopic composition; δ18O= +0.18 to –0.01‰, δ17O = –4.39 to –4.48‰. Specimens:main mass and type specimen, WAM.
Chuckwalla 35°15′N, 118°06′WKern County, California, USAFound 1992 NovemberIron (IAB)
A single mass of 1.802 kg was found by Mr. Melvin Englishwhile quail hunting in the foothills of the TehachapiMountains. Classification (J. Wasson, UCLA): bulkcomposition Ni = 65.9 mg/g; Co = 4.61 mg/g, Ga = 100 µg/g,As = 12.4 µg/g, Ir = 2.72 µg/g, Au = 1.468 µg/g; see Wassonet al. (2002). The meteorite contains diamonds, some visiblemacroscopically, and many visible under the microscope. Thediamonds closely resemble those in Allan Hills A77283described by Clarke et al. (1981). Specimens: type specimens82.6 g UCLA, 38 g SI; main mass, GO.
A192 S. S. Russell et al.
Cimarron 37.85°N, 100.35°WGray County, Kansas, USAFound ~1948Carbonaceous chondrite (CM2)
A single stone of unknown weight was found by a rancher ona farm 3.4 miles north of Cimarron and sent to the Universityof Kansas in the early 1950s. A piece was later acquired by ameteorite collector and samples given to NAU in 1998 andpieces to AMNH in 1992 and 1993. Classification andmineralogy (M. Zolensky JSC; T. Bunch NAU): olivineranges from Fa1 to Fa64, with a peak at Fa1–2, average Fa1.2,PMD 11%. Low Ca pyroxene ranges from Fs2Wo5 to Fs5Wo4,also present are diopside, enstatite-diopside, pigeonite, andchromite. Porphyritic olivine, barred olivine and granularolivine crystals are most abundant, maximum chondrulediameter is 2 mm. Chondrules are sparse, matrix andchondrule rims comprise ~85 vol% of the meteorite. Thepercentage of matrix is similar to that of Bells and Nogoya,but the composition of these is lower in S and Mg, and higherin Si; this could be due to terrestrial weathering. Specimens:type specimen 21 g AMNH; 7.1 g NAU.
Dar al Gani 664–1022, see Saharan meteorites from Libya
Dar al Gani 879 27°08′N, 16°28′ELibyaFound 2000 NovemberAchondrite (ureilite)
A dark crusted stone of 26 g was found. Mineralogy andclassification (A. Burroni and L. Folco, MNA-SI): ureilitewith bimodal texture. Large twinned pigeonite (En85Wo7)crystals up to 16 mm in size poikilitically enclose olivine andpigeonite domains with typical, fine-grained (avg. grain size0.5 mm), granoblastic ureilite texture. In the typical-textureddomains, olivine and pigeonite have homogeneous cores(Fo92; En85Wo7) and reduced rims; intergranularcarbonaceous material mainly consists of graphite flakes.Moderate undulose extinction in silicates indicates moderateshock (S2). Weathering is moderate. Specimens: typespecimen, 5 g and thin section at MNA-SI; main mass withanonymous finder.
Dar al Gani 881 27°26′N, 16°12′ELibyaFound 2000 NovemberAchondrite (howardite)
A crusted stone of 86 g was found by a private collector in theDar al Gani desert. Mineralogy and classification (A. Burroniand L. Folco, MNA-SI): polymict breccia; clasts (up to severalmm in size) interspersed in a fragmental matrix include: 1)fine-grained basaltic eucritic clasts; 2) medium-grainedcumulate eucritic clasts (mostly pigeonite En58Wo6 and calcicplagioclase); 3) dark, quench-textured clasts with
microporphyritic pigeonite crystals set in cryptocrystalline orglassy matrix; 4) large (up to 1.5 mm in size) single-crystalfragments of low-Ca pyroxene of diogenitic origin(En70Wo3). The rock is cross-cut by discrete shock meltveinlets up to 0.25 mm thick. DaG 881 is possibly paired withDaG 923 and DaG 932. Specimens: type specimen, 17.6 g,and thin section MNA-SI; main mass with anonymous finder.
Dar al Gani 896 ~27°45′N, 16°53′ELibyaFound 2000 NovemberAchondrite (primitive, ungrouped)
A 22.6 g, dark, ~50% fusion crusted, stony fragment wasfound in Dar al Gani by a private collector. The specimen ismoderately oxidized and irregularly fractured. On slicing, itshows an homogeneous lithology. Shock veins of dark glasscross-cut the entire specimen. Classification and mineralogy(L. Folco, MNA-SI): abundant fine-grained, skeletal olivinecrystals (Fo82) are set in a mesostasis mainly consisting ofrhyolitic glass plus quench crystallites of pigeonite(En54Wo9). Minor mineral constituents include enstatite(En83Wo2), augite (En37Wo30), and traces of chromite,sulfides, Fe-Ni metal and phospates. Undulose extinction andplanar fracturing in olivine indicate moderate shock. Thinveins of secondary carbonates are present, most likely due toterrestrial weathering. Major element composition (P. Bland,OU) estimated from the mean of 256 broadbeam microprobeanalyses (spot size 20 µm,) indicates a komatiitic IUGScomposition (SiO2 = 47.22 wt%, Na2O + K2O = 1.53 wt%,MgO = 29.87 wt%) with chondritic Mn/Mg 7.5 × 10−3.Oxygen isotopes (I. A. Franchi, OU): δ17O = +2.547‰, δ18O= +3.501‰, ∆17O = +0.726‰, similar to mean H chondrite.Data suggest an affinity with igneous inclusions in ordinarychondrites and impact melt origin. Specimens: main masswith anonymous finder; 5.442 g and four thin sections, MNA-SI.
Dar al Gani 915 27°21′N, 16°11′ELibyaFound 2000 November Achondrite (howardite)
A crusted stone of 740 g was found. Mineralogy andclassification (A. Burroni and L. Folco, MNA-SI): polymictbreccia; with clasts (up to 1 cm in size) set in a fragmentalmatrix: 1) fine-grained, subophitic and intergranular, calcicplagioclase plus pigeonite-bearing eucritic clasts; 2) fine-grained, granular, pigeonite (En46Wo11) and calcicplagioclase-bearing eucritic clasts with various degrees ofmetamorphic annealing; 3) dark, quench-textured clasts withmicroporphyritic pigeonite crystals (and calcic plagioclaseplus pyroxene relics) set in cryptocrystalline or glassy matrix;4) large (up to 1.5 mm in size) single-crystal fragments oflow-Ca pyroxene of diogenitic origin (En64Wo1). DaG 915 is
Meteoritical Bulletin No. 87 A193
possibly paired with DaG 881 and DaG 932. Specimens: typespecimen, 23.1 g, and one thin section at MNA-SI; main masswith anonymous finder.
Dar al Gani 923 27°00′N, 16°21′ELibyaFound 2000 NovemberAchondrite (ureilite)
A weathered, crusted stone of 255 g was found. Mineralogyand classification (A. Burroni and L. Folco, MNA-SI): olivineand pigeonite-bearing ureilite with typical texture (averagegrain-size 1 mm). Mafic silicates show homogeneous corecompositions (olivine Fo80; pigeonite En77Wo9) and wide,strongly reduced rims. Undulose extinction, planar fracturesand kinking in both olivine and pigeonite indicate moderateshock deformation. Specimens: type specimen, 21.2 g, andone thin section, MNA-SI; main mass with anonymous finder.
Dar al Gani 932 27°24′N, 16°14′ELibyaFound 2000 NovemberAchondrite (howardite)
A crusted stony fragment of 23 g was found. Classificationand mineralogy (A. Burroni and L. Folco, MNA-SI): the thinsection that was studied (about 20 mm2) is dominated bymedium to large plagioclase and pyroxene crystal fragmentsof eucritic and diogenitic origin set in a fragmental matrix. Amm-sized fayalitic olivine crystal fragment is also set in thematrix. DaG 932 is possibly paired with DaG 881 and DaG915. Specimens: type specimen, 3.5 g, and two polished thinsections at MNA-SI; main mass with anonymous finder.
Dar al Gani 975 27°19.63′N, 16°13.00′ELibyaFound 1999 August 21Martian meteorite (basaltic shergottite)
A 27.55 g stone was found on 1999 August 21 in the sanddesert of Dar al Gani. Classification and mineralogy (A.Greshake, MNB; M. Kurz, Kurz): a basaltic shergottite withporphyritic texture; large chemically zoned olivinephenocrysts are set into a fine-grained groundmass consistingmostly of pyroxene and maskelynite; minor phases includechromite, Ti-rich chromite, sulfides, phosphates, and smallFe-rich olivines; olivine phenocrysts contain melt inclusions,small chromites and exsolution lamellae; pyroxenes aremostly chemically zoned pigeonites, some containorthopyroxene cores; olivine phenocrysts, Fa24.3–38.3;pigeonite, Fs21.1–29Wo5.9–13.8; orthopyroxene, Fs17.4–21.8Wo1.8–
3.4; augite, Fs18.5Wo34; matrix olivine, Fa35.9–39.8; maskelynite,An66.5–71.4; shock stage, S4; contains melt veins and meltpockets; low degree of weathering. Possibly paired with DaG476, 489, 670, 735 and 876. Specimens: main mass withanonymous finder; type specimen, 8.5 g, plus one polishedthin section MNB.
Dar al Gani 976 27°03.25′N, 16°23.25′ELibyaFound 1999 August 20Achondrite (ureilite, polymict)
A single stone of 32.03 g was found on 1999 August 20 in thesand desert of Dar al Gani. Classification and mineralogy (A.Greshake, MNB; M. Kurz, Kurz): a fragmental breccia withlithic and mineral clasts set into a ureilitic matrix dominatedby large olivine and pigeonite crystals; olivine core Fa13.4–23.8;reduced olivine rims, Fa1–15; pigeonite cores, Fs17–19.8Wo10–
10.8; reduced pigeonite rims, Fs4.3–10.2Wo3.4–6.7; pigeonitecontains up to 1.2 wt% Cr2O3; mineral clasts are plagioclase,An6.4–23.8, and orthopyroxene, Fs0.5–10.2; lithic clasts includeureilite material and fine-grained more Fe-rich olivine-pyroxene material; several C1-like clasts consisting ofmagnetites, sulfides and carbonates embedded into aphyllosilicate matrix were encountered; shock stage, S4; lowdegree of weathering. Specimens: main mass withanonymous finder; type specimen 7.8 g plus one polished thinsection, MNB.
Dar al Gani 983 26°44.25′N, 16°53.97′ELibyaFound 2002 March 23Achondrite (eucrite, polymict)
A single stone of 933 g, partially covered with a shiny blackfusion crust, was found on the Dar al Gani plateau during aGerman-Libyan expedition by J. Schlüter, F. Thiedig, L.Schultz and Abd Elfatah M. Abu Agreb. Mineralogy andclassification (J. Schlüter, Hamburg). The cut stone shows abright grey surface with strong brecciation with open cracksand some melt veins with vesicles. Cracks and vesiclesoccasionally contain white aggregates of gypsummicrocrystals. The meteorite consists of mineral and lithicclasts set in a fine-grained fragmental matrix. Clasts include:1) megacrysts of pigeonite, Fs37.9Wo4.4 (range Fs31.1–51.1;Wo1.5–7.2), and plagioclase An94.8 (range An92.7–95.4) up to 10mm in size; 2) equigranular, pigeonite, and plagioclase-bearing cumulate eucrite; pigeonite, Fs54.6Wo3.1 (range Fs48.5–
56.7; Wo1.5–9.8), with augitic (Fs25.0Wo40.9)) exsolution lamellaeup to 7 micrometers wide and maskelinitized plagioclase,An93.6 (range An88.7–96.4) are present in equal proportions; 3)dark, recrystallized impact melt with a spinifex-like textureconsisting mainly of pigeonite, Fs55.3Wo2.13 (range Fs54.1–56.4;Wo1.6–3.1) and plagioclase, An84.3 (An75.5–90.6). Diogeniticcomponents have not been found. The opaque componentsshow only slight weathering. Accessory minerals includingilmenite, chromite and troilite have been observed. The bulkcomposition of the meteorite is similar to Sioux County orJuvinas. Specimens: type specimens 281 g, Hamburg, 20 g,MPI, main mass, Industrial Research Center (IRC), Tripoli,Libya.
A194 S. S. Russell et al.
Dar al Gani 995 27°10.35′N, 16°23.17′ELibyaFound 2001 January 3Achondrite (eucrite)
A single stone of 56.12 g, partly covered by fusion crust, wasfound by an anonymous finder in the sand desert of Dar al Gani.Classification and mineralogy (A. Greshake, MNB; M. Kurz,Kurz): the specimen has subophitic texture with plagioclaselaths embedded in exsolved Ca-pyroxene, augite and silica;several areas of the meteorite are recrystallized; plagioclase,An89.5 (range An88.4–90.6); exsolved Ca-pyroxene withpigeonite lamellae, Fs51.8–60Wo5–15.2 and augite lamellae, Fs31–
34.2Wo37.3–40.5; unexsolved augite Fs30.7Wo40.6; minor phasesinclude orthopyroxene, ilmenite and Ti-rich chromite;plagioclase contains small crystallographically orientatedinclusions of augite, pigeonite and silica; augite contains smallplagioclase and Ti-rich chromite inclusions; the sampleappears unbrecciated in thin section; low degree of shock; lowdegree of weathering. Specimens: type specimen, 11.6 g, plusone polished thin section, MNB; main mass with anonymousfinder.
Dar al Gani 996LibyaFound 1999 May 14Lunar meteorite (fragmental breccia)
A single stone of 12.31 g was found by an anonymous finderin the sand desert of Dar al Gani. Classification andmineralogy (A. Greshake, MNB; M. Kurz, Kurz): afragmental breccia with lithic and mineral fragments set intoa fine-grained clastic matrix; the clast size is generally ≤1mm; mafic clasts are by far more abundant than feldspathicclasts; schlieren and vesicles are rare. Plagioclasecomposition, An96.7 (range An94.3–98.3); pigeonite, Fs19.7–
51.3Wo5.5–14.1; augite, Fs24.7–38.7Wo24.7–41.7; most Ca-pyroxenescontain pigeonite exsolution lamellae; olivine, Fa30.5 (rangeFa14.2–43.2). Orthopyroxene, Fe,Ni metal, ilmenite, Mg-Al-chromite, and troilite are present as minor phases; crystallinefragments include intersertal impact melt rocks, dark fine-grained and microporphyritic impact melt clasts, olivine,pyroxene and cataclastic feldspar; no regolith component,i.e., glass spherules was found; very strong mosaicism ofplagioclase, as well as abundant melt veins and melt pocketsattest a high degree of shock; the meteorite is moderatelyweathered; calcite occurs in cracks. Specimens: main masswith anonymous finder; type specimen, 2.5 g, plus onepolished thin section, MNB.
Dar al Gani 999 27°01.55′N, 16°21.23′ELibyaFound 2000 April 14Achondrite (ureilite, polymict)
Numerous fragments totalling 2106 g were found in the sanddesert of Dar al Gani. Classification and mineralogy (A.
Greshake, MNB; M. Kurz, Kurz): a fragmental breccia withmineral and lithic clasts set into a ureilitic matrix dominatedby large olivines; olivine core, Fa14.3–23.5; reduced olivinerims, Fa2.9–13.5; mineral clasts are pigeonite, Fs14.3Wo8.5 andorthopyroxene, Fs9.3; lithic clasts consist of fine-grainedolivine (Fa22) and pyroxene (Fs19.3Wo4.5) rich material; shockstage, S3; low degree of weathering. Specimens: main masswith anonymous finder; type specimen 20.8 g plus onepolished thin section, MNB.
Dar al Gani 1000 27°00.81′N, 16°21.95′ELibyaFound 1997Achondrite (ureilite, polymict)
A single stone of 17.92 g was found in the sand desert of Daral Gani. Classification and mineralogy (A. Greshake, MNB;M. Kurz, Kurz): a fragmental breccia with mineral and lithicclasts set into a ureilitic matrix dominated by large olivine andless abundant pyroxene crystals; olivine cores, Fa13.2–21.8;reduced olivine rims, Fa5–11.9; pyroxene cores, Fs14.9; reducedpyroxene rims, Fs4.4; mineral clasts are plagioclase, An22.9and orthopyroxene, Fs8.3; lithic clasts are fine-grained, moreFe-rich olivine-pyroxene material; shock stage, S3; lowdegree of weathering. Specimens: main mass with PeterJäger, Apolda, Germany; type specimen 4.2 g plus onepolished thin section, MNB.
Dar al Gani 1022 ~27°05′N, 16°15′ELibyaFound 2001 April 25Ordinary chondrite (LL7)
A stone of 33.6 g was found in the Dar al Gani region.Classification and mineralogy (S. Afanasiev, M. Nazarov,Vernad): the meteorite shows an equigranular texture; rarechondrule relics are present; plagioclase grain size up to 200µm. Mineral phases have homogeneous chemicalcomposition: olivine, Fa29.6; orthopyroxene, Fs25.0Wo2.42 (1.2wt% CaO); plagioclase, An11.2Or3.6; metal is commonlyoxidized and contains up to 45 wt% Ni and 2 wt% Co;chromite and troilite are present; shock stage S2; weatheringgrade W3. Specimens: type specimen, 7 g, and one thinsection, Vernad; main mass with anonymous owner.
Dar al Gani 1023 27°1.55′N, 16°23.27′ELibyaFound 1999 summerAchondrite (ureilite, polymict)
A stone of 149 g was found by an anonymous collector in theDar al Gani desert. Mineralogy and classification (H. Takeda,Chiba; T. Ishii and M. Ohtsuki, UTok): fragmental breccia,with lithic and mineral clasts embedded in a cataclastic matrixof predominantly ureilitic material. Lithic clasts andfragments include mafic ureilitic material (olivine 86 vol%and pyroxene 12 vol%), Na-rich plagioclase fragments and
Meteoritical Bulletin No. 87 A195
rare subrounded, dark brown Na-, K-rich glassy grain (SiO268 wt%, Al2O3 13.6 wt%, MgO 5.6 wt%, CaO 5.3 wt%, Na2O6.3 wt%, K2O 0.8 wt%). The pyroxene composition rangesfrom En79Wo6 to En62Wo4 and En59Wo31; olivine compositionranges from Fo90 to Fo75. The plagioclase composition rangesfrom An13Ab85 to An33Ab62. A slice of a lithic clast of 3.7 ×2.7 cm in size (sub-sample ,02; 6.89 g slice), is one of themost heavily shocked ureilites known. All mafic silicates areconverted into very fine grained materials with a granoblastictexture; carbonaceous vein materials are lost from many grainboundaries; glassy shock-vein materials are observed at someparts of the thin section. Olivine (80 vol%) is more abundantthan pyroxene (20%). Pyroxene composition ranges fromEn86Wo2 to En77Wo10 and En69Wo6; olivine compositionranges from Fo96 to Fo66. The stone is weathered, with abrownish color in hand specimen, but in thin section theweathering grade appears to be very low. Specimens: typespecimen, 20.75 g (including sample, 02), NSMT, one thinsection, Chiba; main mass with anonymous finder.
Dhofar 294-837, see Oman meteorites
Dhofar 304 18°24.2′N, 54°09.0′EOmanFound 2001 April 13Lunar meteorite (anorthositic impact melt breccia)
A brownish grey stone weighing 10 g was found in the Dhofarregion, Oman. Mineralogy and classification (M. Nazarov,Vernad; L. Taylor, UTenn): fusion crust is absent; meteorite isa clast-rich impact melt breccia; mineral fragments and lithicclasts are embedded in a very fine-grained impact-meltmatrix; the lithic clast population is dominated by impact meltbreccias; possible igneous rocks and granulites of mostlyanorthositic and gabbro-noritic compositions are rare.Mineral compositions are: feldspar, An93–99; orthopyroxene,Wo1–5En70–90; clinopyroxene, Wo6–42En40–50; olivine, Fo60–90(Fe/Mn 87 at). Accessory minerals are Ti-rich chromite, Cr-pleonaste, ilmenite (7–8 wt % MgO), troilite, and FeNi metal(7.8 wt% Ni; 0.6 wt% Co). The composition of the impact-melt matrix (wt%) is SiO2 = 45.0, TiO2 = 0.34, Al2O3 = 25.3,Cr2O3 = 0.17, FeO = 5.71, MnO = 0.12, MgO = 7.09, CaO =14.8, Na2O = 0.37, K2O = 0.04, P2O5 = 0.07. The meteorite ismoderately weathered; gypsum, calcite, celestite, barite, andFe hydroxides occur in cracks and holes. Dhofar 304 ispossibly paired with Dhofar 025 and Dhofar 301 because thestones were found nearby and they are similar in texture,mineral chemistry and degree of weathering. Specimens: typespecimens of 2 g, and a thin section, Vernad; main mass withanonymous finder.
Dhofar 305 19°19.8′N, 54°47.0′EOmanFound 2001 June 28 Lunar meteorite (anorthositic impact melt breccia)
A light-grey stone weighing 34.11 g was found in the Dhofarregion of Oman. Mineralogy and classification (M. Nazarov,Vernad; L. Taylor, UTenn): fusion crust is absent; themeteorite is an impact melt breccia consisting of mineralfragments and lithic clasts set within fine-grained, well-crystallized impact-melt matrix; clasts of impact meltbreccias are most common; granulites and possible igneousrocks are rare and have mainly anorthositic and troctoliticcompositions; orthopyroxenite clasts are present; feldspar,An87–98; orthopyroxene, Wo1–5En40–88; clinopyroxene; Wo6–
48En30–70; olivine, Fo44–90 (Fe/Mn = 94 at); accessory mineralsare Ti-rich chromite, Cr-pleonaste, ilmenite (1–8 wt% MgO),armalcolite, troilite, and FeNi metal (17–32 wt% Ni; 1.3–2.3wt% Co); composition of the impact-melt matrix is (wt%)SiO2 = 43.9, TiO2 = 0.16, Al2O3 = 28.5, Cr2O3 = 0.10, FeO =3.69, MnO = 0.07, MgO = 6.08, CaO = 15.9, Na2O = 0.36,K2O = 0.02, P2O5 = 0.04; the stone is moderately weathered;calcite, celestite, gypsum, and Fe hydroxides are present.Dhofar 305 is close to Dhofar 303, which was found nearby,in degree of weathering, mineral chemistry, and matrixcomposition. The meteorites may be paired, but they are verydifferent in texture. Pairing with Dhofar 081/280, 302, 306,and 307 is also possible. Specimens: type specimens of 7 g,and a thin section, Vernad; main mass with anonymous finder.
Dhofar 306 19°19.7′N, 54°47.1′EOmanFound 2001 June 29Lunar meteorite (anorthositic impact melt breccia)
A light-grey stone weighing 12.86 g was found in the Dhofarregion of Oman. Mineralogy and classification (M. Nazarov,Vernad; L. Taylor, UTenn): fusion crust is absent; themeteorite is an impact melt breccia consisting from mineralfragments and lithic clasts cemented by fine-grained impact-melt matrix; clast population is dominated by impact meltbreccias; granulites and cataclastic igneous rocks ofanorthositic, troctolitic and noritic compositions are present;devitrified glass fragments occur also; a characteristic featureof the lithic clast population is abundant high mg# lithologies;feldspar, An93–98; orthopyroxene, Wo1–5En50–90;clinopyroxene; Wo10–48En30–75, olivine, Fo48–94 (Fe/Mn = 87at); accessory minerals are Ti-rich chromite, Cr-pleonaste,ilmenite (3–8 wt% MgO), armalcolite, silica, Ca-phosphate,troilite, and FeNi metal (7–68 wt% Ni, 0.3–3.4 wt% Co);composition of the impact-melt matrix is SiO2 = 44.0, TiO2 =
A196 S. S. Russell et al.
0.15, Al2O3 = 27.2, Cr2O3 = 0.12, FeO = 4.00, MnO = 0.05,MgO = 7.55, CaO = 15.5, Na2O = 0.33, K2O = 0.04, P2O5 =0.07 (wt%); the stone is moderately weathered; celestite,calcite, and Fe hydroxides are present. Dhofar 306 is differentin texture and mineral chemistry from Dhofar 081/280, 302,303, 305, and 307, which were found nearby. However, themeteorites may be paired. Specimens: type specimen, 2.6 gand a thin section, Vernad; main mass with anonymous finder.
Dhofar 307 19°19.7′N, 54°46.9′EOmanFound 2001 April 14Lunar meteorite (anorthositic impact melt breccia)
A light-grey stone weighing 50 g was found in the Dhofarregion of Oman. Mineralogy and classification (M. Nazarov,Vernad; L. Taylor, UTenn): fusion crust is absent; the meteoriteis an impact melt breccia; fine-grained impact melt is mostabundant; mineral fragments and rare lithic clasts ofanorthositic, troctolitic, and gabbro-noritic compositions occurin the impact-melt matrix; the presence of rare dunite fragmentsis a characteristic feature of the meteorite; glass veins arecommon; feldspar, An89–98; orthopyroxene, Wo1–5En50–90;clinopyroxene; Wo6–48En40–75;, olivine, Fo38–94 (Fe/Mn = 92at); accessory minerals are Ti-rich chromite, Cr-pleonaste,ilmenite (2–6 wt % MgO), troilite, and FeNi metal (8–49 wt%Ni, 0.3–2.0 wt% Co); composition of the glass veins is SiO2 =43.8, TiO2 = 0.09, Al2O3 = 30.8, Cr2O3 = 0.09, FeO = 2.58, MnO= 0.05, MgO = 4.06, CaO = 17.3, Na2O = 0.36, K2O = 0.01,P2O5 = 0.02 (wt%); the stone is moderately weathered; calcite,gypsum, celestite, barite, and Fe hydroxides are present.Dhofar 307 is similar in texture and mineral chemistry toDhofar 305, found nearby. The meteorites are likely to bepaired. Pairing with Dhofar 081/280, 302, 303, and 306 is alsopossible. Specimens: type specimen, 10 g and thin section,Vernad; main mass with anonymous finder.
Dhofar 309 19°19.6′N, 54°47.3′EOmanFound 2002 January 14Lunar meteorite (anorthositic impact melt breccia)
A grey, partly fusion-crusted 81.3 g stone was found in theDhofar region of Oman. Classification and mineralogy (S.Demidova, Vernad; G. Kurat, NHMV): the meteorite is a clast-poor impact melt breccia; mineral fragments and lithic clastsare embedded in a matrix of devitrified glass. The clastpopulation is dominated by granulite clasts of mainlyanorthositic and troctolitic composition; fragments of possiblepristine rocks and single mineral fragments are less common.Mineral compositions: plagioclase An93–98Or0.1–0.4; olivineFo75–89 (atomic Fe/Mn ≈ 79); orthopyroxene En80–86Wo2–5;clinopyroxene En46–82Wo5–46; accessory minerals are Ti-poorchromite and Cr-pleonaste, ilmenite (4–9 wt% MgO), troilite,and FeNi metal. The composition (wt%) of the impact meltmatrix is MgO 6.2, CaO 16.1, Al2O3 29.1, SiO2 44.3, FeO 3.1;terrestrial weathering is not significant, although celestite and
calcite are present in cracks. Dhofar 309 is different in textureand mineral chemistry from Dhofar 081/280, 302, 303, 305,306, 310 found nearby. However, the meteorites may bepaired. Specimens: 16.5 g plus two thin sections, Vernad; mainmass with anonymous finder.
Dhofar 310 19°19.7′N, 54°47.1′EOmanFound 2002 January 15Lunar meteorite (anorthositic fragmental breccia)
A grey 10.8 g stone was found in the Dhofar region of Oman.Classification and mineralogy mineralogy (S. Demidova,Vernad; G. Kurat, NHMV): fusion crust is almost absent; themeteorite is a fragmental regolith breccia containingnumerous mineral fragments and clasts of feldspathic rocksembedded in a devitrified glassy matrix; clasts of granulitesand possible igneous rocks are abundant and have mainlyanorthositic and troctolitic-noritic compositions, impact meltbreccias and pyroxenitic clasts are also present; plagioclaseAn96–99Or0.1–0.2; olivine Fo44–86 (atomic Fe/Mn ≈ 79);orthopyroxene En59–88Wo1–5; clinopyroxene En33–77Wo5–47;accessory minerals are Ti-rich chromite, ulvöspinel,pleonaste, ilmenite (2–7 wt% MgO), armalcolite, silica,troilite, FeNi metal; composition of the impact melt matrix isMgO 4.8, CaO 18.5, Al2O3 29.1, SiO2 43.5, FeO 3.0 (wt%);the stone is moderately weathered: calcite and gypsum veinsand celestite inclusions are present. Dhofar 310 was foundclosely to Dhofar 302, 303, 305, 306, 307, 081/280, and maybe paired with some of these meteorites. Specimens: 2.5 gplus a thin section, Vernad; main mass with anonymousfinder.
Dhofar 311 19°19.6′N, 54°47.0′EOmanFound 2001 April 14Lunar meteorite (anorthositic impact melt breccia)
A small light-grey stone weighing 4 g was found in theDhofar region of Oman. Mineralogy and classification (S.Demidova, Vernad; L. Taylor, UTenn): fusion crust is absent;mineral fragments and rounded lithic clasts occur within afine-grained to cryptocrystalline impact-melt matrix; thelithic clast population comprises impact-melt breccias, aswell as cataclastic granulitic and igneous rocks of anorthositicand troctolitic compositions; clasts of impact-melt brecciasare most abundant and typically show breccia-in-brecciatextures; feldspar, An95–98; orthopyroxene, Wo2–5En45–85;clinopyroxene; Wo6–45En40–74, olivine, Fo57–88 (Fe/Mn ≈ 91at); accessory minerals include: Cr-pleonaste, Al-chromite,troilite, and FeNi metal (3–27 wt% Ni; 0.2–1.9 wt% Co); thestone is moderately weathered; calcite, gypsum, celestite,barite, and Fe hydroxides are present. Dho 311 was found 25m from Dho 280, but the meteorites are very different inweathering grade and lithology. Dho 311 is most similar intexture and mineral chemistry to Dho 303 found nearby. Themeteorites may be paired. Pairing with Dho 302, 305, 306,
Meteoritical Bulletin No. 87 A197
307, 309, 310, 730, and 731 is also possible. Specimens: typespecimen of 1.7 g plus a thin section, Vernad; main mass withanonymous finder.
Dhofar 490 18°43.00′N, 54°27.00′EOmanFound 2001 March 17Lunar meteorite (anorthositic fragmental breccia)
A dark grey, crusted stone weighing 34.05 g was found in theDhofar region of Oman. Classification and mineralogy (A.Greshake, MNB; M. Kurz, Kurz): meteorite is an anorthositicfragmental breccia consisting of clasts of various lithologiesembedded into a glassy, partly devitrified fine-grained matrix;the clast size is generally below 3 mm; vesicles are abundant;feldspar: An96.0–99.3; pyroxene: Fs11.5–35.7Wo8.2–44.9 andolivine: Fa30.6–50.0; augites dominate over Ca-poor pyroxenesand often contain pigeonite exsolution lamellae; accessoryphases are Fe-Ni metal and ilmenite; crystalline fragmentsinclude microporphyritic impact melt breccias, intersertalimpact melt clasts, gabbroic anorthosites, and large feldspar;no mare basalt clasts and no glass spherules have beenidentified; feldspar generally shows pronounced undulatoryextinction and sometimes mosaicism indicating strong shockmetamorphism; the meteorite is moderately weathered;gypsum, celestite and calcite occur in cracks and holes; Dho490 may be paired with Dho 280, since they were foundnearby and have similar mineralogical characteristics.Specimens: 7 g and one thin section, MNB; main mass withanonymous finder.
Dhofar 500 18°23.2′N, 54°12.2′EOmanFound 2000 January 24Achondrite (ungrouped)
A stone weighing 116 g was found in the Dhofar region ofOman. Mineralogy and classification (C. Lorenz and M.Ivanova, Vernad.): the rock is a metabreccia and consists of atleast three different lithologies: pyroxene-feldspar, pyroxene-olivine and pyroxene-olivine-feldspar. In texture thelithologies vary from medium to coarse-grained, poikiloblasticto equigranular. Mineral chemistry: olivine Fa4.8; CaO 0.13wt%, Cr2O3 0.42 wt%; orthopyroxene is En95Wo2, Fe/Mn ratiois 6 (at); feldspar is An13–34. Olivine and pyroxene are of thesame compositions in the lithologies. The minor phases are Ca-rich augite En52Wo44; Cr-rich troilite (up to 3.11 wt% Cr),chromite and rare minute grains of Fe-Ni metal. Weatheringgrade is W3. The oxygen isotope composition (R. N. Clayton,UChi): δ18O = +9.21‰; δ17O = +4.29‰; ∆17O = –0.49‰, is notin the range of known meteorite groups but close to thewinonaite-IAB-IIICD trend and ureilites. Mineralogically themeteorite may have some links to primitive achondrites butcompositions of olivine and troilite are close to those in
polymict ureilites. However, this meteorite lacks a carbon-richmatrix. Specimens: a type specimen of 23.5 g and a thin section,Vernad; main mass with anonymous finder.
Dhofar 535 19°20.0′N, 54°47.7′EOmanFound 2000 January 16Chondrite (ungrouped)
Many stones weighing a total of 204 g were found in the Dhofarregion of Oman. Mineralogy and classification (M. Ivanova,Vernad; L. Taylor, UTenn): the meteorite consists ofchondrules, 0.08–3.2 mm in diameter, (0.86 mm in average) ofdifferent types, PO, POP, BO, RP, CC, and their fragmentsembedded in a fine-grained matrix. Chondrule/matrix ratio is1.1. Olivine and low-Ca pyroxene have large compositionalranges: olivine has Fa1–50, CaO 0.2 wt%; Al2O3 0.06 wt%,Cr2O3 0.09 wt%, PMD of Fa 42%; low-Ca pyroxene is Wo2–
3.5En53–95; chondrules contain glassy mesostasis. Accessoryminerals include: pigeonite, chromite, troilite, rare hydroxides,and rare FeNi metal (Ni 5 wt%; Co 0.4 wt%).Thermoluminescence studies (A. I. Ivliev, Vernad) indicatepetrologic type 3.2/3.3. The meteorite is heavily weathered,and some silicates are altered. Weathering grade is W5; shockstage is S1. Based on the very low abundance of FeNi metal andhydroxides, Dho 535 could belong to either the LL or Rchondrite groups but with very abundant matrix. The averagesize of chondrules is consistent with LL chondrites. Ahistogram showing the distribution of olivine is similar tounequilibrated ordinary chondrites. FeNi metal is mostlykamacite, typical for H chondrites and unusual for Rchondrites. Sulfide assemblages and chromite chemistry arealso unusual for R chondrites. The absence of refractory objectsand olivine chemistry distinguish Dho 535 from C3 chondrites.Oxygen isotope composition (R. N. Clayton, UChi): δ18O =+8.56‰; δ17O = +4.96‰, ∆17Ο = 4.51‰ is unusual for anychondrite type. Specimens: type specimen of 46.8 g and thinsection, Vernad; main mass with anonymous finder.
Dhofar 622 19°13.672′N, 54°51.221′EOmanFound 2001 January 15Ordinary chondrite (H4, anomalous)
The sample (working and find number: OM 1.01–24) wasfound as a single fragment of 60 g in the Dhofar region.Mineralogy and classification (A. Bischoff and A. Sokol,Mün): Although the chemical analyses of olivine (Fa18.5) andpyroxene (Fs16.8 ± 1.2) are similar to those of H-chondrites, thisrock is not a typical H-chondrite, and consists of much morematrix than typical ordinary chondrites. R.N. Clayton (UChi)states that Dhofar 622 “has a lower ∆17O than any ordinarychondrite we have measured (typical H-chondrites have ∆17O= +0.7).” The oxygen isotope data are: δ18O = +5.15; δ17O =
A198 S. S. Russell et al.
+2.92; ∆17O = +0.25‰. The meteorite is very weakly shocked(S2) and moderately to heavily weathered (W3-4).Specimens: main mass with anonymous finder; thin sectionsand type specimen, 12 g, Mün.
Dhofar 700 19°18.5′N, 54°33.1′EOmanFound 2002 November 15Achondrite (diogenite)
Twelve dark-grey stones totalling 2770 g were found in theDhofar region of Oman. Classification and mineralogy (S.Demidova, Vernad; G. Kurat, NHMV): fusion crust is absent.The meteorite has an equigranular texture, and consistsdominantly of orthopyroxene (Wo2.5–7En62–71; Fe/Mn ≈ 25at.). Accessory minerals are clinopyroxene Wo8–25En55–66,olivine Fo63–68, plagioclase An89–95, silica, chromite, troiliteand FeNi metal (0.2–3.8 wt% Ni, 0.3–0.8 wt% Co); terrestrialweathering is not significant; rare Fe hydroxide is present.The mafic silicates in Dho 700 have the low mg# that is acharacteristic feature of diogenites. Specimens: 350 g plusthin section, Vernad; main mass with anonymous finder.
Dhofar 730 19°19.5′N, 54°47.5′EOmanFound 2002 November 9Lunar meteorite (anorthositic impact melt breccia)
A light-grey stone weighing 108 g was found in the Dhofarregion of Oman. Mineralogy and classification (M. Nazarov,Vernad; L. Taylor, UTenn): fusion crust is absent; lithic clastsand mineral fragments set within a fine-grained impact meltmatrix; the lithic clast population is dominated by impact-meltbreccias and cataclastic granulitic and igneous rocks ofanorthositic and troctolitic compositions; rare dunite fragmentsare present; feldspar, An86–98; orthopyroxene, Wo2–4En56–85;clinopyroxene; Wo6–46En14–71; olivine, Fo55–92 (Fe/Mn ≈ 86 at).Accessory minerals include: chromite, Cr-pleonaste,armalcolite, ilmenite, silica, troilite, and FeNi metal (6–48 wt%Ni; 1–2.4 wt% Co); the stone is moderately weathered; calcite,gypsum, celestite, barite, and Fe hydroxides are present. Themeteorite may be paired with Dho 302, 303, 305, 306, 307, 309,310, 311, and 731 found nearby. Specimens: type specimens of22 g, and a thin section, Vernad; main mass with anonymousfinder.
Dhofar 731 19°20.0′N, 54°47.7′EOmanFound 2002 November 11Lunar meteorite (anorthositic impact melt breccia)
A light-grey stone weighing 36 g was found in the Dhofarregion of Oman. Mineralogy and classification (M. Nazarov,Vernad; L. Taylor, UTenn): fusion crust is absent; lithic clastsand mineral fragments occur within a fine-grained impact melt
matrix; the lithic clast population consists mainly of impactmelt breccias of anorthositic and troctolitic compositions;feldspar, An95–97; orthopyroxene, Wo2–5En53–85;clinopyroxene; Wo6–45En30–81, olivine, Fo52–87 (Fe/Mn ≈ 84 at).Accessory minerals include: Cr-pleonaste, chromite, ilmenite,troilite and FeNi metal (0.5–66 wt% Ni; 0.2–2 wt% Co); Cr-pleonast is most common; the stone is moderately weathered;calcite, gypsum, celestite, barite, smectite, and Fe hydroxidesare present. Dho 731 may be paired with Dho 302, 303, 305,306, 307, 309, 310, 311, and 730. Specimens: type specimens of7.5 g, and a thin section, Vernad; main mass with anonymousfinder.
Dhofar 732 19°24.3′N, 54°34.7′EOmanFound 2002 November 15Achondrite (ungrouped, orthopyroxene-rich)
A small brownish stone weighing 17 g was found in theDhofar region of Oman. Mineralogy and classification (S.Demidova, Vernad; G. Kurat, NHMV): fusion crust is absent.The coarse-grained rock consists mainly of lath-shaped,zoned orthopyroxene (Wo0.4–5En82–96) and interstitialmesostasis (5–10%); minor rounded olivine (Fo93–95) grainsare present; the mesostasis consists of clinopyroxene (Wo12–
40En54–81) and silica set within Ca, Al-rich, Na-poor glass;accessories are chromite, troilite, and FeNi metal (1.6–8.1wt% Ni; 0.3–0.6 wt% Co); Fe/Mn of orthopyroxene (5–17 at.)is very low and clearly distinguishes the meteorite fromdiogenites; the stone is moderately weathered; there areabundant Fe hydroxide inclusions and holes in the rock.Oxygen isotope composition (R. N. Clayton, UChi): δ17O =+2.77‰, δ18O = +6.64‰ indicate a possible relation of themeteorite with silicate inclusions from IAB irons, winonaitesor ureilites. Specimens: type specimens of 3.5 g, and a thinsection, Vernad; main mass with anonymous finder.
Dhofar 733 18°35.3′N, 54°13.8′EOmanFound 2002 November 12Lunar meteorite (anorthositic granulitic breccia)
A brownish grey stone weighing 98 g was found in the Dhofarregion of Oman. Mineralogy and classification (S. Demidova,Vernad; G. Kurat, NHMV): fusion crust is absent; the rockcontains relics of mineral and lithic clasts and showsgranoblastic or poikiloblastic textures; anorthositic, troctoliticand gabbro-noritic lithologies are present. Mineralcompositions: feldspar, An89–96; orthopyroxene, Wo4–5En73–76;clinopyroxene, Wo36–40En48–52; olivine, Fo71–76 (Fe/Mn ≈ 87at). Accessory minerals are armalcolite, ilmenite, Al-chromite,Ca-phosphate, troilite, and FeNi metal (31–43 wt% Ni; 1.3–1.7wt% Co); lath-shaped armalcolite is most common; the stone ismoderately weathered; smectite, gypsum, and Fe hydroxides
Meteoritical Bulletin No. 87 A199
are present. Dho 733 was found far away from other lunarstones collected in the Dhofar region and has a distinctlydifferent texture. It is probably not paired with any other Dhofarlunar finds known so far. Specimens: type specimens of 20 g,and a thin section, Vernad; main mass with anonymous finder.
Dhofar 735 19°04.1′N, 54°46.8′EOmanFound 2002 November 9Carbonaceous chondrite (CM2)
Two stones weighing 304 g and 77 g were found on November2002 in the Dhofar region of Oman. Mineralogy andclassification (M. Ivanova, Vernad; L. Taylor, UTenn): fusioncrust is present, the meteorite consists of altered chondrules,sometimes with a halo around, olivine aggregates, andfragments of matrix material set within a phyllosilicate matrix.Olivine, Fa0.3–22, CaO 0.35 wt%, Cr2O3 0.28 wt%. Noorthopyroxene is present. Refractory inclusions are rare andconsist of anorthite, Al-rich pyroxene and forsterite. The minorphases are kamacite, taenite, and tetrataenite (Ni, up to 60wt%), troilite, rare pentlandite, chromite, Mg-ilmenite,schreibersite, and Ca-carbonates. The matrix is composedmainly of serpentine. Tochilinite was not found. Weatheringgrade is W1. Oxygen isotope composition is in the range ofmetamorphosed CM chondrites (R. N. Clayton, UChi): δ18O =+21.99‰; δ17O = +10.85‰; ∆17O = –0.58‰. Specimens: atype specimen of 58.8 g and a thin section, Vernad; main masswith anonymous finder.
Dhofar 836 18°20.92′N, 54°12.84′EOmanFound 2000 August 15Achondrite (ureilite)
A single stone weighing 995 g, and split into two pieces wasfound by an anonymous finder in the Dhofar region of Oman.Mineralogy and classification (H. Takeda, Chiba; T. Ishii andM. Ohtsuki, UTok.): medium-grained (1–2 mm), equigranularolivine (Fo79 core; Fo90 rim) and pigeonite (Ca10Mg74Fe16 toCa11Mg71Fe19). Carbonaceous matter occurs as narrow,intergranular veins. Weakly shocked (S1), with raremosaicism in olivine. The sample is weathered to brownishcolor in hand specimen, W1. Dho 836 was found only 6 kmNW of Dho 837, but the two specimens differ in compositionand texture, and so may not be paired. Specimens: typespecimen 20.2 g NSMT; thin section, Chiba; main mass withanonymous finder.
Dhofar 837 19°35.30′N, 54°57.10′EOmanFound 2000 springAchondrite (ureilite)
A single stone weighing 900.1 g, and split into two pieces wasfound by an anonymous finder in August 2000 in the Dhofarregion of Oman. Mineralogy and classification (H. Takeda,
Chiba; T. Ishii and M. Ohtsuki, UTok): A few medium-grained olivine and pigeonite grains (up to 2.1 × 1.5 mm insize) are set in a texture of smaller grained minerals withcarbonaceous material and fine metal veins at grainboundaries. Olivine grains (75 vol%) are more abundant thanpigeonite (20%). The metal veins are less than 5 vol%. Thepigeonite composition Ca5Mg76Fe19 is uniform and the Fovalues of olivine range from 78 to 79. Weakly shocked (S1-2).The sample is weathered to brownish color in hand specimen,W1. Dho 837 was found only 6 km SE of Dho 836, but thetwo specimens differ in composition and texture, and so maynot be paired. Dho 837 has some textural similarities to Dho295, but as the two specimens have very different Fe atomic%, and were found around 113 km apart, they are notnecessarily paired. Specimens: type specimen 20.8 g NSMT;thin sections, Chiba, KyuU; main mass with anonymousfinder.
Elbert 39°14.8′N, 104°35.29′WElbert County, Colorado, USAFell 1998 January 11Ordinary chondrite (LL6)
A fireball was observed over Elbert County and reported inseveral local newspapers. A single 680.5 g stone was found ina field on 2000 March 4, by Dustin Riffel, a five-year-old boy,while walking with his mother on their family property.Classification (A. Rubin, UCLA): Olivine, Fa30.5 ± 0.44, shockstage S2, weathering grade W0. Specimens: type specimen,19 g, UCLA; main mass with Riffel family.
Finger Ridge (FIN), see Antarctic ANSMET meteorites
Fortuna 35°08′S, 65°22′WFortuna, Province San Luis, ArgentinaFound 1998 May 27Achondrite (winonaite)
A single 312 g stone of elongated form partly covered byfusion crust was found on 1998 May 27 near the village ofFortuna, Province San Luis, Argentina. Classification andmineralogy (A. Greshake, MNB; M. Kurz, Kurz): themeteorite exhibits an equigranular texture with abundanttriple junctions, the average grain size is about 115 µm; itcontains low-Ca pyroxene, Ca-pyroxene, olivine, plagioclase,Fe,Ni metal, and troilite with low-Ca pyroxene being thedominant silicate phase. The composition of the silicates isquite reduced: low-Ca pyroxene, Fs5.5–6.7Wo1.1–1.7; Ca-pyroxene, Fs2.4–2.9Wo45.6–46.5; olivine, Fa4.3–5.1; plagioclase,An14.5–16. Fe, Ni metal and troilite veins up to 1.5 mm wideand extending over several cm are prominent; no relictchondrules were found. Oxygen isotope composition (R.Clayton and T. Mayeda, UChi): δ17O = +1.61‰, δ18O =+4.68‰; shock stage S2; degree of weathering W0/1.Specimens: main mass with anonymous finder; typespecimen 23 g plus one polished thin section MNB.
A200 S. S. Russell et al.
Frontier Mountain (FRO), see Antarctic PNRA meteorites
Frontier Mountain 01012 72°58′16′′S, 160°20′02′′EAntarcticaFound 2001 December 9Achondrite (ureilite)
A weathered, 30 % fusion crusted meteorite fragment of 19.2g was recovered. Mineralogy and classification (R. Carampinand A. M. Fioretti, UPad): FRO 01012 shows mosaicizedtexture and consists of olivine Fo78 (with Fo94 reduced rims)and pigeonite En75Wo7 with interstitial carbonaceousmaterials. Abundant diamond is present as small grainswithin carbonaceous material, as revealed by itscathodoluminescence (strong blue-red dispersion) under thebeam of the electron microprobe. Olivine shows a very strongmosaicism, and pigeonite is polysynthetically twinnedindicating shock stage S5. Main mass, type specimen, thinsection, MNA-SI.
Frontier Mountain 01088 72°57′08′′S, 160°27′19′′EAntarcticaFound 2001 December 16Achondrite (ureilite)
A crusted stone of 11.1 g was recovered. Mineralogy andclassification (R. Carampin and A. M. Fioretti, UPad): FRO01088 shows poikilitic texture and consists of olivine Fo75,pigeonite En76Wo10, and interstitial carbonaceous materialswith oriented graphite lamellae. The pigeonite includesrounded crystals of olivine and flakes of graphite. Abundant,small diamond grains occur in the carbonaceous material, asrevealed by its cathodoluminescence (strong blue-reddispersion) under the beam of the electron microprobe. Mostolivine shows a very strong mosaicism, and locally hints ofincipient solid-state recrystallization, corresponding to ashock stage S5/6. Secondary reduction has affected mostsilicate crystals. Weathering is minor, with thin limonite veinsin fractures. Main mass, type specimen, thin section, MNA-SI.
Frontier Mountain 01089 72°57′08′′S, 160°27′20′′EAntarcticaFound 2001 December 16Achondrite (ureilite)
A weathered stony fragment of 2.1 g was recovered.Mineralogy and classification (R. Carampin and A. M.Fioretti, UPad): FRO 01089 shows typical texture andconsists of olivine Fo77 (with Fo85 reduced rims), pigeoniteEn70 Wo13 and interstitial carbonaceous materials. Silicatemineral mode is olivine 91 vol% and pigeonite 9 vol%.Weathering is minor, with thin limonite veins in fractures.Main mass, type specimen, thin section, MNA-SI.
Frontier Mountain 01147 72°58′25′′S, 160°20′17′′EAntarcticaFound 2001 December 21Achondrite (ureilite)
A weathered, stony fragment of 0.5 g was recovered.Mineralogy and classification (A. Burroni and L. Folco,MNA-SI): Olivine and pigeonite ureilite with typical texture(average grain size 1 mm). Mafic silicates showhomogeneous core compositions (olivine Fo80; pigeoniteEn75Wo8) and wide, strongly reduced rims. Graphite formslarge intergranular flakes up to 1 mm in maximum elongation.Undulose extinction, planar fractures and kinking in botholivine and pigeonite indicate moderate shock deformation.Main mass, type specimen, thin section, MNA-SI.
Gasseltepaoua 14°9.05′N, 2°2.50′WSoum, Djibo, Burkina FasoFell 2000 August 22Ordinary chondrite (H5)
A fist-sized stone (weight unknown) was seen to fall byfarmers working outdoors in the village of Gasseltepaoua,northern Burkina Faso. Mineralogy and classification (M.Bourot-Denise, MNHNP): Ordinary chondrite, H5 (Fa19.2Fs17.1), S4, W1. Specimens: type specimen, 16.7 g, MNHNP;main mass, Museum of Bureau of Mines and Geology ofBurkina Faso in Ouagadougou.
Great Sand Sea 019, see Saharan meteorites from Egypt
Hammadah al Hamra 291–327, see Saharan meteoritesfrom Libya
Hammadah al Hamra 294, correctionThe latitude of the place of find was listed incorrectly inMeteoritical Bulletin 86 (2002). The correct latitude is 29°06′N.
Hammadah al Hamra 298, correctionThe latitude of the place of find was listed incorrectly inMeteoritical Bulletin 86 (2002). The correct latitude is 29°05′N.
Hammadah al Hamra 317 11°35.58′N, 29°21.06′ELibyaFound 2001 springEnstatite chondrite (EL4)
Two dark brown stones, a larger one of 103 g and a smallerone of 2 g were found in the Hammadah al Hamra region.Classification and mineralogy (G. Pratesi, V. Moggi Cecchi,MSP): the partly fusion-crusted stone is shield-shaped; well-
Meteoritical Bulletin No. 87 A201
defined chondrules and 50 µm sized enstatite crystals indicatepetrologic type 4. Major phases are enstatite (En98.5Wo0.9),kamacite (Fe = 90.46, Ni = 7.51, Si = 0.57, P = 0.53, Co =0.47 wt%) and troilite; other minor phases are diopside(En52.91Wo46.85) and plagioclase (An26.60) in very small grains(<5 µm). Neither niningerite nor alabandite was found. Theplagioclase composition, as well as the presence of diopside,is unusual compared with other known EL chondrites. Insidethe chondrules, which have an average size ranging from 600to 1200 µm, very small rounded grains containing a calciumchloride phase (1–3 µm size) have been observed. Based ontexture, mineralogy and chemistry (mainly An content ofplagioclase >13 mol% and Si content of kamacite <1.9 wt%;Keil, 1968; Zhang et al., 1995) the meteorite is classified as anEL4 chondrite. Terrestrial weathering grade is rather low(W1); optical features (undulatory extinction of enstatite)indicate that the sample is weakly shocked (S3). Specimens:main mass, type specimen and thin section, MSP.
Harper Dry Lake 001–008, see Americas meteorite finds
Hart Camp, classificationHart Camp (Lamb County, Texas: found 1970) has now beenclassified as an H6 chondrite (olivine, mean Fa20.8; low-Capyroxene, mean Fs18.2Wo1.5). Classification: R. Jones, UNM.
Hiroshima 34°27′N, 132°23′EJapanFell 2003 February 1–3Ordinary chondrite (H5)
A 414 g stone was discovered on February 4, 2003 in thedelivery center of a pharmacutical company by workerssearching for the cause of a leaking roof. The meteoritepenetrated the steel sheet roofing and plasterboard and hit aroller conveyor belt then fell to the floor. The fall must haveoccurred after the center closed on the evening of February 1.Several people in Hiroshima observed a fireball around 22:30on February 1. Classification (A. Okada, RIKEN; S. Yoneda,NSM): olivine, Fa17.0–18.7; pyroxene Fs15.7–18.6 CaO 0.56–1.01%. Noble gas analysis (J. Park, N. Ebisawa, and K.Nagao, UTok): 21Ne exposure age about 90 Myr. Specimens:main mass in possession of the finder and on long-term loan atthe Hiroshima City Childrens Culture and Science Center;type specimen, 27 g, NSM.
Jalu, see Saharan meteorites from Libya
Jiddat al Harasis 022–073, see Oman meteorites
Jiddat al Harasis 026, reclassificationOn the basis of a TL sensitivity of 0.0046–0.01 (A. I. Ivliev,Vernad), JaH 026 is assigned to metamorphic subtype L3.1.
Jiddat Arkad, see Oman meteorites
Khatiyah 25.43°N, 50.78°EDukhan, QatarFound 2000 MayOrdinary chondrite (H5)
A 1.5 kg single stone was found by Colin Wade while out witha running club. Classification (R. Jones, UNM): olivine, Fa18.0
± 0.7; pyroxene, Fs15.9 ± 0.2Wo0.9 ± 0.2. Shock stage, S3.Specimens: type specimens 20 g NHM, ~13.6 g and a thinsection, UNM; main mass C. Wade.
Kilabo 12°46′N, 9°48′ENigeriaFell 2002 July 21, 19:30 hrs local timeOrdinary chondrite (LL6)
Mr. Mallam Yahava Muhammad of Hadejia, Nigeria,observed a brilliant fireball moving south to north. Two louddetonations were heard several minutes later. Mr. MallamAudu and several neighbours in Kilabo heard the stone falland later recovered it. The meteorite was found in the cratermeasuring 35 cm wide by 20 cm deep in sandy soil. Themeteorite had fragmented on impact into many pieces, thelargest of which was 2.2 kg. A total weight of ~19 kg wasrecovered. Stones were recovered in five villages in theregion, with the largest piece in Kilabo. Classification (P.Sipiera, Harper; M. Zolensky, JSC): olivine, Fa31.1, CaO<0.09, predominantly <0.05. Low Ca-pyroxene, Fs27.1 PMD =0.02. Abundant coarse-grained plagioclase, mainly An84Or5,ranges from An61Or25 to An86Or3. Coarse-grained diopsideand troilite are abundant; pentlandite is a minor phase. Themeteorite is brecciated, with thick black shock veins present.Shock stage is S3, weathering grade is W0. Specimens: typespecimen, 30 g, PSF; main mass Mr Avraham Wysznski,SIMAT USA Inc., New York, NY, USA.
Kilbabo, synonym for Kilabo
Kufra, see Saharan meteorite from Libya
Meteorite Hills (MET), see Antarctic ANSMET meteorites
Milton 40°17′15′′N, 95°22′36′′WAtchison County, Missouri, USAFound 2000 OctoberPallasite
A single mass of 2040 g was found in a bean field by Ben Rogersand Gary Wennihan. Initial identification was made by C. Rohsand J. Reese at Northwest Missouri State University.Classification and mineralogy (R. Jones, UNM; J. Wasson,UCLA): Small, angular olivines (73 vol%), mean Fa17.2; molarFe/Mn = 123; metal composition, Ni = 151 mg/g, Co, 9.6 mg/g,
A202 S. S. Russell et al.
Ga, 15.3 µg/g; As, 10.1 µg/g; Ir, 50.4 µg/g, Au, 1.16 µg/g. Meanoxygen isotope ratios of olivine (T. Larson and Z. Sharp,UNM): δ18O = +0.52 ‰, δ17O = –2.87‰. Specimens: mainmass with finder; type specimen, 69.7 g, plus polished thinsection, UNM; 73.5 g at Northwest Missouri State University.
Mount Crean (CRE), see Antarctic ANSMET meteorites
Myrtle Springs 30° 27′13.8′′S, 137°59′24.6′′ESouth AustraliaFound 2002 July 11Ordinary chondrite (H4)
A single stone of 52.99 g was found by Mr. Don McCollwhile searching for tektites. Classification (M. ZbikUniversity of South Australia; A. Pring SAM): olivine, Fa19.6 ±
0.6; pyroxene, Fs18.2 ± 0.7Wo1.3 ± 0.8. Shock stage S2, themeteorite contains extensive iron oxide staining. See Zbikand Pring (2003). Specimens: Main mass and type specimen,SAM.
Neuschwanstein 47°31.5′N, 10°48.5′EBavaria, GermanyFell 2002 April 6; 20:20 hrs (UT)Enstatite chondrite (EL6)
A brilliant fireball, shaking the ground and rattling windows,was reported by many eyewitnesses in Austria and Germany.The fall circumstances were well documented by theEuropean Fireball Network (EFN). Reduction of the EFNphotographs allowed calculation of the orbit and impact area(Spurny et al. 2002) which ultimately led to the recovery of asingle stone of 1.75 kg on July 14, 2002. Gammaspectrometry (G. Heusser and H. Neder, MPI-K) of the stoneindicates a small pre-atmospheric radius of less than 20 cmmainly from the low 60Co activity of 1.2 ± 0.5 dpm/kg. Short-lived radionuclides strongly indicate that the recoveredmeteorite was indeed the object that fell on the above date.Classification and mineralogy (A. Bischoff, Mün and J.Zipfel, MPI): the meteorite has a metamorphic texture with asmall number of chondrule relics. Major phases are enstatite(FeO <0.1 wt%), plagioclase (Ab82), and metal (~1.5 wt% Si).Large crystals of sinoite (up to 200 µm) and graphite (up to700 × 200 µm) are present. Additional phases so far observedare schreibersite ((Fe,Ni)3P), troilite (FeS), oldhamite (CaS),daubreelite (FeCr2S4), alabandite, ((Mn,Fe)S), and an SiO2-phase (containing 1–2 wt% Al2O3). Bulk chemistry:abundances of moderately volatile lithophile elements aretypical for EL chondrites, low Mn/Mg = 0.010 and Na/Mg =0.045, and low Zn concentration (Zn <20 ppm); highconcentrations of siderophile elements, e.g., Ni = 1.94% andIr = 0.76 ppm, reflect higher than usual metal contents for ELchondrites. Based on texture, mineralogy and chemistry themeteorite is classified as an EL6 chondrite. Optical featuresindicate that the rock is very weakly shocked (S2). Theresidence time of about three months on the ground resultedin the first signs of weathering (W0/1). The exposure age is
~48 Ma; trapped subsolar noble gases are present (L. Frankeand L. Schultz, MPI). Specimens: type specimen, 20 g, MPI;thin sections: Mün; main mass, unknown.
Northwest Africa 167–1814, see Saharan meteorites fromMorocco and surrounding countries
Northwest Africa 998Algeria or MoroccoPurchased 2001 SeptemberMartian meteorite (nakhlite)
A. and G. Hupé (Hupé) purchased, from dealers at the TucsonGem and Mineral Show in 2002 February, the main massfrom a 456 g stone that had been acquired at an unspecifiedsite in western Algeria or eastern Morocco in 2001September. Dimensions before cutting: 72 mm by 65 mm by48 mm. Classification and mineralogy (A. Irving and S.Kuehner, UWS): a friable, dark green rock with minor orange-brown alteration products that probably are of pre-terrestrialorigin. It is composed mainly of subhedral, olive-green,complexly zoned subcalcic augite (Fs22Wo39) withsubordinate yellow olivine (Fa64), orthopyroxene (Fs49Wo4),interstitial plagioclase (Ab61Or4 containing 0.1 wt% SrO, andexhibiting normal birefringence), titanomagnetite,chlorapatite and pyrrhotite. The overall texture is that of ahypabyssal, adcumulate igneous rock, and the apparentcrystallization sequence is olivine, orthopyroxene,titanomagnetite, augite, apatite, plagioclase. There is a weakpreferred orientation of prismatic pyroxene crystals, many ofwhich have very distinctive zoning, with cores of augitesurrounded by irregular, inverted pigeonite rims (nowconsisting of orthopyroxene with fine augite lamellae). Trainsof tiny melt inclusions are present along healed fractureswithin pyroxene; microprobe study confirms that most ofthese are K-Na-Al-bearing silicate glass, but some areintergrowths of glass and Fe-bearing carbonate, which mayrepresent quenched immiscible silicate-carbonate liquids.Symplectitic intergrowths of titanomagnetite and low-Capyroxene are present at grain boundaries between large,discrete olivine and titanomagnetite grains, but are notpresent around chromian titanomagnetite inclusions withinolivine. These observations suggest that a pre-terrestrialoxidation process produced the symplectites, and involvedhigh temperature, deuteric fluid infiltration along grainboundaries; such fluids also may have produced the irregularpigeonitic rims on augite crystals. Secondary (probably pre-terrestrial) ankeritic carbonate, K-feldspar (some Fe-bearing),serpentine (?), calcite and a Ca sulfate are present on grainboundaries and within cracks in augite. Oxygen isotopecomposition (D. Rumble, CIW): replicate analyses of acid-washed augite by laser fluorination gave δ18O = +3.9 ± 0.2‰;δ17O = +2.4 ± 0.1‰; ∆17O = +0.30 ± 0.02‰. Specimens: typespecimens, 20 g, UWS, 20 g, FMNH, and two polished thinsections, UWS; main mass, Hupé.
Meteoritical Bulletin No. 87 A203
Northwest Africa 1109MoroccoPurchased 2001 October/DecemberAchondrite (eucrite, polymict)
A. and G. Hupé (Hupé) purchased four stones totalling 2.54kg from a Moroccan dealer in 2001 October and December,but the total weight of this material including that held byother collectors is estimated to be nearly 6 kg. The stonesshow distinctive white and grey mineral and lithic clasts in alight tan matrix Classification and mineralogy (A. Irving andS. Kuehner, UWS): polycrystalline clasts include basalticeucrite (ophitic texture, variable grain size, mainly anorthite +pigeonite Wo16Fs57, FeO/MnO = 30); cumulate eucrite(coarse grained, equigranular, mainly anorthite + exsolvedpigeonite with accessory silica); rare eucritic breccias anddistinctive ferroan intergrowths (fayalite + hedenbergite +silica ± troilite). Mineral clasts include homogeneouspigeonite grains (Wo15Fs31, FeO/MnO = 26), pigeonite grainswith clinopyroxene exsolution lamellae (FeO/MnO = 30–33),anorthitic plagioclase (Ab6-Ab10) and a silica polymorph.Accessory minerals in clasts and matrix include ilmenite, Femetal, chromite, baddeleyite and apatite. Specimens: typespecimen, 20 g, and four polished thin sections, UWS; mainmass, Hupé.
Northwest Africa 1195MoroccoPurchased 2002 March/April Martian meteorite (basaltic shergottite)
A. and G. Hupé (Hupé) purchased a 50 g fragment of a brokenstone with a distinctive, thin weathering rind collected bynomads near Safsaf, Morocco in 2002 March, andsubsequently purchased the remainder of the same elongatedstone (total weight 315 g). Dimensions of the reassembledstone are 133 mm × 43 mm × 37 mm. Classification andmineralogy (A. Irving and S. Kuehner, UWS): olivinemegacrysts (up to 4 mm) are set in a groundmass of low-Capyroxene and maskelynite (Ab37Or0.5 to Ab41Or0.7) withminor Ti-chromite, pyrrhotite, ilmenite and Mg-bearingmerrillite. The euhedral to subhedral shapes of most of theolivine grains suggest that they are phenocrysts rather thanxenocrysts. Olivine exhibits strong compositional zoning(cores Fa19, FeO/MnO = 54; rims Fa40, FeO/MnO = 62) andcontains abundant inclusions of chromite, clinopyroxene,orthopyroxene, and pyrrhotite. The groundmass low-Capyroxenes are zoned from cores of pigeonite (Wo7Fs26, FeO/MnO = 37.1) or, less commonly, orthopyroxene (Wo4Fs23,FeO/MnO = 37.0) to rims of more Fe-rich pigeonite(Wo12Fs33, FeO/MnO = 36.6). Occurring very rarely ongroundmass pyroxene grains are patchy overgrowths of anFe-rich mineral (possibly related to chamosite or chlorite,with 35 wt% FeO, 5 wt% Al2O3, 1.5 wt% MgO and a lowoxide sum of 85 wt%, suggesting the presence of water orhydroxyl). Calcite occurs sparsely along grain boundaries and
as thin veinlets. Texture and mineral compositions are similarto those in olivine-phyric basaltic shergottite DaG 476/670,but olivine is much more magnesian than in other olivine-phyric basaltic shergottites SaU 005/008 and NWA 1068/1110. Specimens: type specimen, 20 g, and two polished thinsections, UWS; main mass, Hupé.
Northwest Africa 1296MoroccoFound 2001 spring Achondrite (angrite)
The single stone weighs 810 g and appears quite fresh with avery thin and shiny, dark-grey, typical fusion crust. It wasfound in Morocco in spring 2001 by an anonymous finder andafterwards bought by a dealer in Bouarfa (Morocco).Petrography, mineralogy, chemistry and classification (A.Jambon, UPVI; J.-A. Barrat, UAng; O. Boudouma, UPVI):The rock has a fine-grained magmatic texture, indicatingrapid cooling, and is significantly different from otherangrites. Numerous small vesicles are present, some of whichfilled with carbonate. Olivine (≈Fo50) was the first phase tocrystallize, as feathery chains a few micrometers in thickness.It is closely associated with anorthite (An98–100) overgrowingthe olivine crystals. These composite chains are separatedfrom one another by intergrown elongated Al, Ti-richdiopside. Both olivine and pyroxene are normally zoned up tomg# <0.01. The most magnesian pyroxene and olivine havemg# of 0.52. The Fe-rich olivines also contain up to 12 wt%CaO, a typical feature of angrites; they appeared afterplagioclase crystallization stopped at the end of thecrystallization sequence when co-crystallization of olivinewith sub-calcic kirschsteinite is observed. Minor phases arepyrrhotite, Ca-phosphate, a silico-phosphate similar to thatfound in d’Orbigny and titanomagnetite. The bulk rockanalysis is that of a typical angrite like d’Orbigny or Sahara99555, with a (Ca/Al)CI of 1.52. Extensive trace element dataconfirm that alkali elements are strongly depleted. Ba isslightly enriched probably as a result of terrestrial alteration;Sr is not. All refractory lithophile incompatible elementsexhibit a flat chondrite normalized pattern with an enrichmentof 13 × CI. Specimens: main mass, Moroccan Import,Asnières, France; type specimen, 49 g, UPVI.
Northwest Africa 1457MoroccoPurchased 2001 December Achondrite (winonaite)
Seven small stones with a total weight of 52 g were purchasedfrom a Moroccan dealer by A. and G. Hupé (Hupé) in 2001December. Classification and mineralogy (A. Irving and S.Kuehner, UWS): medium-grained, equilibrated metamorphictexture with triple junctions among mineral grains. Abundantenstatite (Fs6Wo1.5, FeO/MnO = 15) and forsteritic olivine(Fa5, FeO/MnO = 18) with subordinate diopside (Fs2.8Wo44,
A204 S. S. Russell et al.
FeO/MnO = 8), sodic plagioclase (Ab82Or4), Ni-poor Fe-Nimetal, troilite, schreibersite, Cr-rich chromite, and Cl-richapatite. Daubreelite occurs as blades within some troilitegrains. Rare chromite grains (up to 20 µm; 66 wt% Cr2O3; Cr/(Cr+Al) = 0.870; Mg/(Mg+Fe) = 0.682) are associated withtroilite. Grain boundaries are veined by heterogeneous Ni-free iron oxides and/or hydroxides. Oxygen isotopecomposition (D. Rumble, CIW): analyses of two whole rockfragments by laser fluorination gave δ18O = +5.1 ± 0.1‰;δ17O = +2.3 ± 0.1‰; ∆17O = –0.40 ± 0.03‰. The texture,mineralogy and oxygen isotopic composition of this samplematch the criteria for winonaites given by Benedix et al.(1998). Specimens: type specimen, 10 g, and one polishedthin section, UWS; main mass, Hupé.
Northwest Africa 1459MoroccoPurchased 2002 MarchAchondrite (diogenite, olivine-bearing)
A small complete stone (49 g) found near Iriqui, Moroccowas purchased from a Moroccan dealer by A. and G. Hupé(Hupé) in 2002 March. The interior of the stone is darkyellow-green, and the exterior is coated by a thin, weatheredfusion crust with protruding subhedral chromite grains (up to4 mm). Classification and mineralogy (A. Irving and S.Kuehner, UWS): coarse-grained cataclastic protogranulartexture. Subequal amounts of orthopyroxene (Fs28Wo4.7 toFs30Wo6.5, FeO/MnO = 28–32) and olivine (Fa36; FeO/MnO =46.5), with minor chromite (Cr/(Cr + Al) = 0.62 cores to 0.66rims), anorthitic plagioclase (Ab6.8-Ab9.3), troilite, and metal(0.06 wt% Ni). Some orthopyroxene grains (up to 10 mm)have sparse exsolution lamellae of clinopyroxene (Fs10Wo46to Fs11Wo45, FeO/MnO = 28–32). Some olivine grains (up to8 mm) have multiple tilt-boundaries. Irregular areas alonggrain boundaries are composed of symplectitic intergrowthsof chromite and orthopyroxene. Oxygen isotope composition(D. Rumble, CIW): δ18O = +3.62 ± 0.02‰; δ17O = +1.72 ±0.04‰; ∆17O = –0.19 ± 0.02‰. Specimens: type specimen,10 g, and one polished thin section, UWS; main mass, Hupé.
Northwest Africa 1500Morocco? Purchased 2000Achondrite (ureilite)
A nearly complete individual of about 3.3 kg with fusion crustpatches was bought by meteorite hunters in Zagora. Duringthe Tucson mineral show it was sold to a mineral dealer andtraded to R. Bartoschewitz in April 2002. Mineralogy andclassification (R. Bartoschewitz, Bart; F. Wlotzka, MPI): Thismonomict rock has a typical ureilite texture of equigranularolivines (0.2–0.5 mm, Fo72, CaO, and Cr2O3 < 0.1%) set inblack vein material with finely dispersed metal. Minorcomponents are augite (Wo45En44) and orthopyroxene(Wo2.2En70), plagioclase (An37), chromite (0.2–0.3 mm, 5%MgO, 12% Al2O3) and metal (1.5% Ni, 0.3% Si). The
plagioclase grains are 0.5 to 3 mm across and in igneouscontact with olivine, the larger ones poikilitically encloserounded olivine grains. Oxygen isotope composition (R.N.Clayton and T. Mayeda, UChi): δ18O = +4.56‰; δ17O =+1.58‰ plot away from other ureilites. But ∆17O versus mg-number extends the ureilite trend. Specimens: type specimen,20 g MPI; main mass, Bart.
Northwest Africa 1569MoroccoFound 2000Achondrite (ureilite)
A 614 g partially crusted stone was purchased in Erfoud,Morocco in 2001. Classification and mineralogy (T. Bunchand J. Wittke, NAU): typical ureilite texture; olivine grain sizeup to 1.5 mm with triple junctions, poorly developedlineation, low-Ni metal (mostly oxidized) interstitial toolivine; low-Ca pyroxene is <1 mm and tends to occur inclusters with interstitial carbonaceous matter. Olivine coresare Fa18, dusty rims are reduced to Fs10; (Cr2O3 up to 0.62wt%; CaO up to 0.41 wt%); low-Ca pyroxene is Fs18Wo8 toFs23Wo9; metal, 0.47 to 5.3 wt% Ni, 0.55 wt% Cr2O3, 0.4wt% P and 0.29 wt% Si; sulfides contain up to 1.4 wt% Cr.Shock level, S2; weathering grade, W1. Specimens: mainmass with anonymous buyer; type specimen, 20.5 g, and thinsection, NAU.
Northwest Africa 1583Northwest AfricaFound 2001/2002 winterRumuruti chondrite (R3.9)
Several small pieces totalling 78 g were found in winter 2001/2002 by an anonymous finder in the Western Sahara.Classification and mineralogy (A. Greshake, MNB; M. Kurz,Kurz): an unbrecciated type 3.9 R chondrite; olivine, Fa37.3 ± 2.6(range Fa28.2–40.2); low-Ca pyroxene, Fs18.0 ± 4.6 (range Fs12.4–
25.3); augite, Fs8.2–10.2Wo30.2–48.4; plagioclase, An7.8–12.1; shockstage, S2; degree of weathering, W1/2. Main mass withanonymous finder; type specimen 15.6 g plus one polished thinsection MNB.
Northwest Africa 1586Northwest AfricaFound 2002 JuneAchondrite (ureilite)
A 400 g stone was collected by nomads in the Sahara and lateron purchased from a dealer in Morocco. Classification andmineralogy (S. Singletary, MIT): typical monomict ureilitetexture with abundant triple junctions and curvedintergranular boundaries. Grain sizes are 1–2 mm on average.Mineral modes are 75% olivine, 25% pyroxene.Homogeneous olivine cores (Fo79, n = 61) have reductionrims that contain finely dispersed grains of metal and olivine(Fo97). The predominant pyroxene is pigeonite with mg# of80 and Wo11 (n = 103). Pigeonite grains have “swaths” (melt
Meteoritical Bulletin No. 87 A205
veins?) that contain a metal and three-pyroxene assemblageconsisting of augite (mg# 90, Wo32, n = 17), orthopyroxene(mg# 86, Wo5, n = 8) and pigeonite (mg# 86, Wo9, n = 6).Specimens: main mass, Bessey; type specimen, 21.9 g, andone thin section, TCU.
Northwest Africa 1644MoroccoPurchased 2001 springAchondrite (eucrite, polymict)
A mass of 214 g was purchased by Bessey from a dealer inMorocco. Mineralogy and classification (S. Singletary, MIT):brecciated texture with several large lithic and mineral clastsin a fragmental matrix. The clasts resemble diogenites,cumulate and basaltic eucrites in mineral composition andtexture. Medium-grained cumulate eucrite clasts of ophitictexture consist of plagioclase (An91–94) and pigeonite (Wo5–10,En37–52), minor orthopyroxene (Wo3, En53) and Ti-richchromite. Basaltic eucrite clasts with a sub-ophitic texturecontain extremely iron-rich augite (possibly pyroxferroite;Wo16–31, En3–8), plagioclase (An82–87), a silica phase and Ti-rich chromite. Sparse (<5 vol%) diogenitic clasts consist oforthopyroxene (Wo2–5). Pyroxene Fe/Mn ranges from 27–33.The possible pyroxferroite grains have Fe/Mn 27–45. Matrixis pyroxene (pigeonite, augite, and orthopyroxene), minorolivine, Fe-rich sulfides, Ti-rich chromite and rare spherulesof glass; one zircon grain was observed; one symplectiticgrain composed of silica, augite and fayalite is interpreted tobe the result of pyroxferroite breakdown. Specimens, typespecimen, 20 g, TCU; main mass, Bessey.
Northwest Africa 1646MoroccoPurchased 2002 October Achondrite (eucrite, cumulate)
A complete fusion-crusted stone (259 g) was purchased froma Moroccan dealer by A. and G. Hupé (Hupé). Classificationand mineralogy (A. Irving and S. Kuehner, UWS): Fine-grained with clasts of anorthite, exsolved pigeonite, chromite,ilmenite, metal, troilite and silica in a complex matrix whichhas the texture of a eutectoid melt of plagioclase + pyroxene.FeO/MnO is 32.8 for orthopyroxene and 34.8 forclinopyroxene. Veinlets of glass probably are quenchedimpact melt. Specimens: type specimen, 20 g, and onepolished thin section, UWS; main mass, Hupé.
Northwest Africa 1647MoroccoPurchased 2002 SeptemberAchondrite (eucrite)
A complete fusion-crusted stone (313 g) acquired from aMoroccan dealer was subsequently purchased at the DenverMineral Show in 2002 September by A. and G. Hupé (Hupé).
Classification and mineralogy (A. Irving and S. Kuehner,UWS): fine grained with subophitic texture; most grains arefractured. Composed of a single lithology that has cross-cutting veinlets of very fine grained, comminuted crystallinedebris. The meteorite contains anorthite laths (Ab5), exsolvedpigeonite (clinopyroxene lamellae in orthopyroxene), somelarger orthopyroxene grains, silica polymorph, ilmenite,troilite and chromite. Minor calcite occurs in a veinlet.Mineral composition: orthopyroxene (Wo2.3Fs61.7, FeO/MnO= 32.0) and clinopyroxene (Wo43.8Fs22.8, FeO/MnO = 29.6).Specimens: type specimen, 20 g, and one polished thinsection, UWS; main mass, Hupé.
Northwest Africa 1648MoroccoPurchased 2002 October Achondrite (diogenite, polymict)
A complete fusion-crusted stone (803 g) was purchased froma Moroccan dealer by A. and G. Hupé (Hupé). Classificationand mineralogy (A. Irving and S. Kuehner, UWS):Heterogeneous breccia composed of multiple clast types ofvarying size. Angular mineral clasts are predominantlyorthopyroxene with subordinate anorthite (Ab5), silica,exsolved pigeonite, ilmenite and troilite. The orthopyroxeneclasts are homogeneous and have low Ca contents, but rangewidely in Fe/Mg ratio (FeO = 12.6–22.5 wt%, FeO/MnO =28.2–34.8), suggesting multiple diogenitic parent rocks.Sparse polycrystalline clasts include cumulate eucrites,basaltic eucrites, a quench-textured clast consisting ofdendritic olivine grains in glass, and fine grained ferroaninter-growths (breakdown of former pyroxferroite) composedof hedenbergite + fayalite + silica ± ilmenite ± troiliteattached to anorthite laths. Breccia consisting of variousdiogenites (>80% by volume), sparse cumulate eucrites andrare basaltic eucrites. Specimens: type specimen, 22 g, andthin section, UWS; main mass, Hupé.
Northwest Africa 1653Northwest AfricaFound 2002Achondrite (howardite)
A single stone of 376 g partly covered by fusion crust wasfound in 2002 by an anonymous finder in the Western Saharandesert and purchased in Zagora in 2002. Classification andmineralogy (A. Greshake, MNB; M. Kurz, Kurz): basalticeucrite and diogenitic clasts are set into a clastic matrix; darkimpact melt fragments are abundant and often show quenchtextures with radial or skeletal shaped aggregates; eucriteclasts contain plagioclase, An91.9 (range An86.2–95.7);pigeonite, Fs35.8–59.2Wo5.8–17.6 and augite, Fs29.9–55.6Wo22.8–
31.1; minor phases include silica, chromite, and ilmenite;diogenite clasts are composed mainly of orthopyroxene, Fs25–
41.4Wo3.1–4.9 and olivine, Fa27.7 (range Fa26.2–30.2); chromite
A206 S. S. Russell et al.
and ilmenite are among the accessory phases; low degree ofshock; low degree of weathering. Main mass with anonymousfinder; type specimen 21.0 g plus two polished thin sections,MNB.
Northwest Africa 1654Northwest AfricaFound 2002Achondrite (eucrite)
A single stone of 49 g partly covered by fusion crust wasfound in 2002 by an anonymous finder in the WesternSaharan desert and purchased in Zagora in 2002.Classification and mineralogy (A. Greshake, MNB; M. Kurz,Kurz): the meteorite is dominated by a recrystallized matrixof 10–20 µm-sized plagioclase, pigeonite with augiteexsolution lamellae, and opaque phases; embedded into thematrix are large mineral fragments of plagioclase and Ca-pyroxene and basaltic clasts; plagioclase contains pigeoniteand troilite inclusions; plagioclase composition, An88.5 (rangeAn85.2–92.3); pigeonite composition, Fs50.3–60.6Wo5.6–15.2;augite composition, Fs29.7–47.4Wo20.2–41.5; minor phasesinclude orthopyroxene (Fs57.9Wo4.3), silica, ilmenite, troilite,and Al-Ti-chromite. A low degree of shock and only amoderate degree of weathering. Main mass with theanonymous finder; type specimen, 11.3 g plus one polishedthin section, MNB.
Northwest Africa 1658Northwest AfricaFound 2002Ordinary chondrite (L3–6)
Six individual stones totalling 1345.5 g were found in 2002by an anonymous finder in Western Sahara and purchased inZagora in 2002. Classification and mineralogy (A. Greshake,MNB; M. Kurz, Kurz): a brecciated meteorite partly coveredby fusion crust; it consists of light-grey, dark-grey and almostblack angular clasts of different petrologic types. The blackfragments resemble impact melt clasts; unequilibratedfragments: olivine composition, Fa2–24.2; pyroxenecomposition, Fs8.2–18.8; equilibrated fragments: olivinecomposition, Fa23.8; pyroxene composition, Fs19.8; moderateshock stage, S3/4; a low degree of weathering, grade W1.Main mass with the anonymous finder; type specimen, 20.5 gplus one polished thin section, MNB.
Northwest Africa 1664 ~29°23′N, ~3°11′WAlgeriaFind 2002Achondrite (howardite)
A very fresh, fully fusion-crusted single stone of 6310 g wasfound by local people in the desert of the Hamadah
Tounassine region in Algeria near the town Tabelbala. Lateron, it was purchased by A. Pani (Pani). Mineralogy andclassification (F. Brandstätter and C. Lorenz, NHMV): themeteorite is a polymict breccia consisting mainly of mineralfragments, lithic clasts (diogenitic and eucritic), chondrule-like objects and (devitrified) glass fragments embedded in afine-grained clastic matrix. Pyroxenes (En13–80Wo1–40) andfeldspars (An80–95) cover the compositional range typical forhowardites. Chondrule-like objects and glass fragments havesizes up to 1 cm. Specimens, type specimen, 258 g, NHMV;main mass, Pani.
Northwest Africa 1666MoroccoPurchased 2002 October Achondrite (eucrite, polymict)
A complete fusion-crusted stone (320 g) was purchased from aMoroccan dealer by D. Gregory (Gregory). Classification andmineralogy (A. Irving and S. Kuehner, UWS): Angular mineralclasts consist of anorthitic plagioclase (An95Ab5), exsolvedpigeonitic pyroxene, silica, ilmenite and troilite. Thepyroxenes contain exsolution lamellae of clinopyroxene (FeO/MnO = 34.8) within orthopyroxene (Wo4.2Fs56.9, FeO/MnO =32.3–35.9). Polycrystalline clasts include various basalticeucrites, cumulate eucrites and derivative fragments(containing anorthite with pyroxene or silica), a 2 cm quench-textured basaltic eucrite clast (containing larger, elongategrains of low-Ca pyroxene in a finer-grained matrix ofpigeonite and anorthite), and an individual breccia clast.Specimens: type specimen, 20 g, and one polished thin section,UWS; main mass, ROM.
Northwest Africa 1669MoroccoPurchased 2001 JanuaryMartian meteorite (basaltic shergottite)
A single stone weighing 36 g was bought in Erfoud by BrunoFectay (Fectay). The location of its find is unknown but AlMala’ika was used as working name. The sample is mostlycovered with desert varnish with a few remnants of fusioncrust. Classification and mineralogy (A. Jambon and O.Boudouma, UPVI; J.–A. Barrat, UAng; M. Bohn, Brest): fine-grained basaltic rock consisting mainly of zoned pyroxeneswith intergrowths of pigeonite En58–25Wo9–19Fs32–61 andaugite En19–47Wo39–24Fs54–18; FeO/MnO ratio of 34 (n = 312).Maskelynite (Ab41–53Or1–6An58–42) appears to be injectedbetween pyroxene phenocrysts. Accessory minerals includepyrrhotite, merrilite, apatite, ulvöspinel, ilmenite, silica, andbaddeleyite. Small melt pockets with stishovite occuring assubmicrometer-sized needles. Pyroxene cores are cut bylarge- and medium-sized fractures, whereas their rims are
Meteoritical Bulletin No. 87 A207
affected by numerous small fractures. Maskelynite is onlyaffected by a few major fractures. Terrestrial calcite is presentmainly as veins cross-cutting the meteorite, as in many otherSaharan finds. Oxygen isotope composition (I. A. Franchi,OU): δ18O = +0.30‰; δ17O = +2.85‰; ∆17O = +4.91‰.Specimen; main mass, Fectay; type specimen, 7.4 g, ENSL.
Northwest Africa 1695MoroccoFound 2001Achondrite (howardite)
A 614 g, fully crusted stone, was purchased in Morocco in 2001.Classification and mineralogy (J. Wittke and T. Bunch, NAU):clast size, <0.5 cm; clast modal analyses on 14 cm2 yield:subophitic basalts with large areas of symplectitecrystallization, 80 vol%; diogenites, 9 vol%; fine-grained (<0.2 mm) subophitic basalts, 6 vol%; other, 5 vol%.Orthopyroxene, Fs17–26 with exsolved pigeonite, Fs28–32Wo7–
10. Common, Fe-rich subophitic clasts of plagioclase, An78, andferroaugite, Fs40Wo39En21, with symplectic mesostasis offayalite, ferrohedenbergite, sulfides, and SiO2 glass. Shockstage, S1, weathering grade, W1. Specimens: main mass withbuyer, type specimen, 21 g with one thin section, NAU.
Northwest Africa 1701MoroccoFound 2002 springOrdinary chondrite (LL5, impact melt breccia)
A dark brown stone of 225 g was bought in Erfoud (Morocco)by M. Chinellato (Chin). Classification and mineralogy (G.Pratesi, V. Moggi Cecchi, MSP): composed of fine-grainedand coarse-grained lithologies. Fine-grained area has a re-crystallization texture with few grains of residual metal andolivine in a matrix of feldspathic glass (An31.1Ab54.7),containing very fine grained (10 µm) olivine and pyroxenecrystals, rimmed by fringes of metal pools and droplets.Pyroxenes in matrix are zoned, bronzite cores, En86.1Wo1.9 topigeonite rims, En66.2Wo10.7. The coarse-grained portionpresents a typical chondritic texture: olivine, Fa27.2, pyroxene,En22.6Wo1.6, metal and troilite. Terrestrial weathering gradeW2; shock stage S4. Specimens: main mass, Chin; typespecimen, 20.4 g, and thin section, MSP.
Northwest Africa 1813Western SaharaFound 2001/2002 winterAchondrite (eucrite, polymict)
One stone of 70 g was found in Western Sahara. Mineralogy(C. Lorenz, Vernad): the polymict breccia consists of anumber of mineral and rock fragments, embedded in a fine-grained clastic matrix. The lithic clasts are coarse- tomedium-grained, poikilitic and poikilo-ophitic pyroxene-
plagioclase rock clasts (~40 vol%), minor fine-grainedgranoblastic pyroxene-plagioclase rock clasts (~5 vol%), meltrocks and breccias. Mineral chemistry: pyroxene isEn37.5Wo3.1 with lamellae of En30.5Wo42.2; feldspar is An88–92.Accessory phases are silica, chromite, ilmenite, troilite andFe-metal. Specimens: one section and 14 g, Vernad; mainmass with anonymous finder.
Northwest Africa 1814MoroccoPurchased after 1999Bencubbin-like meteorite
One moderately oxidized, partially crusted stone, weighing156 g, was purchased in Morocco. It is said to have beenfound in April 1999 in the region between Taouz and Ouzina.Mineralogy and classification (C. Fiéni and C. Perron,MNHNP): very similar to Bencubbin and Weatherford. Itconsists of large clasts (up to about 1 cm in size) of Fe-Nimetal (about 60 vol%) and barred or cryptocrystallinesilicates. Olivine Fa2.8, CaO 0.25 wt%, Cr2O3 0.37 wt%; low-Ca pyroxene En94Wo1.4; high-Ca pyroxene En49Wo47.5;feldspathic mesostasis. Clasts are embedded in a metal-silicate impact melt, whose silicate portion has FeO ~20 wt%.Specimens: type specimen, 21 g, MNHNP, main mass, Fectay.
Oman meteorites(355 meteorites)OmanFound 2000–2002
Table 4 reports 355 meteorites that were found duringfieldwork in the desert of Oman by people searching formeteorites.
Park Forest 41°29′05′′N, 87°40′45′′WCook County, Illinois, USAFell 2003 March 26, approx. 23:50 hrs local timeOrdinary chondrite (L5)
A bright fireball was seen by numerous observers in parts ofIllinois, Indiana, Wisconsin and Ohio around midnight ofMarch 26, 2003. Numerous stones fell, mostly concentratedin the area of the village of Park Forest. At least two houses inPark Forest were struck, as was the Fire Station. Dozens ofother stones or fragments of stones were recovered in the areain the hours and days following the fall. Total mass recoveredis more than 18 kg, largest stone ~3 kg in possession of finder.Description and classification (S. Simon, UChi; M. Wadhwa,FMNH; P. Sipiera, PSF): Most stones are partly to fullyfusion-crusted. Some broken faces show brecciated texture,angular clasts. Cross-cutting dark veins and dark pockets maybe of impact melt origin. No visible chondrules in handsample. Abundant troilite and metal visible in some brokenfaces. Chondrules and maskelynite are visible in thin section.
A208 S. S. Russell et al.
Mean olivine composition Fa24.7, mean low-Ca pyroxeneFs20.7Wo1.6. Shock stage S5. Specimens: type specimen 515 g(hit fire station), FMNH. Other stones at FMNH: 1200 g, 529g, 183 g, 159 g, 125 g.
Pê 11°20.02′N, 3°32.53′WHoundé, Burkina FasoFell 1989 June 14, 7:30 local timeOrdinary chondrite (L6)
A fist-sized stone (weight unknown) was seen to fall byfarmers working in a field near to Pê, southwestern BurkinaFaso. The chief of the village threw the stone away because itwas thought to be a bad omen; later, however, geologists fromBureau of Mines and Geology of Burkina Faso inOuagadougou managed to retrieve few fragments.Mineralogy and classification (M. Bourot-Denise, MNHNP):Ordinary chondrite, L6 (Fa25.4Fs22.1), S1, W0, very friable.Specimens: type specimen, 11.1 g, MNHNP; some fragments,Museum of Bureau of Mines and Geology of Burkina Faso inOuagadougou.
Pétèlkolé 14°3.12′N, 0°25.20′ETéra, NigerFell 1995 April 10Ordinary chondrite (H5)
The fall occurred in the afternoon and was eye-witnessed by ashepherd in the campground of Garauol Olo, near Pétèlkolé,Téra district, not far from the border with Burkina Faso. Onestone of 189 g was collected just after the impact, under fewcentimetres of sand. An investigation in Pétèlkolé led by AmaSalah Issack (Department of Geological and MiningResearch) confirmed that only one stone was collected andprovided the coordinates of the fall. Mineralogy andclassification (L. Latouche, MNHNP): Ordinary chondrite,H5 (Fa18Fs16), S2, W0. Specimens: type specimen, 30 g,MNHNP, 60 g Africa Museum, Brussels, Belgium; mainmass, University of Niamey, Niger.
Pitino, see American meteorite finds
Point Berliet, see Saharan meteorites from Niger
Queen Alexandra Range (QUE),see Antarctic ANSMETmeteorites
Rebiana, see Saharan meteorites from Libya
Saharan meteorites from Algeria(33 meteorites)AlgeriaFound 1989–2001
A number of different finders recovered these meteoritesfrom several regions of the Algerian Sahara (Table 5).
Saharan meteorites from Egypt(1 meteorite)EgyptFound 1999 December
Louis Carion and others found this meteorite from the GreatSand Sea region of the Egyptian Sahara (Table 6).
Saharan meteorites from Libya(94 meteorites)LibyaFound 1998–2001
A number of different finders recovered these meteoritesfrom several regions of the Libyan Sahara (Table 7).
Saharan meteorites from Morocco and surroundingcountries
(298 meteorites)Northwest AfricaPurchased or found 1999–2002
Many meteorites lacking first-hand documentation of the findlocation are being sold by Moroccan rock and mineraldealers, and by people from other countries who havecollected material in Morocco. These meteorites are all soldas Moroccan finds, but there are plausible reports that somewere actually collected in Algeria or Western Sahara. Othermeteorites have been reported from this region with whatappear to be precise find locations. The reliability of localityinformation associated with these meteorites is difficult toassess owing to the anonymity of all of the finders and mostof the original sellers, and because the NomenclatureCommittee lacks the resources to investigate. All meteoritesfound in this region are numbered in a “Northwest Africa”(NWA) series. The Nomenclature Committee considers itpossible that differently numbered specimens are paired witheach other or with other named meteorites and some mayeven be derived from the same individual object. Table 8 lists298 specimens of this type.
Saharan meteorites from Niger(8 meteorites)NigerFound 1999, 2001, 2002
A number of different finders found these meteorites fromseveral regions of the Sahara of the Republic of Niger (Table9).
Saharan meteorites from unknown locations(20 meteorites)Sahara, country unknownFound 1998–2000
A number of different anonymous finders recovered thesemeteorites from unknown locations within the Sahara (Table10).
Meteoritical Bulletin No. 87 A209
Sahara 00177 +0°09.25′, z+0°06.87′WFound 2000Carbonaceous chondrite (C3/4, CV-like)
A 12 g stone was found by Labenne. Mineralogy andclassification (M. Bourot-Denise, MNHNP): related toreduced CVs, similar to Coolidge and Loongana 001.Chondrules, chondrule fragments and CAIs make up ~75vol% of the meteorite. Overall, chondrules are smaller than inAllende, with a mean size ~500 µm. CAIs (~10 vol%) arelarge, up to 1 mm in size. The largest and most abundantchondrules are type-I, porphyrytic olivine-pyroxenechondrules, often of irregular shape, with olivine crystals inthe 10–40 µm size range, and abundant opaque beads. Lessabundant metal-poor barred olivine, radial pyroxene andother chondrules are generally smaller (100–300 µm) andmore rounded. Olivine, Fa8.0 ± 1.0 (range: 5.0–9.6); low-Capyroxene Fs7.6 ± 2.4 (range: 3.4–10.5). Chondrule mesostasis iscompletely devitrified. A few chondrules are partiallyrimmed with silica (as is the case in Coolidge). Fe-Ni metal iskamacite, with minor taenite. Weakly shocked, metal is notwarped, troilite is monocrystalline. Moderately weathered;metal grains, especially those in the matrix or on chondrulesedges, have a 2–5 µm-wide limonite rims; veins in chondrulessilicates are also filled with limonite; troilite is unaltered.Type specimen, 4 g, MNHNP, main mass with Labenne.
Saint-Aubin 48°29′N, 3°35′EAube Champagne, FranceFound 1968Iron, octahedrite (ungrouped)
Five masses of total weight 472 kg were found by farmers whileploughing, within a strewn field a few miles across.Classification (E. Dransart and M. Baron, EMTT): kamacitebandwidth 0.4 mm; bulk composition Ni = 11.5 ± 1%, Co = 4mg/g, P = 2 mg/g, Ir = 0.02 µg/g, Ga = 28 µg/g, Ge = 83 µg/g.The meteorite contains sarcopside and/or graftonite andneedles of schreibersite up to 6 cm in length. It shows typicalshock features (Neumann lines and shock-hatched kamacite).Specimens: type specimen 86 g MNHNP; 500 g EMTT; mainmass with finders.
San Juan 001 25°34.5′S, 69°47.7′WTaltal, Antofagasta, ChileFound 2001 December 1Ordinary chondrite (L5)
Three stones of 1229 g total mass were found within 1 km ofeach other. Classification (M. Zolensky, JSC): Olivine, Fa24.5;pyroxene, Fs21.6, shock stage S1/2, weathering grade W2.Specimens: type specimen 60 g, SI; main mass, RodrigoMartinez.
San Juan 002 25°34.5′S, 69°47.7′WTaltal, Antofagasta, ChileFound 2002 February 20Ordinary chondrite (H6)
Thirty four masses of the meteorite were found by RodrigoMartinez during a desert search, with a total weight of 345 g.Classification (M. Zolensky, JSC): Olivine, Fa19.25 PMD0.004, low Ca-pyroxene, Fs19 PMD 0.008, contains abundantcoarse-grained plagioclase, Ab79Or8 to Ab83Or4. Shock stageS1, weathering grade W3. Specimens: main mass Mr. R.Martinez; type specimen 21g, SI.
Sandy Creek 40°26′N, 98°04′WClay County, Nebraska, USAFound 1999 July 6Ordinary chondrite (L5)
One stone of 1330 g was found on an airport runway while itwas being graded. Classification (A. Rubin, UCLA): Olivine,Fa25.2 ± 0.6, shock stage S4, weathering grade W4. Specimens:type specimen 55.7 g, UCLA; 37.6 g, DMNH; main massJensen.
Sayh al Uhaymir 085–169, see Oman meteorites
Sayh al Uhaymir 085 21°04.1′N, 57°16.2′EOmanFound 2002 January 11Carbonaceous chondrite (CV3)
Three stones of 112 g total were found on the surface of thedesert. Mineralogy and classification (M. Ivanova, M.Nazarov, Vernad): The meteorite consists of matrix, olivineaggregates, chondrules, their fragments, and CAIs. Thematrix/chondrule ratio is 0.8. Olivine, Fa0.7–80.5; low-Capyroxene, Fs0.7–22.6; pigeonite, augite, diopside, and Al-diopside are also present. Mesostasis in chondrules is altered;accessories are kamacite and taenite, magnetite, chromite,sulphides and sulphates. Two observed CAIs are 0.9 × 1.0 mmand 1.7 × 1.9 mm in size, mostly fine-grained, consisting ofmelilite, spinel, Al-diopside, and anorthite. Matrix is finegrained and altered, with development of phyllosilicates.Microprobe analyses were performed at UTenn. Specimens:type specimen, 25 g, and thin section, Vernad; main mass withanonymous finder.
Sayh al Uhaymir 089 20°52.9′N, 57°12.0′EOmanFound 2001 January 17Ordinary chondrite (L/LL3.6/3.7)
One complete stone of 2618 g was found on the surface of thedesert. Classification (S. Afanasiev, Vernad): chondrules are
A210 S. S. Russell et al.
well defined (up to 7 mm in diameter), fine-grained, ofdifferent types: porphyritic olivine-pyroxene and olivine,radial pyroxene, barred olivine, granular andcryptocrystalline. Shock stage S2; weathering grade W2. Thecomposition of olivine is Fa25.0; the pyroxene composition isFs6.25–23.4 (n = 20); PMD of Ni content in kamacite is 5.58(n = 30), and TL sensitivity measurements are in the range of0.46–1.0 (A. I. Ivliev, Vernad). Microprobe analyses weredone by N. Kononkova, Vernad. Bulk iron content is Fe0 = 4.2wt%. Specimens: type specimen, 350 g, and a thin section,Vernad; main mass with anonymous finder.
Sayh al Uhaymir 120 21°00.2′N, 57°19.3′EOmanFound 2002 November 17Martian meteorite (basaltic shergottite)
A stone of 75 g was found in the area of previous shergottitefinds. This stone has a well-preserved black fusion crust. It isa grey-greenish stone with porphyritic texture; large olivinephenocrysts are embedded in a groundmass consisting ofmaskelynite and pigeonite. SaU 102 is paired with SaU 005/008/051/060/090/094. Classification (S. Afanasiev, Vernad).Specimens: type specimen, 15.8 g, Vernad; main mass withanonymous finder.
Sayh al Uhaymir 150 20°59′31.3′′N, 57°19′11,7′′EAl Ghaba, OmanFound 2002 October 8Martian meteorite (basaltic shergottite)
A 107.7 g olive-brown colored stone of relatively angularshape with one small area of thin black-brown fusion crustwas recovered on a Miocene fresh-water limestone gravelplateau about 43 km south of Al Ghaba by Rainer and SvenBartoschewitz. Mineralogy and classification (R.Bartoschewitz, Bart, P. Appel and B. Mader, Kiel):porphyritic texture with olivine phenocrysts up to 2 mm(Fo67–64) set in a matrix consisting of feldspathic glass (An53–
66Or0.3–0.8) and pigeonite (En62–69Wo7–11) with minor Ca-poorpyroxene (En65–66Fs34–35). Shock melt veins and pockets arepartly recrystallized. Shock stage, S5. Oxygen isotopiccomposition (R.N. Clayton, UChi): δ17O = +2.78‰, δ18O =+4.74‰, they fall in the SNC field. SaU 005, 008, 051, 060,and 094 were found in the same area and may be paired.Specimens: 17.7 g Muzeum Ziemi PAN, al. Na Skarpie 27,PL- Warszawa, 2.7 g Kiel, main mass Bart.
Sayh al Uhaymir 169 20°34.391′N, 57°19.400′EOmanFound 2002 January 16Lunar meteorite (KREEP-rich mafic impact melt brecciaand adhering regolith)
A complete, light grey-greenish rounded stone (70 × 43 × 40mm) weighing 206.45 g was found in the Sayh al Uhaymirregion of Oman. Finders, mineralogy and classification: E.
Gnos, B. A. Hofmann, and A. Al-Kathiri (UniBern): darkbrown fusion crust is only locally preserved. The impact meltbreccia (87 vol% of the stone, based on 8 X-ray tomographicsections) contains 25–40 vol% of strongly shocked igneousrocks and crystal clasts (up to 17 mm) derived from norites,evolved magmatites, and granulites set in a fine-grained (<0.1mm) crystalline matrix. Most crystal fragments are shockedplagioclases, locally associated with enstatite. In addition toplagioclase metallic iron, spinel, olivine, and orthopyroxeneclasts are present. The fine-grained impact melt matrixconsists mainly of short prismatic low-Ca pyroxene (En61–64,Wo2–4), interstitial plagioclase (An75–81) intergrown withpotassium feldspar. The remaining minerals are poikiliticilmenite, whitlockite, olivine (Fo58–59), zircon, and traces oftroilite, kamacite and tridymite. The regolith (13 vol%)present one one side of the meteorite comprises crystallineand glassy volcanic rocks, igneous lithic fragments, brecciafragments, fragments of mafic granulites, and crystalfragments. The impact melt breccia contains 32 ppm Th and8.5 ppm U, 0.47% K (K/U = 553), indicating a lunar origin.This is further confirmed by fusion-crust Fe/Mn of 75.1(microprobe, n = 14) and impact melt bulk Fe/Mn of 79.Oxygen isotope composition (I. A. Franchi, OU) are alsoconsistent with a lunar origin (∆17O = 0.001 ± 0.032‰). Thisimpact melt breccia is the most strongly KREEP-erichedlithology among all known lunar rocks. Weathering: W1 (Femetal shows only little oxidation). Specimens: All in NMB.
Séguédine, see Saharan meteorites from Niger
Shalim 002–003, see Oman meteorites
Shişr 006–021, see Oman meteorites
Souslovo 55°25.770′N, 55°47.236′EBashkortostan, RussiaFound 1997 JulyOrdinary chondrite (L4)
In late July 1997, Ismagil Gaysin and his son Radik wereloading hay on to a cart near Souslovo village, 10 km N ofBirsk town. The cart was not safe on the sloping track, and thefather asked his son to find a stone to secure the wheel. Radikfound a stone buried in soil in the nearest ditch. When thework was finished, they decided to bring the stone homebecause it had an unusual color and shape. Later, they thoughtthat the stone (weighing 19.3 kg) could be a meteorite, and in2002 sent a piece to the Vernadsky Institute, Moscow foridentification. In 1966 March 30, 15:45 UT, a bright fireballwas observed in the region and it could be that the meteoritefind might be related to the fireball. Classification andmineralogy (S. Afanasiev, Vernad): olivine, Fa23.5; pyroxene,Fs23.2Wo1.3; shock stage, S2; Weathering grade, W0/1.Specimens: 6147 g, Vernad; main mass with anonymousowner.
Meteoritical Bulletin No. 87 A211
Southampton 44°30.385′N, 81°22.33′WBruce, Ontario, CanadaFound 2001 April 26Pallasite
A single 3.58 kg stone was recovered by Mr. Carl Youngwhile walking along the beach of Lake Huron. Classification(N. MacRae, S. Kissin, UWO): olivine, Fo87.5; metal Ni 94.7mg/g, Co 5.15 mg/g, As 18.5 µg/g, Au 2.12 µg/g, Cr <2 µg/g,Cu 144 µg/g, Ga 17.2 µg/g, Ge 77.8 µg/g, Ir 0.137 µg/g, Pt<0.4 µg/g, Re <5.6 ng/g, Sb <30 ng/g, W 190 ng/g.Specimens: main mass property of finder and currently held atUWO, type specimen, 175.6 g, UWO.
Spade 34°00′04′′N, 102°07′42′′WLamb County, Texas, USAFound October 2000Ordinary chondrite (H6)
A single mass of 8.86 kg was found in a grass field by Mr. J.Talbert while farming. Classification and mineralogy (R.Jones, UNM; A. Rubin, UCLA): Olivine, mean Fa19; Low-Capyroxene, mean Fs17Wo3.75; Plagioclase, mean Ab79.9Or5.8;kamacite, mean Ni 6.9 wt%, Co 0.46 wt%. Shock stage S2,weathering grade W2. Spade is an annealed impact melt rock.It has very low abundances of relict chondrules and coarsemafic silicates; heterogeneous plagioclase; high Wo contentsof low-Ca pyroxene; chromite-plagioclase assemblages; andextensive silicate darkening. Specimens: main mass withfinder; type specimen, 81 g, plus thin section, UNM.
Tambo del Meteorito 23°58.86′S, 68°18.78′WSan Pedro de Atacama, Antofagasta, ChileFound 2002 January 27Ordinary chondrite (H6)
A single 13.84 g stone was found by Mr. Lorenzo Villaloboson the desert surface while searching for Inca potteryfragments. Classification (M. Zolensky, JSC): Olivine, Fa17.0.Low Ca-pyroxene, Fs20.4, CaO >1%. Augite, plagioclase,pentlandite, and troilite are abundant. Shock stage S1,weathering grade W5. Specimens: main mass EdmundoMartinez, type specimen 3 g, SI.
Tanezrouft 003–061, see Saharan meteorites from Algeria
Tanezrouft 057 25°16′N, 0°09′EAlgeriaFound 2002 December 23Carbonaceous chondrite (C4)
A large (5.4 kg), dark grey, moderately compact stone,lacking fusion crust was found by F. Beroud and C. Boucher.Mineralogy and classification (B. Devouard and J.-L.Devidal, UBP; B. Zanda and M. Denise, MNHNP): largechondrules (around 1mm in diameter), matrix around 50% butlocally more abundant (~70%), numerous irregular whitishinclusions up to 3 mm, and occasional zoned CAIs up to
17 mm. In addition, several large (up to 2.5 cm) dark greyinclusions show a finer grained petrology, with no (orextremely rare) chondrules or CAIs. More of these fine-grained inclusions are visible at the surface of the handsample. The meteorite is nearly equilibrated: olivines arearound Fa30 ± 4 except for a few unequilibrated chondrules;OPX range from Fs3 to Fs30, with a mean at Fs19. Thegroundmass is highly recrystallized, with homogeneousolivine, orthopyroxene and plagioclase grains around 100 µmin size. The groundmass is texturally equilibrated, althoughmost grains seem to be porous. Magnetite is the dominantopaque mineral, associated with minor FeS, Ni-richmonsulfide, minor pentlandite and possibly pyrite. Outsidechondrules, small magnetite grains and minute sulfide grainsare scatterred within the matrix. No metal was observed.However, iron hydroxides patches are visible, and metal orsulfides may be have been obliterated by terrestrialweathering. The numerous irregular inclusions retain a fine-grained texture made of plagioclase and clinopyroxene thatmay be metamorphosed CAIs. The overall characteristics ofthis meteorite are consistant with a C4 classification, withaffinities to the CV oxidized subgroup and/or the CK group.Specimens: type specimen, 110 g, MNHNP; main mass withfinders.
Tassédet 001–003, see Saharan meteorites from Niger
Tentacle Ridge (TEN), see Antarctic ANSMET meteorites
Thiel Mountains (TIL), see Antarctic PSF meteorites
Thuathe ~29°20′S, 27°35′ELesothoFell 2002 July 21, ~13:49 GMTOrdinary chondrite (H4/5)
A meteorite travelling east to west exploded over Lesothoproducing an elliptical strewn field extending 7.4 by 1.9 km(bearing: ~276°) on the westernmost lobe of the Thuathe (orBerea) Plateau, ~12 km east of the capital city of Maseru(approximate strewnfield apex coordinates: (W) 29°19′31′′S,27°34′37′′E; (E) 29°19′54′′S, 27°39′19′′E; (N) 29°19′11′′S,27°37′2′′E; (S) 29°20′14′′S, 27°36′54′′E). The explosion wasaccompanied by an extraordinarily loud, 15 s long noisewhich was heard over a large (100 km radius) area of Lesotho;the fall was eye-witnessed by several people who reportedsightings of dust trails of “sparkling objects” over Lesothoand the southern part of the Free State Province of SouthAfrica. Many villagers of Ha Ralimo, Boqate Ha Majara, andBoqate Ha Sofonia reported falls of stones close tothemselves and onto their homes. The estimated total mass ofrecovered material is ~30 kg, including 418 stones in the 2 gto 2.4 kg mass range for a total of 24.673 kg which werecollected and catalogued by A. Ashworth and David P.Ambrose (National University of Lesotho), one stone of
A212 S. S. Russell et al.
1.020 kg held by Dr. Molisana Molisana (National Universityof Lesotho), 5 stones acquired by the National Museum ofLesotho in Maseru, some were collected by the GeologyDepartment, Free State University, Bloemfontein, and severalothers purchased by members of the public. Mineralogy andclassification (W. U. Reimold, Wits; P. C. Buchanan, NIPR):most freshly cut slices from several stones show ahomogeneous beige to light-grey lithology speckled withabundant and heterogeneously distributed (20% to, inexceptional cases, >50 vol%) metal particles; some are cross-cut by dark shock veinlets and show brecciated structure withlight grey matrix surrounding lighter colored, well-roundedinclusions; chondrules distinctly recognizable; olivineFa17.4 ± 0.8; shock stage S2/3. Specimens (numbers in bracketsrefer to the catalog by A. Ashworth and David P. Ambrose):207 g (stone #58), Bleloch Museum, School of Geosciences,University of the Witwatersrand; 294 g (stone #59), 309 g(stone #60), 342 g (stone #61) plus four thin sections, one thinsection of stone #58, Wolf Uwe Reimold (Wits); 67 g (stone#54), 45 g (stone #111), 110 g (stone #56), 146 g (stone #193),16 g (stone #356), 15 g (stone #359), one thin section of stone#59 and #60, Paul C. Buchanan (NIPR); 127 g (stone #57),Christian Koeberl (UVienna); 5 stones of unknown weights,National Museum of Lesotho in Maseru; additional materialat the Geology Department, Free State University,Bloemfontein.
Tifariti 26°30′N, 10°30′WWestern SaharaFound 2002 January 2Ordinary chondrite (L6)
A 5.4 g stone devoid of fusion crust was found near theTifariti army post by Mr. Valentino Luppi, a member of anItalian humanitarian mission in the Saharawi territories.Classification and analyses (R. Serra, OAM; L. Folco, MNA-SI): granoblastic texture; olivine, Fa24, pyroxene, Fs21Wo1.5;shock stage, S3; weathering grade, W5. Specimens: mainmass OAM; thin section MNA-SI.
Tiffa 007, see Saharan meteorites from Niger
Twodot, see American meteorite finds
Umm as Samim, see Oman meteorites
Yamato (Y), see Antarctic NIPR meteorites
Zinder ~13°47′N, 8°58′ENigerFound 1999Pallasite (pyroxene-rich)
A 46 g, mostly crusted meteorite, was found in a field outsideZinder, Niger and purchased in 2001 by a mineral collector.Precise site location is unknown. Description and
classification (J. Wittke and T. Bunch, NAU): Unusually highabundance of orthopyroxene; modal analyses: opx, 28 vol%;ol, 27 vol%; metal, 44 vol%; sulfide, 1.0 vol%; chromite, <0.1 vol%. Olivine, mg# = 89, molar Fe/Mn = 32; opx, mg# =87, Wo2.2; molar Fe/Mn = 20. Metal, Ni = 7.15 wt%; Co =0.58 wt%. Chromite, Cr2O3 = 60.1 wt%; molar Cr/(Cr + Al) =0.85. Weathering grade, W1. Specimens, main mass withowner; type specimen 5.8 g, one polished mount, and one thinsection, NAU (original weight was 9.54 g)
Zlin 49°15′N, 17°40′ESouth Moravia, Czech RepublicOrdinary chondrite (H4)
A 3.3 g stone was found in Zlin in the collection of Mr.Jaroslav Novak, purchased before 1939. Its provenance isunknown. Classification (Jakuba Haloda and Patricie Tycova,PCU): Olivine, Fa18.5, Ca in olivine 0.04 wt%, MnO inolivine 0.4%. Pyroxene, Fs16.3Wo1.2. Accessory mineralsinclude chromite, merillite, chlorapatite, troilite, andcristobalite-bearing objects. Specimens: main mass Mr.Novak; type specimen 1.8 g plus a thin section, PCU.
Acknowledgments–This bulletin was prepared by theMeteorite Nomenclature Committee of the MeteoriticalSociety under the Principal Editorship of Sara Russell.Members for 2003 are L. Folco (Associate Editor for Africa),J. Goswami, M. Grady (Associate Editors for Oman), J.Grossman (Chair), R. Harvey, R. Jones (Associate Editor forthe Americas), M. Kimura, D. Kring, J. Koblitz, Y. Lin, T.McCoy (Associate Editors for Antarctica), M. Nazarov, H.Palme, and J. Zipfel (Associate Editors for Northwest Africa).
REFERENCES
Benedix G. K., McCoy T. J., Keil K., Bogard D. D., and Garrison D.H. 1998. A petrologic and isotopic study of winonaites: Evidencefor early partial melting, brecciation, and metamorphism.Geochimica et Cosmochimica Acta 62:2535–2553.
Clarke R. S. Jr., Appleman D. E., Ross, D. R. 1981. An Antarctic ironmeteorite contains preterrestrial impact-produced diamond andlonsdaleite. Nature 291:396–398.
Keil K. 1968. Mineralogical and chemical relationships amongenstatite chondrites. Journal of Geophysical Research 73:6945–6976.
Rocchette P., Sagnotti L., Bourot-Denise M., Consolmagno G., FolcoL., Gattacceca J., Osete M. L., and Pesonen L. 2003. Magneticclassification of stony meteorites: 1. Ordinary chondrites.Meteoritics & Planetary Science 38(2):251–268.
Spurny P., Oberst J., and Heinlein D. 2003. Photographic observationof Neuschwanstein, a second meteorite from the orbit of thePribram chondrite. Nature 423:151–155.
Stöffler D., Keil K., and Scott E. R. D. 1991. Shock metamorphismof ordinary chondrites. Geochimica et Cosmochimica Acta 55:3845–3867.
Wasson J. T. and Kallemeyn G. W. 2002. The IAB iron-meteoritecomplex: A group, five subgroups, numerous grouplets, closelyrelated, mainly formed by crystal segregation in rapidly coolingmelts. Geochimica et Cosmochimica Acta 66:2445–2473.
Meteoritical Bulletin No. 87 A213
Wlotzka F. 1993. A weathering scale for the ordinary chondrites(abstract). Meteoritics 28:460.
Zhang Y., Benoit P. H., Sears D. W. G. 1995. The classification andcomplex thermal history of the enstatite chondrites. Journal ofGeophysical Research 100:9417–9438.
M. Zbik and A. Pring. Forthcoming. The Myrtle Springs meteorite:An H4 chondrite from South Australia. Transactions of the RoyalSociety of South Australia.
ABBREVIATIONS FOR ANALYSTS AND SPECIMEN LOCATIONS
These abbreviations are used in the “Info” columns of tablesin The Meteoritical Bulletin. Unless specifically noted, alltype specimens are at the home institution of the first listedanalyst and main masses are with anonymous finders.
Bart1: Classified: Bart; purchased U. Eger; type specimen,Vernad; specimen, Bart; main mass, U. Eger.Bart2: Classified: Wlotzka, MPI and Bart; purchased. Fectay;type specimen, MPI; main mass, Bart.Bart3: Classified: Bart; purchased Fectay; type specimen,Vernad; main mass, Bart.Bart4: Classified: F. Melcher, Hanover and Bart; typespecimen, VernadBart5: Classified: Bart and P. Appel, Kiel; type specimen,VernadBart6: Classified: A. Pack, Köln and Bart; type specimen,VernadBart7: Classified: F. Melcher, Hanover and Bart; typespecimen, WitsBart8: Classified: Bart; type specimens, Mün (6 g); Vernad(15 g); main mass, Bart.Bart9: Classified: Bart; type specimens, Mün (10 g); Vernad(11 g); main mass, Bart.Bart10: Classified: Bart; type specimen, Vernad (20 g); mainmass, 300 g, Gehler; 140 g, Bart.Be1: Classified: A. Greshake, MNB and M. Kurz, Kurz; mainmass, Kurz.Be2: Classified: A. Greshake, MNB and M. Kurz, Kurz.Be3: Classified: A. Greshake, MNB and M. Kurz, Kurz; mainmass, E. Sommer, 68809 Neulussheim.Be4: Classified: A. Greshake, MNB; main mass, StefanRalew, Kunibertstraße 29, 12524 Berlin.Be5: Classified: A. Greshake, MNB, J. Otto, Industriestraße33, 79194 Gundelfingen, Germany, and M. Kurz, Kurz.Be6: Classified: A. Greshake, MNB and M. Kurz; main mass,Peter Jäger, Apolda, Germany.Be7: Classified: A. Greshake, MNB.Bern1: Classified: E. Gnos, B. Hofmann and A. Al-Kathiri,NMB.CU1: Classified: M. Weisberg, KCCU; type specimen,AMNH.Frei1: Classified: J. Otto and A. Ruh, Frei.Ha1: Classified: P. Sipiera and K. J.Cole, Harper; typespecimen, PSF; found by Pelison; main mass, Pelison.
Ha2: Classified: P. Sipiera and K. J. Cole, Harper; typespecimen, PSF; found by Gomet on sandy soil while crossingerg Rebiana between Koufra and Tazurbu; main mass, Gomet.Ha3: Classified: P. Sipiera, Harper; main masses and typespecimens, PSFHam1: Classified: J. Schlüter, Ham; main mass, IndustrialResearch Center, Tripoli, LibyaHam2: Classified: J. Schlüter, Ham; main mass, Dr. S. Buhl,Berlin; finder Tuareg Souleymane Icha.JSC1: Classified: M. Zolensky, JSC; type specimen, SI; mainmass, Bessey.K1: Classified: G. Weckwerth, Köln, and Bart; type specimen,NHMV; other specimens, 20 g, Gehler; 10 g, Bart.La1: Classified: A. Rubin, UCLA; main mass, Hupé.La2: Classified: J. Wasson, UCLA; main mass, Cilz.La3: Classified: P. Warren, UCLA; main mass, Cilz.La4: Classified: A. Rubin, UCLA; purchased by Gessler fromMike Pimentel (who directed a local search in Morocco);main mass, Gessler.La5: Classified: A. Rubin, UCLA; purchased by Gessler fromBessey; main mass, Gessler.La6: Classified: A. Rubin, UCLA; purchased by Gessler fromthe finder Labenne; main mass, Gessler.La7: Classified: A. Rubin, UCLA and G. Benedix, WashU;purchased by Gregory; type specimen, ROM, and 18 g,UCLA.La8: Classified: A. Rubin, UCLA; main mass, R. MatsonLa9: Classified: A. Rubin, UCLA; main mass, R. VerishLa10: Classified: A. Rubin, UCLA; main mass, Cilz, J.SchwadeMIT1: Classified: S. Singletary, MIT; type specimen, TCU;main mass, Bessey.MP1: Classified: J. Zipfel, MPI; main mass, Kraus.MP2: Classified: J. Zipfel, MPI; main mass, R. and A.Adnane.Mün1: Classified: A. Sokol and A. Bischoff, Mün; purchasedby Chin from Bessey; main mass, Chin.Mun2: Classified: A. Sokol and A. Bischoff, Mün.Mün3: Classified: A. Sokol and A. Bischoff, Mün, data ±1mol. %; main mass JNMC. NAU1: Classified: T. Bunch and J. Wittke, NAU; main mass,purchaser.NAU2: Classified: T. Bunch and J. Wittke, NAU; main mass,Hupé.NAU3: Classified: T. Bunch and J. Wittke, NAU.Pa1: Classified: M. Bourot-Denise, MNHNP and R. Rochette,CEREGE; main mass, Chin.Pa2: Classified: M. Bourot-Denise, MNHNP; main mass, P.Thomas.Pa3: Classified: M. Bourot-Denise, MNHNP; main mass,Fectay.Pa4: Classified: M. Bourot-Denise, MNHNP; main mass, G.Merlier.Pa5: Classified: M. Bourot-Denise, MNHNP; main mass,MNHNP.
A214 S. S. Russell et al.
Pa6: Classified: M. Bourot-Denise, MNHNP; finder Carion.Pa7: Classified: C. Fieni andC. Perron, MNHNP; main mass,Fectay.Pa8: Classified: B. Devouard and J.-L. Devidal, UBP, and B.Zanda, MNHNP; type specimen, MNHNP; main masses withfinders, F. Beroud and C. Boucher.Pa9: Classified: B. Devouard and J.-L. Devidal, UBP, B.Zanda and M. Denise, MNHNP; main mass with finders, F.Beroud and C. Boucher.Pa10: Classified: M. Bourot-Denise, MNHNP; finder, Mr. andMrs Letallec.Pa11: Classified: M. Bourot-Denise, MNHNP; finder, B.Dejonghe.Pa12: Classified: M. Bourot-Denise, MNHNP; finderLabenne.Pad1: Classified: R. Carampin and A. M. Fioretti, UPad;specimens at MNA-SI.PCU1: Classified: J. Haloda and P. Tycova, PCU.Pr1: Classified: V. Moggi Cecchi and G. Pratesi, MSP; mainmass, Chin.Pr2: Classified: V. Moggi Cecchi and G. Pratesi, MSP.Pr3: Classified: V. Moggi Cecchi and G. Pratesi, MSP; finder,G. Pratesi, MSP.Rom1: Classified: A. Maras and M. Macrì, URoma;specimens at MNA-SI.Sn1: Classified: A. Burroni and L. Folco, MNA-SI.Sn2: Classified: A. Burroni, L. Folco, MNA-SI; thin section,MNA-SI, type specimen, OAM.Sn3: Classified: A. Burroni, L. Folco, MNA-SI; thin section,MNA-SI, main mass, OAM.Sn4: Classified: A. Burroni, C. Ferraris and L. Folco; allspecimens at MNA-SI.UPVI1: Classified: A. Jambon, UPVI, J.-A. Barrat, UAng andO. Boudouma, UPVI; main mass with dealer (MoroccanImport, Asnieres, France).UPVI2: Classified: A. Jambon and O. Boudouma, UPVI, J.-A. Barrat, UAng and M. Bohn, Brest; type specimen, ENSL;main mass, Fectay.UWS1: Classified: A. Irving, UWS; main mass, ROM.UWS2: Classified: A. Irving and S. Kuehner, UWS; mainmass, Hupé.Vn1: Classified: F. Brandstätter and M. Bukovanska, NHMV;main mass, Fectay.Vn2: Classified: F. Brandstätter, NHMV; main mass, Pani.Vr1: Classified: S. Afanasiev, Vernad, analyzed by N.Kononkova, Vernad.Vr2: Classified: S. Afanasiev, Vernad, analyzed by A. Ulianov,MwSU; additional type specimen at MwSU.Vr3: Classified: M. Nazarov, Vernad, L. Taylor, UTenn.Vr4: Classified and analyzed by D. Badyukov, VernadVr5: Classified: S. Afanasiev, Vernad, analyzed by A.Ulianov, MwSU. TL measurements A. I. Ivliev, Vernad.Vr6: Classified: S. Afanasiev, Vernad, analyzed by N.Kononkova, Vernad. TL measurements, A. I. Ivliev, Vernad.
Vr7: Classified: S. Afanasiev, Vernad, analyzed by C. Lorenz,Vernad.Vr8: Classified: C. Lorenz, Vernad.Vr9: Classified: S. Demidova, Vernad.Vr10: Classified: S. Demidova, Vernad, L. Taylor, UTenn.Vr11: Classified: S. Demidova, Vernad, G. Kurat, NHMV.Vr12: Classified: M. Ivanova, Vernad, L. Taylor, UTenn.Vr13: Classified: C. Lorenz, M. Ivanova, Vernad.Vr14: Classified: M. Ivanova, Vernad.Vr15: Classified at Vernad.Vr16: Classified: Bart; type specimen, Vernad, main mass,Bart.Vr17: Classified: Bart; type specimen, Vernad, main mass, A.Gehler (Wolfburg, Germany).Vr18: Classified: S. Afanasiev, M. Nazarov, Vernad.Vr19: Classified: S. Afanasiev, Vernad; main mass, Farmer.
ADDRESSES OF METEORITE COLLECTIONS AND RESEARCH FACILITIES
AMNH: American Museum of Natural History, New York,NY 10024, USA.
Bart: Bartoschewitz Meteorite Laboratory, Lehmweg 53, D-38518 Gifhorn, Germany.
Bessey: Dean Bessey, Box 6306, Stn A, Toronto Ontario,Canada, M5W 1P7.
Brest: IFREMER, Brest BP 7029280 Plouzane, France.Carion: Alain Carion, 6 rue Jean du Bellay, 75004 Paris,
France.CEREGE: Centre Européende Recherche et d’Enseignement
de Géosciences de l’Environment, Aix en Provence,Cedex 4, France.
Chiba: Chiba Institute of Technology, Tsudanuma,Narashino, Chiba 275–0016, Japan.
Chin: Matteo Chinellato, Via Triestina, 126/A-30030 Tessera,Venezia, Italy.
Cilz: Marlin Cilz, Montana Meteorite Lab, Box 1063, Malta,MT 59538, USA.
CIW: Carnegie Insitution Washington, GeophysicalLaboratory, 5251 Broad Branch Rd., NW, WashingtonDC 20015, USA.
DMNH: Denver Museum of Natural History, City Park,Denver, CO 80205, USA.
EMTT: Etudes Métallurgiques et de Traitement Thermique,Parc du Chater-Bât. B, 1, avenue du Chater, 69340Francheville, France.
ENSL: Ecole Normale Supérieure de Lyon, Laboratoire deSciences de la Terre, 46 allée d’Italie 69364 Lyon Cedex,France.
Farmer: Mike Farmer, 1001 W. St Mary, Tucson, AZ 85745,USA.
Fectay: Bruno Fectay and Carine Bidaut, La Memoire de laTerre SARL Rue de la Mairie, 39240 La Boissiere,France.
Meteoritical Bulletin No. 87 A215
FMNH: Field Museum of Natural History, Chicago, IL60605, USA.
Frei: Institut für Mineralogie, Universität Freiburg,Albertstrasse 23b, 79104 Freiburg, Germany.
Gehler: Reichhenberger Ring 3, D-38440 Wolfsburg,Germany.
Gessler: N. Gessler, Box 706, 22148 Monte Vista Road,Topanga, CA 90290–0706, USA.
GO: Griffith Observatory, 2800 East Observatory Road, LosAngeles, CA 90027–1255 USA.
Gomet: D. Gomet, lieu dit Lahouratte, 40180 Herm, France.Ham: Mineralogical Museum, Universität Hamburg,
Grindelallee 48, D-20146 Hamburg, Germany.Harper: Planetary Studies Foundation, c/o Harper College,
Schmitt Meteorite Research Group, 1200 W. AlgonquinRd., Palatine, IL 60067, USA.
Hupé: G. and A. Hupe, 2616 Lake Youngs Court SE, Renton,WA 98058, USA.
Jensen: Jensen Meteorites, 16730 E Ada Pl., Aurora, CO80017–3137, USA.
JSC: Johnson Space Center, Houston, TX 77058, USA.KCCU: Kingsborough College, City University of New York,
Brooklyn, NY 11235, USA.Kiel: Mineralogy Department, Universität Kiel, D-24098,
Kiel, Germany.Köln: Universität zu Köln, Institut für Mineralogie und
Geochemie, Zülpicher Straße 49 b, 50674 Köln,Germany.
Kraus: Thomas Kraus, German-Space-Shop, Büchelstr. 87,53227 Bonn, Germany.
Kurz: M. Kurz, Schillerstrasse 7, D-34626 Neukirchen,Germany.
KyuU: Department of Earth and Planetary Science, KyushuUniversity Hakozaki, Higashi-ku, Fukuoka-shi 812–8581, Japan.
Labenne: Labenne Meteorites, 16 Boulevard Gambetta,02700 Tergnier, France.
Matson: Rob Matson, 8 Merano Ct., Newport Coast, CA92657, USA.
MIT: Department of Earth and Planetary Sciences, 54–1224,Massachusetts Institute of Technology, Cambridge, MA02139, USA.
MNA-SI: Mus. Naz. dell’Antartide, Univ. di Siena, ViaLaterina 8, I-53100 Siena, Italy.
MNB: Museum für Naturkunde, Invalidenstrasse 43, D-10115Berlin, Germany.
MNHNP: Museum National d’Histoire Naturelle, Paris,France.
Monash: School of Geosciences, Monash University,Victoria, 3800 Australia.
MPI: Max-Planck-Inst. Chemie, Abt. Kosmochem, Postf.3060, D-55020 Mainz, Germany.
MPI-K: Max-Planck-Institut Kernphysik, Saupfercheckweg1, D-69117 Heidelberg, Germany.
MSNP: Museo di Storia Naturale, Univ. di Pisa, Via Roma 53,I-56100 Calci (Pisa), Italy.
MSP: Museo di Scienze Planetarie, Via Galcienese, I-59100Prato, Italy.
MwSU: Department of Geology, Moscow State University,Vorobjovy Gory, Moscow, 119899, Russia.
Mün: Institut für Planetologie, Wilhelm-Klemm-Str. 10,48149 Münster, Germany.
NAU: Northern Arizona University, Flagstaff, AZ 86011,USA.
NHM: Natural History Museum, Cromwell Road, LondonSW7 5BD, UK.
NHMV: Naturhistorisches Museum, Postfach 417, A-1014Wien, Austria.
NIPR: National Institute of Polar Research, 9–10, Kaga 1-chome, Itabashi-ku, Tokyo 173–8515 Japan.
NMB: Bern Natural History Museum, Bernastrasse 15, CH-3005 Bern, Switzerland.
NSMT: National Science Museum, 3–23–1 Hyakunin-cho,Shinjuku-ku, Tokyo, 169–0073, Japan.
OAM: Osservatorio Astronomico e Museo “Giorgio Abetti”in San Giovanni in Persiceto, Bologna, Italy.
OU: Planetary and Space Science Research Institute, OpenUniversity, Milton Keynes, UK.
Pani: A. Pani, Meteorites-Minerals-Fossils, Lassallestr. 4/20,A-1020 Vienna, Austria.
PCU: Charles University, Faculty of Science, Institute forCheochemistry, Mineralogy and Mineral Resources,Albertov 6, 128 43 Prague 2, Czech Republic.
Pelisson: Richard and Roland Pelisson, 270 Rue de laCascade, 38660 La Terrasse, France.
PSF: James M. DuPont Collection, Planetary StudiesFoundation, 4405 Three Oaks Road, Suite B, CrystalLake, Illinois 60014, USA.
RIKEN: Institute of Phys. and Chem. Research, 2-1Hirosawa, Wako Saitama 351–0198, Japan.
ROM: Royal Ontario Museum, 100 Queen’s Park, Toronto,Ontario M5S 2C6, Canada.
SAM: Department of Mineralogy, South Australian Museum,North Terrace, Adelaide South Australia 5000.
SI: Department of Mineral Sciences, NHB-119, NationalMuseum of Natural History, Smithsonian Institution,Washington, DC 20560, USA.
Tunis: Départment du Geologie, Faculté de Sciences deTunis, Campus Universitaire, 1060 Tunis, Tunisie.TCU: Oscar E. Monnig Collection, Dept. of Geology, Texas
Christian University, Ft. Worth, Texas 76129.UAng: Université d’Angers, Faculté des Sciences, 2 bd
Lavoisier, 49045 Angers Cedex, France.UChi: Enrico Fermi Institute, University of Chicago,
Chicago, IL 60637, USA.UCLA: Institute of Geophysics and Planetary Physics,
University of California, Los Angeles, CA 90095–1567,USA.
A216 S. S. Russell et al.
UNM: Institute of Meteoritics, Department of Earth andPlanetary Sciences, University of New Mexico,Albuquerque, NM 87131, USA
UPad: C. N. R., I-35122, Padova, Italy.UBP: Université Blaise Pascal, Clermont-Ferrand, France.UPVI: Université Pierre & Marie Curie (Paris VI), 4 Place
Jussieu, 75005 Paris, France.URoma: Dpt. di Scienze della Terra, Università di Roma “La
Sapienza,” I-00185, Italy.UTenn: Planetary Geosciences Institute, Department of
Geological Sciences, University of Tennessee,Knoxville, TN 37996, USA.
UTok: 7–3–1 Hongo, Bunkyo-ku, Tokyo 113–0033, JapanUVienna: Institute of Geochemistry, University of Vienna, A-
1090 Vienna, Austria.UWO: University of Western Ontario, London, Ontario N6A
3KT, Canada.
UWS: Department of Geological Sciences, University ofWashington, Box 351310, Seattle, Washington 98195,USA.
Verish: Meteorite Recovery Foundation, PO Box 237,Sunland, CA 91040, USA.
Vernad: Vernadsky Institute of Geochemistry and AnalyticalChemistry, Russian Academy of Sciences, Kosygin Str.19, Moscow 117975, Russia
Vic: Museum Victoria, GPO Box 666E, Melbourne, Victoria3001, Australia.WAM: Western Austr. Museum, Francis Street, Perth, Western
Australia 6000, Australia.WashU: McDonnell Center for Space Sciences, Washington
Univ., One Brookings Drive, St. Louis, MO 63130, USA.Wits: Department of Geology, University of Witwatersrand, P.
O. Wits 2050 Johannesburg, South Africa.
Meteoritical Bulletin No. 87 A217
Tabl
e 1.
Ord
inar
y ch
ondr
ite fi
nds
from
the
Am
eric
as.
Nam
eFi
nd s
iteC
ount
y, S
tate
Latit
ude
Long
itude
(W)
Mas
s(g
)D
ate
foun
dPc
sC
lass
Shoc
kW
GFa (m
ol%
)Fs (m
ol%
)W
o(m
ol%
)Fi
nder
Type
spec
(g)
Info
a
a See
“A
bbre
viat
ions
for a
naly
sts a
nd sp
ecim
en lo
catio
ns.”
Nor
th A
mer
ica
(USA
)B
luew
ing
008
dese
rtPe
rshi
ng, N
V40
°16.
774′
N11
8°56
.785′
451.
708
/13/
2001
1H
5S2
W3
18.8
––
Mat
son
21.7
La8
Har
per D
ry L
ake
001
dry
lake
San
Ber
nard
ino,
CA
35°3
.061′N
117°
18.4
03′
13.0
09/1
7/19
991
LL3
S2W
329
pk
––
Veris
h3.
8La
9H
arpe
r Dry
Lak
e 00
2dr
y la
keSa
n B
erna
rdin
o, C
A35
°3.0
4′N
117°
18.0
57′
12.0
09/1
7/19
991
H6
S3W
319
.4–
–Ve
rish
3.6
La9
Har
per D
ry L
ake
003
dry
lake
San
Ber
nard
ino,
CA
35°2
.55′
N11
7°18
.502′
95.0
09/1
7/19
991
L6S3
W3
24.9
––
Veris
h20
.9La
9H
arpe
r Dry
Lak
e 00
4dr
y la
keSa
n B
erna
rdin
o, C
A35
°3.3
1′N
117°
18.1
54′
37.0
10/0
7/19
991
LL3
S2W
229
pk
––
Veris
h10
.1La
9H
arpe
r Dry
Lak
e 00
5dr
y la
keSa
n B
erna
rdin
o, C
A35
°3.0
38′N
117°
18.1
13′
24.0
10/0
7/19
991
H6
S3W
319
.4–
–Ve
rish
5.2
La9
Har
per D
ry L
ake
006
dry
lake
San
Ber
nard
ino,
CA
35°2
.833′N
117°
18.4
51′
26.0
11/1
2/19
991
H6
S2W
519
.4–
–Ve
rish
6.5
La9
Har
per D
ry L
ake
007
dry
lake
San
Ber
nard
ino,
CA
35°2
.972′N
117°
15.8
14′
166.
709
/03/
2000
1H
5S2
W4
18.4
––
Veris
h24
.2La
9H
arpe
r Dry
Lak
e 00
8dr
y la
keSa
n B
erna
rdin
o,C
A35
°3.1
16′N
117°
15.6
83′
12.5
09/0
3/20
002
H6
S4W
320
.0–
–Ve
rish
2.5
La9
Twod
othi
llsid
eW
heat
land
, MT
46°4
2′N
110°
08′
2140
010
/25/
1999
1H
6S2
W3
18.9
––
Elk
hunt
er23
9La
10
Sout
h A
mer
ica
(Arg
entin
a)Pi
tino
Cam
po d
el
Cie
lost
rew
n fie
ld
Sant
iago
del
Est
ero
27º2
8′S
60º3
5′16
67.0
2002
1H
5S4
W2
15.8
14.9
1.4
Farm
er42
.4V
r19
Tabl
e 2.
Met
eorit
es fr
om F
ront
ier M
ount
ain
colle
cted
by
the
Italia
n PN
RA
in D
ecem
ber 2
000.
Nam
eLa
titud
e(S
)Lo
ngitu
de(E
)M
ass
(g)
Piec
esC
lass
Shoc
kW
GFa (m
ol%
)Fs (m
ol%
)C
omm
ents
aIn
fob
FRO
010
0672
°57′
06′′
160°
30′3
3′′
5.6
1H
5S1
W1
1916
–Pa
d1FR
O 0
1007
72°5
7′07′′
160°
30′3
4′′
2.6
1L4
S2W
023
17–
Pad1
FRO
010
0872
°57′
07′′
160°
30′3
4′′
3.2
1L3
S2W
022
12–2
0–
Pad1
FRO
010
0972
°57′
10′′
160°
30′4
1′′
6.7
1H
6S2
W2
1816
–Pa
d1FR
O 0
1010
72°5
7′09′′
160°
30′2
7′′
0.7
1H
5S2
W1
1916
–Pa
d1FR
O 0
1011
72°5
7′49′′
160°
32′1
2′′
11.6
1H
5S4
W0
1916
–Pa
d1FR
O 0
1012
72°5
8′16′′
160°
20′0
2′′
19.2
1U
re–
––
–Se
e se
para
te e
ntry
Pad1
FRO
010
1372
°59′
14′′
160°
24′2
3′′
11.4
1H
3S2
W2
1916
–Pa
d1FR
O 0
1014
72°5
9′20′′
160°
24′1
8′′
3.6
1H
3/4
S3W
119
15–
Pad1
FRO
010
1572
°59′
20′′
160°
24′2
1′′
1.2
1H
5S4
W1
1917
–Pa
d1FR
O 0
1016
72°5
9′21′′
160°
24′2
1′′
1.6
1H
3S4
W2
1–22
1–31
–Pa
d1FR
O 0
1017
72°5
9′20′′
160°
24′1
9′′
1.5
1H
3–4
S4W
12–
294–
22br
Pad1
FRO
010
1872
°59′
20′′
160°
24′1
7′′
1.2
1H
5S3
W1
1917
brPa
d1FR
O 0
1019
72°5
9′24′′
160°
24′1
2′′
1.9
1H
3–6
S3/4
W1
1917
brPa
d1FR
O 0
1020
72°5
9′23′′
160°
24′1
2′′
2.3
1H
6S2
W1
2017
–Pa
d1FR
O 0
1031
72°5
9′24′′
160°
24′1
4′′
9.0
1H
3–6
S2W
118
–23
17–2
2br
Rom
1FR
O 0
1032
72°5
9′27′′
160°
24′1
2′′
27.0
2H
3S2
W1
8–31
7–25
–R
om1
FRO
010
3372
°59′
25′′
160°
24′0
7′′
6.2
1H
3–6
S2W
219
–24
17–2
4br
Rom
1FR
O 0
1034
72°5
9′20′′
160°
24′1
9′′
1.0
1H
3S3
W2
19–2
216
–18
–R
om1
FRO
010
3572
°59′
20′′
160°
24′1
9′′
2.6
1H
3S3
W1
16–2
28–
19br
Rom
1FR
O 0
1036
72°5
9′20′′
160°
24′1
9′′
0.8
1H
3-6
S2W
216
–32
4–22
brR
om1
FRO
010
3772
°59′
20′′
160°
24′1
9′′
18.2
1H
3-6
S4W
217
–22
10–1
6br
Rom
1
A218 S. S. Russell et al.
Tabl
e 2.
Met
eorit
es fr
om F
ront
ier M
ount
ain
colle
cted
by
the
Italia
n PN
RA
in D
ecem
ber 2
000.
Continued.
Nam
eLa
titud
e(S
)Lo
ngitu
de(E
)M
ass
(g)
Piec
esC
lass
Shoc
kW
GFa (m
ol%
)Fs (m
ol%
)C
omm
ents
aIn
fob
FRO
010
3872
°59′
20′′
160°
24′1
9′′
3.1
2H
3S3
W2
9–19
9–23
brR
om1
FRO
010
3972
°59′
22′′
160°
24′2
6′′
22.0
1H
3/4
S3W
216
17–
Rom
1FR
O 0
1040
72°5
9′20′′
160°
24′1
9′′
13.6
1H
3/4
S2W
115
16br
Rom
1FR
O 0
1041
72°5
9′27′′
160°
24′2
7′′
4.9
1H
3–6
S4W
312
–19
6–17
brR
om1
FRO
010
4272
°59′
21′′
160°
24′2
6′′
2.0
1H
3–5
S4W
319
16v,
br
Rom
1FR
O 0
1044
72°5
9′21′′
160°
24′1
9′′
26.6
1H
5S2
W2
1817
–Sn
4FR
O 0
1045
72°5
9′21′′
160°
24′1
9′′
8.9
1H
4S2
W1
1816
–Sn
4FR
O 0
1046
72°5
9′22′′
160°
24′1
0′′
5.1
1H
4S2
W2
1816
–Sn
4FR
O 0
1047
72°5
9′23′′
160°
24′1
6′′
0.9
1H
4/5
S2W
220
18–
Sn4
FRO
010
4872
°59′
22′′
160°
24′2
2′′
6.8
1H
3/4
S2W
1/2
20–2
310
–21
–Sn
4FR
O 0
1049
72°5
9′22′′
160°
24′2
2′′
44.1
1H
3/4
S1W
1/2
1–25
5–18
–Sn
4FR
O 0
1050
72°5
9′24′′
160°
24′2
6′′
3.2
1H
4–6
S1W
1/2
16–2
612
–17
brSn
4FR
O 0
1051
72°5
9′21′′
160°
24′1
8′′
10.6
1H
4S2
W2
1917
–Sn
4FR
O 0
1053
72°5
9′23′′
160°
24′2
0′′
8.4
1H
3S1
/2W
114
–35
14–3
5–
Sn4
FRO
010
5472
°59′
18′′
160°
24′2
6′′
1.3
1H
3S1
/2W
21–
151–
15–
Sn4
FRO
010
5572
°57′
12′′
160°
27′2
9′′
14.0
1L3
S4W
111
–19
11–1
9–
Sn4
FRO
010
5672
°59′
17′′
160°
24′2
2′′
0.8
1H
3S1
/2W
13–
243–
24–
Sn4
FRO
010
5772
°59′
19′′
160°
24′2
3′′
15.2
1H
3–6
S1-4
W1
6–17
2–18
brSn
4FR
O 0
1058
72°5
9′20′′
160°
24′2
1′′
1.3
1H
4S3
W2
1816
–Sn
4FR
O 0
1059
72°5
9′20′′
160°
24′2
2′′
5.4
1H
3S1
W1
8–17
14–1
6–
Sn4
FRO
010
6072
°59′
22′′
160°
24′1
6′′
1.8
1H
6S1
W1
1917
–Sn
4FR
O 0
1061
72°5
9′24′′
160°
24′2
6′′
4.1
1H
3S2
W1
5–17
4–16
brSn
4FR
O 0
1063
72°5
9′16′′
160°
24′3
1′′
0.7
1H
3S2
W1
8–19
3–18
brSn
4FR
O 0
1064
72°5
9′17′′
160°
24′3
0′′
1.2
1L6
S5W
224
22v
Sn4
FRO
010
6572
°59′
17′′
160°
24′3
0′′
1.7
1H
3S2
W1
10–2
07–
18br
Sn4
FRO
010
6672
°59′
19′′
160°
24′2
6′′
5.6
1H
3S2
W1
8–18
9–15
brSn
4FR
O 0
1067
72°5
9′21′′
160°
24′2
4′′
8.4
1H
3S2
W2
2–30
16–2
0–
Sn4
FRO
010
6872
°59′
23′′
160°
24′1
8′′
13.6
1H
3–6
S2W
18–
183–
31br
Sn4
FRO
010
6972
°59′
24′′
160°
24′
23′′
5.4
1H
5S1
W1
17,1
17,8
–Sn
4FR
O 0
1070
72°5
9′24′′
160°
24′2
3′′
6.6
1H
3S1
W2
5–23
5–21
brSn
4FR
O 0
1071
72°5
9′23′′
160°
24′0
9′′
1.7
1H
4–6
S2W
220
18br
Sn4
FRO
010
7272
°59′
24′′
160°
24′1
4′′
6.5
1H
5S1
W2
2018
–Sn
4FR
O 0
1073
72°5
9′24′′
160°
24′1
1′′
1.0
1H
3–6
S1W
11–
295–
19br
Sn4
FRO
010
7472
°59′
24′′
160°
24′1
0′′
3.0
1H
3S1
W2
1–23
7–19
brSn
4FR
O 0
1075
72°5
9′26′′
160°
24′2
2′′
5.5
1H
3S1
–3W
217
–20
6–17
brSn
4FR
O 0
1076
72°5
9′26′′
160°
24′1
8′′
2.1
1H
4/5
S2W
221
19v
Sn4
FRO
010
7772
°57′
10′′
160°
24′4
6′′
9.7
1H
6S4
W2
1816
–Sn
4FR
O 0
1078
72°5
7′15′′
160°
27′0
7′′
15.0
1L6
S5W
227
23–
Sn4
FRO
010
7972
°57′
09′′
160°
26′5
9′′
0.9
1L6
S4W
226
22–
Sn4
FRO
010
8072
°57′
07′′
160°
27′1
5′′
0.4
1H
6S3
W2
2019
brSn
4FR
O 0
1081
72°5
9′23′′
160°
24′2
6′′
3.4
1H
3–6
S1W
218
–22
5–18
brSn
4
Meteoritical Bulletin No. 87 A219
Tabl
e 2.
Met
eorit
es fr
om F
ront
ier M
ount
ain
colle
cted
by
the
Italia
n PN
RA
in D
ecem
ber 2
000.
Continued.
Nam
eLa
titud
e(S
)Lo
ngitu
de(E
)M
ass
(g)
Piec
esC
lass
Shoc
kW
GFa (m
ol%
)Fs (m
ol%
)C
omm
ents
aIn
fob
FRO
010
8272
°59′
23′′
160°
24′2
6′′
5.0
1H
3–6
S3–5
W1
1813
v, b
rPa
d1FR
O 0
1083
72°5
9′23′′
160°
24′2
4′′
11.1
1H
5–6
S3W
120
18br
Pad1
FRO
010
8572
°59′
20′′
160°
24′2
8′′
4.2
1H
4S2
W1
1816
–Pa
d1FR
O 0
1086
72°5
8′24′′
160°
28′2
9′′
9.8
1H
5S4
W0
1916
–Pa
d1FR
O 0
1087
72°5
7′15′′
160°
26′5
1′′
76.4
1H
5S3
W1
1917
–Pa
d1FR
O 0
1088
72°5
7′08′′
160°
27′1
9′′
11.1
1U
re–
––
–Se
e se
para
te e
ntry
Pad1
FRO
010
8972
°57′
08′′
160°
27′2
0′′
2.1
1U
re–
––
–Se
e se
para
te e
ntry
Pad1
FRO
010
9072
°57′
08′′
160°
27′3
7′′
9.9
1LL
(L)3
S2W
00.
5–35
1–32
–Pa
d1FR
O 0
1091
72°5
7′07′′
160°
27′1
6′′
1.6
1L4
S2W
025
20–
Pad1
FRO
010
9272
°57′
07′′
160°
27′1
6′′
4.9
1H
3–6
S4W
019
17br
Pad1
FRO
010
9372
°57′
07′′
160°
27′2
0′′
26.4
1L6
S4W
025
22–
Pad1
FRO
010
9572
°57′
12′′
160°
27′3
9′′
21.6
1H
6S4
W1
1916
v, b
rPa
d1FR
O 0
1096
72°5
7′12′′
160°
27′4
3′′
3.3
1H
6S3
W1
2017
brPa
d1FR
O 0
1097
72°5
7′15′′
160°
26′1
8′′
0.9
1L6
S4W
126
21–
Pad1
FRO
010
9872
°57′
06′′
160°
30′4
2′′
10.1
1L6
S5W
126
22–
Pad1
FRO
010
9972
°57′
06′′
160°
30′4
2′′
3.7
1H
5–6
S2W
217
16br
Sn4
FRO
011
0072
°57′
06′′
160°
30′4
2′′
11.3
1H
4S2
W2
1615
–Sn
4FR
O 0
1102
72°5
7′08′′
160°
27′4
1′′
17.4
1H
4S2
W2
1715
–Sn
4FR
O 0
1103
72°5
7′15′′
160°
24′4
7′′
2.0
1L4
S4W
223
19–
Sn4
FRO
011
0472
°57′
06′′
160°
30′4
0′′
13.9
1H
4/5
S3W
217
16–
Sn4
FRO
011
0572
°57′
01′′
160°
30′4
3′′
2.5
1H
6S3
W2
1816
brSn
4FR
O 0
1106
72°5
7′07′′
160°
30′3
0′′
9.5
1H
5S3
W2
1615
–Sn
4FR
O 0
1107
72°5
7′08′′
160°
30′2
2′′
9.2
1L4
S1w
223
19–
Sn4
FRO
011
0872
°57′
10′′
160°
27′5
5′′
11.7
1H
6S2
w2
1715
vSn
4FR
O 0
1109
72°5
7′10′′
160°
27′4
9′′
4.7
1H
6S3
W1
1715
brSn
4FR
O 0
1110
72°5
7′08′′
160°
27′4
5′′
0.8
1H
6S2
W1
1715
–Sn
4FR
O 0
1111
72°5
7′06′′
160°
30′4
2′′
5.0
1L4
S2W
124
20–
Sn4
FRO
011
1272
°57′
11′′
160°
29′5
5′′
37.0
1L4
S2W
123
19–
Sn4
FRO
011
1372
°57′
15′′
160°
27′4
4′′
31.2
1H
6S2
W2–
320
17–2
2br
Sn4
FRO
011
1472
°57′
07′′
160°
27′3
3′′
0.3
1H
6S1
W2
2018
–Sn
4FR
O 0
1115
72°5
7′10′′
160°
31′1
4′′
3.4
1H
3S1
W1
196–
16–
Sn4
FRO
011
1672
°59′
40′′
160°
24′0
2′′
4.6
1H
3S1
W1–
211
–36
5–25
–Sn
4FR
O 0
1117
72°5
8′14′′
160°
31′2
3′′
11.2
1H
3/4
S1W
219
–24
18–
Sn4
FRO
011
1872
°59′
27′′
160°
24′1
6′′
4.7
1H
6S2
W2
2018
brSn
4FR
O 0
1119
72°5
9′31′′
160°
24′0
0′′
7.2
1H
3S2
–3W
221
13–2
3–
Sn4
FRO
011
2072
°59′
31′′
160°
24′0
1′′
0.5
1H
3S1
–2W
28–
2016
–19
–Sn
4FR
O 0
1121
72°5
7′08′′
160°
27′4
5′′
5.1
1H
5S1
–2W
220
18–
Sn4
FRO
011
2272
°57′
07′′
160°
27′4
9′′
3.5
1H
4–5
S2–3
W2
2018
–Sn
4FR
O 0
1123
72°5
7′06′′
160°
27′4
7′′
0.7
1H
3S1
–2W
220
19–
Sn4
FRO
011
2472
°57′
09′′
160°
27′5
4′′
3.2
1H
3S1
–2W
220
19–
Sn4
FRO
011
2572
°57′
07′′
160°
28′0
2′′
0.3
1H
3S1
W2
2019
–Sn
4
A220 S. S. Russell et al.
Tabl
e 2.
Met
eorit
es fr
om F
ront
ier M
ount
ain
colle
cted
by
the
Italia
n PN
RA
in D
ecem
ber 2
000.
Continued.
Nam
eLa
titud
e(S
)Lo
ngitu
de(E
)M
ass
(g)
Piec
esC
lass
Shoc
kW
GFa (m
ol%
)Fs (m
ol%
)C
omm
ents
a
a See
“A
bbre
viat
ions
for a
naly
sts a
nd sp
ecim
en lo
catio
ns.”
Info
b
b Abb
revi
atio
ns: b
r = b
recc
iate
d; v
= v
eine
d.
FRO
011
2672
°57′
06′′
160°
27′4
7′′
1.3
1H
3S5
W2
2623
–Sn
4FR
O 0
1127
72°5
7′07′′
160°
27′3
4′′
2.9
1H
6S1
W2
1917
–Sn
4FR
O 0
1128
72°5
7′08′′
160°
27′3
3′′
0.8
1L3
S1W
19–
417–
32–
Sn4
FRO
011
2972
°57′
11′′
160°
27′2
4′′
0.3
1H
6S1
–2W
2–3
1918
brSn
4FR
O 0
1130
72°5
9′32′′
160°
23′5
9′′
3.6
1H
3S1
W1–
218
–22
4–20
–Sn
4FR
O 0
1131
72°5
9′32′′
160°
23′5
9′′
2.0
1H
3S1
–3W
217
–32
13–2
1br
Sn4
FRO
011
3272
°59′
33′′
160°
24′0
0′′
4.6
1L6
S5W
2–3
2622
–26
–Sn
4FR
O 0
1134
72°5
9′32′′
160°
24′0
0′′
18.2
1H
5S2
W2
2018
–Sn
4FR
O 0
1135
72°5
9′33′′
160°
24′0
6′′
1.9
1H
5S2
W2
2119
–Sn
4FR
O 0
1137
72°5
9′32′′
160°
23′4
6′′
19.6
1H
5S2
W3
1614
–Sn
4FR
O 0
1138
72°5
9′41′′
160°
23′5
9′′
4.2
1H
3S3
W2
166–
17–
Sn4
FRO
011
3972
°59′
41′′
160°
23′5
9′′
2.2
1H
6S2
W2
1816
brSn
4FR
O 0
1140
72°5
8′39′′
160°
30′3
9′′
38.2
1H
6S2
W2
1716
–Sn
4FR
O 0
1141
72°5
9′32′′
160°
24′0
1′′
13.9
1H
5/6
S2W
216
15–
Sn4
FRO
011
4272
°59′
32′′
160°
24′0
0′′
0.8
1H
4S3
W2
1815
–Sn
4FR
O 0
1143
72°5
9′32′′
160°
24′0
0′′
1.4
1H
3S2
W2
5–47
2–16
brSn
4FR
O 0
1144
72°5
9′35′′
160°
24′0
1′′
8.4
1H
3S3
W2
11–2
73–
15br
Sn4
FRO
011
4572
°59′
35′′
160°
24′0
2′′
12.3
1H
4S2
W2
1716
–Sn
4FR
O 0
1146
72°5
9′34′′
160°
24′2
5′′
1.0
1H
6S1
W2
1716
–Sn
4FR
O 0
1147
72°5
8′25′′
160°
20′1
7′′
0.5
1U
re–
––
–Ss
ee se
para
te e
ntry
Sn4
FRO
011
5072
°57′
35′′
160°
38′5
6′′
11.0
1H
6S1
W1
1715
–Sn
4FR
O 0
1151
72°5
9′16′′
160°
24′0
3′′
3.6
1H
3S3
W1
6–19
3–17
brSn
4FR
O 0
1152
72°5
9′17′′
160°
23′5
7′′
1.5
1H
4S2
W2
1616
–Sn
4FR
O 0
1153
72°5
9′18′′
160°
24′0
5′′
6.7
1H
3S2
W1
17–2
214
–16
–Sn
4FR
O 0
1154
72°5
9′18′′
160°
24′0
5′′
8.9
1H
3–5
S1–4
W1
10–1
58–
17br
Sn4
FRO
011
5572
°59′
18′′
160°
24′0
5′′
0.3
1H
3S3
W2
15–1
914
–18
–Sn
4FR
O 0
1156
72°5
9′22′′
160°
24′0
8′′
0.1
1H
3/4
S3W
216
6–13
–Sn
4FR
O 0
1157
72°5
9′22′′
160°
24′0
8′′
0.7
1H
5S3
W2
1917
–Sn
4FR
O 0
1158
72°5
9′22′′
160°
24′0
8′′
0.6
1H
5/6
S2W
217
15–
Sn4
FRO
011
5972
°59′
22′′
160°
24′0
8′′
0.6
1H
3S2
W2
186–
21br
Sn4
FRO
011
6072
°59′
23′′
160°
24′1
1′′
0.9
1H
3S3
W1
3–19
10–1
6br
Sn4
FRO
011
6172
°59′
33′′
160°
23′4
3′′
0.3
1H
5S2
W2
1716
–Sn
4FR
O 0
1162
72°5
9′36′′
160°
24′0
0′′
2.5
1H
3S2
W2
17–4
03–
21br
Sn4
FRO
011
6372
°59′
36′′
160°
24′0
0′′
0.9
1H
3S2
W2
1–18
2–16
brSn
4FR
O 0
1164
72°5
9′22′′
160°
24′1
0′′
0.8
1H
4S4
W2
1817
–Sn
4FR
O 0
1165
72°5
9′21′′
160°
24′1
5′′
4.5
1H
3/4
S2W
217
12–1
6–
Sn4
FRO
011
6672
°59′
13′′
160°
24′3
0′′
5.5
1H
5S2
W1
1815
–Sn
4FR
O 0
1167
72°5
7′07′′
160°
31′2
0′′
3.9
1H
6S1
W2
1716
–Sn
4FR
O 0
1168
72°5
7′06′′
160°
31′1
7′′
4.0
1H
5S2
W1
1816
–Sn
4FR
O 0
1169
72°5
7′10′′
160°
31′2
0′′
6.2
1H
6S5
W1
1716
–Sn
4
Meteoritical Bulletin No. 87 A221
Tabl
e 3.
Met
eorit
es c
olle
cted
from
the
Thie
l Mou
ntai
ns, A
ntar
ctic
a by
the
Plan
etar
y Sc
ienc
e Fo
unda
tion
(PSF
) in
Janu
ary
2001
.
Nam
eLa
titud
e(S
)Lo
ngitu
de(E
)M
ass
(g)
Piec
esC
lass
Shoc
kW
Ga
a Wea
ther
ing
grad
e sy
stem
follo
ws t
hat f
or A
NSM
ET A
ntar
ctic
met
eorit
es.
Fa (mol
%)
Fs (mol
%)
Info
b
b See
“A
bbre
viat
ions
for a
naly
sts a
nd sp
ecim
en lo
catio
ns.”
TIL
9901
085
°09.
924′
94°4
7.84
1′11
6.8
1H
5S2
A18
.717
.9H
a3TI
L 99
011
85°0
9.51
1′94
°37.
275′
473
1L5
S2A
24.6
20.7
Ha3
TIL
9901
285
°09.
281′
94°3
5.37
8′15
91
L4S3
A23
.620
.3H
a3TI
L 99
013
85°0
9.92
1′94
°43.
472′
248.
51
L4S2
/3A
23.5
20.8
Ha3
TIL
9901
485
°10.
069′
94°4
3.67
3′37
1.3
1L5
S3A
23.7
19.9
Ha3
TIL
9901
585
°09.
914′
94°4
4.02
5′78
.61
H5
S3A
16.8
15.5
Ha3
TIL
9901
685
°09.
906′
94°4
6.62
7′43
1E6
–A
/B–
0.5
Ha3
TIL
9901
785
°09.
807′
94°5
1.41
7′15
27.6
1L4
S3A
24.2
21.1
Ha3
TIL
9901
885
°09.
908′
94°5
0.77
1′43
6.9
1H
4S3
A/B
18.5
16.8
Ha3
TIL
9901
985
°09.
629′
94°4
7.48
1′13
61
L5S4
A26
.022
.0H
a3
Tabl
e 4.
Met
eorit
es fr
om O
man
.
Nam
eD
ate
foun
dLa
titud
e(N
)Lo
ngitu
de(E
)M
ass
(g)
Pcs
Cla
ssSh
ock
WG
Fa (mol
%)
Fs (mol
%)
Wo
(mol
%)
Com
men
tsa
Type
bIn
foc
Al H
uqf (
AH
)A
H 0
0104
/30/
0019
°25.
2′57
°11.
3′41
.51
L4S5
W2
2522
.11.
5i.m
.10
Vr1
Dho
far
(Dho
)D
ho 2
9404
/13/
0118
º36.
8′54
º30.
0′59
8868
H3.
9S1
W2
16.5
–18.
06.
26–2
4.1
0.5–
4.6
–60
9V
r2D
ho 2
9610
/03/
0019
°19.
7′54
°42.
0′14
121
L5S2
W4
24.8
21.7
1.4
–48
8V
r2D
ho 2
9704
/14/
0118
º28.
3′54
º09.
2′69
81
L6S2
W3/
424
.822
.11.
3–
33.2
Vr2
Dho
298
08/0
4/01
18º1
0.6′
54º1
5.8′
677
1H
6S1
W3
1816
.81.
6–
112
Vr2
Dho
299
05/0
4/01
18º3
2.8′
54º1
8.6′
410
1L3
.9S3
W4
11.3
–26.
31.
84–2
3.4
0.3–
2.7
–99
.5V
r2D
ho 3
0404
/13/
0118
º24.
2′54
º09.
0′10
1Lu
nar
––
––
–Se
e se
para
te e
ntry
2V
r3D
ho 3
0506
/28/
0119
º19.
8′54
º47.
0′34
.11
1Lu
nar
––
––
–Se
e se
para
te e
ntry
7V
r3D
ho 3
0606
/29/
0119
º19.
7′54
º47.
1′12
.86
1Lu
nar
––
––
–Se
e se
para
te e
ntry
2.6
Vr3
Dho
307
04/1
4/01
19º1
9.7′
54º4
6.9′
501
Luna
r–
––
––
See
sepa
rate
ent
ry10
Vr3
Dho
308
04/1
3/01
18º2
4.2′
54º0
9.0′
21
Luna
r–
––
––
pr D
ho 0
25, 3
01, 3
040.
64V
r3D
ho 3
0901
/14/
0219
º19.
6′54
º47.
3′81
.31
Luna
r–
––
––
See
sepa
rate
ent
ry16
.5V
r11
Dho
310
01/1
5/02
19º1
9.7′
54º4
7.1′
10.8
1Lu
nar
––
––
–Se
e se
para
te e
ntry
2.5
Vr1
1D
ho 3
1104
/14/
0119
º19.
6′54
º47.
0′4
1Lu
nar
––
––
–Se
e se
para
te e
ntry
1.7
Vr1
0D
ho 3
1310
/04/
0118
º27.
1′54
º01.
9′20
01
H5
S1W
317
.717
.11.
2–
60V
r2D
ho 3
1411
/12/
0119
°19.
1′54
°43.
8′50
14
L6S2
W3–
424
.321
1.4
–34
8V
r2D
ho 3
1511
/12/
0119
°21.
2′54
°49.
5′41
1.25
9H
5S3
W3
17.3
15.5
1.3
–23
6V
r2D
ho 3
1612
/12/
0119
°09.
3′54
°47.
2′32
151
L6S1
W1
24.8
21.2
1.6
–59
1V
r2D
ho 3
1712
/14/
0118
°35.
3′54
°01.
1′28
971
L5S4
W1
24.3
21.6
1.6
–73
6V
r2D
ho 3
1806
/23/
0118
º10.
8′54
º10.
5′52
215
L6S3
W4
25.4
21.4
1.7
–25
6V
r2D
ho 3
1901
/25/
0018
°34.
2′54
°17.
2′41
61
H5
S4W
318
.717
1.3
–12
6V
r2D
ho 3
2004
/04/
0119
º02.
3′54
º36.
7′41
31
L6S4
W3
24.5
22.1
1.5
–64
Vr2
Dho
321
04/0
4/01
18º2
0.9′
54º1
7.2′
594
1H
4S2
W3
18.8
17.7
1.5
–82
Vr2
A222 S. S. Russell et al.
Tabl
e 4.
Met
eorit
es fr
om O
man
. Continued.
Nam
eD
ate
foun
dLa
titud
e(N
)Lo
ngitu
de(E
)M
ass
(g)
Pcs
Cla
ssSh
ock
WG
Fa (mol
%)
Fs (mol
%)
Wo
(mol
%)
Com
men
tsa
Type
bIn
foc
Dho
322
03/0
4/00
18º2
0.2′
54º1
3.3′
658
1H
5S1
W4
1817
.71.
1–
130
Vr2
Dho
323
03/0
4/01
18º1
3.1′
54º0
6.4′
688
1H
5S1
W4
19.6
18.2
1.5
–10
6V
r2D
ho 3
2407
/04/
0118
º54.
2′54
º34.
7′44
81
H6
S3W
318
.517
1.3
prob
ably
pr D
ho 3
4694
Vr2
Dho
325
05/0
4/01
18º2
8.9′
54º0
8.1′
584
1L3
.5S2
W4
1.66
–45.
30.
7–22
.00.
5–5.
5Fe
0 8.
02 w
t%79
.2V
r6D
ho 3
2601
/26/
0019
°02.
0′54
°30.
9′61
81
H5
S4W
318
.817
.71.
1–
242
Vr2
Dho
327
04/0
4/01
18º2
3.3′
54º0
8.0′
421
1L6
S4W
425
.121
.91.
4–
70V
r2D
ho 3
2801
/25/
0018
°58.
8′54
°24.
3′53
67
LL5
S4W
431
.826
.41.
9–
120
Vr2
Dho
329
03/1
1/00
18°5
5.1
54°3
4.7′
475
3H
6S3
W3
18.8
171
–19
4V
r2D
ho 3
3001
/17/
0219
°22.
9′54
°35.
6′15
61
L4S3
W3
23.6
20.8
1.4
–42
Vr1
Dho
331
06/0
3/00
18°0
8.5′
54°0
5.2′
946
1H
5S3
W4
18.3
17.2
1.4
–20
2V
r2D
ho 3
3206
/03/
0018
°16.
1′54
°07.
3′79
41
H5
S3W
219
.417
.81.
7–
166
Vr2
Dho
333
06/0
3/00
18°2
2.5′
54°0
8.3′
410
1L6
S2W
325
.122
.11.
5–
88.6
Vr2
Dho
335
04/2
5/00
18°5
8.4′
54°4
1.3′
555
1L6
S3W
124
.521
.61.
5–
88.4
Vr2
Dho
336
08/0
4/01
18°4
5.3′
54°3
4.8′
468
1L6
S3W
324
.921
.81.
5–
99.6
Vr2
Dho
337
04/1
3/01
18°4
3.6′
54°4
0.5′
580
5L5
S3W
325
.123
1.6
–80
.4V
r2D
ho 3
3804
/14/
0118
°45.
7′54
°42.
2′11
401
H4
S1W
317
.516
.51.
4–
198
Vr2
Dho
339
04/1
4/01
18°3
8.4′
54°3
3.6′
941
L6S2
W1
23.8
21.3
1.6
–28
.1V
r1D
ho 3
4004
/27/
0018
°53.
3′54
°45.
4′23
61
L4S2
W3
25.7
22.4
1.5
–47
.9V
r1D
ho 3
4104
/28/
0019
°19.
7′54
°42.
3′11
61
H5
S2W
318
.817
.71.
3–
31.9
Vr1
Dho
342
04/1
3/01
18º1
9.7′
54º0
2.1′
581
H5
S1W
218
.216
.82
–16
.4V
r1D
ho 3
4311
/04/
0118
º20.
7′54
º11.
8′62
1H
5S2
W3
18.2
16.8
1.3
–21
.4V
r1D
ho 3
4404
/13/
0118
º26.
6′54
º13.
0′76
1H
5S3
W3
17.9
17.6
1.1
br, b
ig m
etal
vei
ns23
.4V
r1D
ho 3
4504
/27/
0019
°07.
0′54
°48.
5′31
1H
4S2
W2
16.8
16.6
1.4
–13
.14
Vr1
Dho
346
07/0
4/01
18º5
4.9′
54º3
6.0′
1345
5H
5S3
W3
18.6
17.4
1.2
prob
ably
pr D
ho 3
2427
9V
r2D
ho 3
4704
/14/
0118
º34.
4′54
º27.
4′62
1L6
S2W
425
.221
.71.
6–
17.4
Vr1
Dho
348
04/1
4/01
18º2
9.0′
54º1
9.5′
419
1L5
S2W
323
.920
.21.
3–
220
Vr1
Dho
349
04/1
4/01
18º2
7.3′
54º1
6.8′
412
1L6
S2W
424
.421
.21.
4–
243
Vr1
Dho
350
04/1
4/01
18º4
9.3′
54º1
3.6′
112
1H
5S1
W3
18.5
16.6
1.3
–47
.3V
r1D
ho 3
8203
/19/
0119
°06.
380′
54°4
9.04
0′15
13
H5/
6S3
W3–
418
.516
––
21M
ün2
Dho
383
03/1
9/01
19°0
6.43
8′54
°49.
051′
139
2H
5S3
W3
18.5
17–
sv, c
alc.
v.
21M
ün2
Dho
385
03/2
0/01
19°0
6.72
2′54
°48.
354′
480
1H
5S3
W3
18.5
16.5
–sv
24M
ün2
Dho
386
03/2
001
19°0
6.19
3′54
°47.
660′
138
1H
5/6
S2W
318
.516
–sv
22M
ün2
Dho
389
03/2
0/01
19°0
6.50
8′54
°47.
967′
160
5H
5S3
W3–
419
.517
.5–
–20
Mün
2D
ho 4
0203
/22/
0119
°18.
010′
54°3
2.14
3′14
01
H6
S2W
419
.517
.5–
–26
Mün
2D
ho 4
0903
/25/
0118
°42.
233′
54°1
2.19
1′16
21
H5
S2W
3–4
1917
.5–
–26
Mün
2D
ho 4
1703
/26/
0118
°45.
835
54°1
3.87
9′16
11
H4/
5S2
W2–
317
.515
.5–
–21
Mün
2D
ho 4
2503
/28/
0118
°37.
623′
54°4
2.56
0′24
81
L5S2
W4
24.5
20.5
–br
26M
ün2
Dho
426
03/2
8/01
18°4
2.49
7′54
°34.
491′
196
1L6
S3W
3–4
24.5
21–
–22
Mün
2D
ho 4
3003
/28/
0118
°54.
206′
54°3
8.34
0′18
21
L5/6
S3W
423
.520
.5–
–22
Mün
2D
ho 4
4003
/31/
0118
°45.
078′
54°2
1.80
5′10
81
H5/
6S2
W4
1816
.5–
–20
Mün
2D
ho 4
5001
/04/
0118
°54.
810′
54°2
9.02
8′10
41
L6S4
W4
2521
.5–
partl
y S5
23M
ün2
Dho
469
01/2
0/01
19°1
4.45
4′′
54°5
1′31
3′′
309
1H
3–4
S2W
315
.3 (m
ax 1
8)14
.7 (m
ax 1
7)1.
6–
23Fr
ei1
Dho
471
01/2
0/01
19°1
5.33′′
54°3
9′66
9′′
158
1L6
S3W
323
.721
.31.
5–
20Fr
ei1
Dho
473
01/2
0/01
19°1
0.55
8′′
54°3
9′41
1′′
145
1L6
S3W
323
.921
.51.
5–
20Fr
ei1
Dho
476
01/2
001
19°0
6.61
4′′
54°4
9′24
7′′
160
1L6
S4W
324
.321
.41.
5–
21Fr
ei1
Dho
480
01/2
0/01
19°0
8.29
7′′
54°4
1′77
6′′
101
1Eu
cS4
W2
–64
.92.
3Pl
ag: A
n 89
-91,
br
20Fr
ei1
Meteoritical Bulletin No. 87 A223
Tabl
e 4.
Met
eorit
es fr
om O
man
. Continued.
Nam
eD
ate
foun
dLa
titud
e(N
)Lo
ngitu
de(E
)M
ass
(g)
Pcs
Cla
ssSh
ock
WG
Fa (mol
%)
Fs (mol
%)
Wo
(mol
%)
Com
men
tsa
Type
bIn
foc
Dho
481
01/2
0/01
19°0
9.95
1′′
54°4
3′12
8′′
120
1H
5S3
W2
16.9
15.9
1.2
–20
Frei
1D
ho 4
8401
/20/
0119
°06.
627′′
54°4
7′32
6′′
383
1H
3/4
S2W
316
.615
.21
–20
Frei
1D
ho 4
8601
/20/
0119
°06.
661′′
54°4
3′73
6′′
855
1H
5S3
W3
18.3
171.
3–
21Fr
ei1
Dho
488
02/2
0/01
19°0
6.37
1′′
54°4
7′94
5′′
652
1H
6S3
W4
18.9
17.4
1.4
–22
Frei
1D
ho 4
9003
/17/
0118
°43.
00′
54°2
7.00′
34.0
51
Luna
r–
––
––
See
sepa
rate
ent
ry7
Be2
Dho
491
04/1
3/01
18º3
5.2′
54º2
3.8′
310
3H
(5?)
S6W
318
.616
.7–
abun
dant
shoc
k m
.v.
95.8
Vr4
Dho
492
04/0
5/01
18º4
2.7′
54º3
9.2′
281
1H
W3
18.5
17–
who
le im
pact
mel
t ro
ck81
Vr4
Dho
493
06/2
5/01
19º0
8.8′
54º3
4.8′
321
LL4
S1W
129
.325
1.8
–12
Vr1
Dho
494
06/2
9/01
19º0
9.0′
54º3
5.0′
311
H5
S2W
318
.717
.51.
8–
14V
r1D
ho 4
9506
/25/
0119
º09.
5′54
º34.
5′31
842
H4
S1W
3–
––
pr D
hofa
r 224
3184
Vr1
Dho
496
03/0
4/00
18°0
9.3′
54°0
6.7′
354
3L4
S4W
324
.723
.21.
4–
65.8
Vr1
Dho
497
04/2
6/00
18°5
8.0′
54°3
8.5′
710
1L4
S2W
324
.324
––
252
Vr1
Dho
498
04/2
7/00
18°4
3.4′
54°5
1.9′
476
8H
5S4
W3
19.7
18.4
––
116.
2V
r1D
ho 4
9901
/11/
0119
º01.
7′54
º32.
9′87
1L6
S2W
324
.921
.4–
–36
.5V
r1D
ho 5
0001
/11/
0018
°23.
2′54
°12.
2′11
61
Ach
ond
Ung
––
––
–Se
e se
para
te e
ntry
23.5
Vr1
3
Dho
501
01/1
6/00
18°2
1.0′
54°1
1.7′
104
1H
4S2
W3
18.6
16.9
1.5
–44
.5V
r2D
ho 5
0201
/25/
0018
°23.
3′54
°17.
5′24
01
H5
S3W
419
181.
3–
98V
r2D
ho 5
0301
/25/
0018
°34.
9′54
°24.
3′32
01
H3.
9S3
W3
19.8
19.4
1.2
PMD
Ol 8
.516
2V
r2D
ho 5
0401
/26/
0018
°44.
1′54
°22.
1′33
11
H4
S4W
318
.818
.61.
5–
60V
r2D
ho 5
0510
/17/
0018
°17.
9′54
°11.
6′37
51
L5S3
W4
24.7
22.7
1.7
–18
8V
r2D
ho 5
0601
/18/
0018
°18.
5′54
°10.
4′34
01
H4
S4W
418
.917
.11.
5–
176
Vr2
Dho
507
01/2
2/00
18°1
9.7′
54°1
1.6′
288
1H
5S4
W3
19.5
18.7
1.4
i.m. b
r pro
b pr
Dho
01
076
.2V
r2
Dho
508
01/2
2/00
18°5
4.7′
54°2
8.5′
270
1L6
S4W
225
.522
.91.
5–
78V
r2D
ho 5
0901
/24/
0018
°08.
4′54
°04.
2′23
81
L6S4
W2
24.5
22.3
1.4
–64
.8V
r2D
ho 5
1001
/25/
0018
°54.
8′54
°21.
7′18
61
H4
S4W
318
.317
.21.
5–
52.6
Vr2
Dho
511
01/2
5/00
18°5
7.4′
54°2
3.1′
521
H4
S4W
317
.817
.21.
4–
25.8
Vr2
Dho
512
01/2
6/00
18°4
8.6′
54°1
5.7′
263.
56
L5S3
W2
24.9
221.
7–
62V
r2D
ho 5
1301
/19/
0018
°20.
1′54
°12.
0′43
41
H5
S4W
318
.617
.11.
7–
98V
r2D
ho 5
1401
/25/
0018
°48.
0′54
°14.
9′16
01
L5S3
W2
25.3
22.1
1.5
–29
.5V
r2D
ho 5
1501
/25/
0019
°00.
4′54
°23.
6′31
520
H5
S4W
419
.617
.41.
3–
95.7
Vr2
Dho
516
03/0
5/00
18°5
2.5′
54°2
8.0′
145
1LL
6S4
W2
26.2
22.9
1.4
–16
.5V
r2D
ho 5
1703
/05/
0018
°55.
5′54
°27.
5′26
01
L6S3
W4
24.5
22.8
1.5
–51
.4V
r2D
ho 5
1803
/11/
0018
°42.
4′54
°22.
8′24
71
H6
S3W
317
16.1
1.2
–16
4V
r2D
ho 5
1903
/11/
0018
°53.
8′54
°32.
3′98
1H
6S3
W3
18.3
17.8
1.4
–23
.6V
r2D
ho 5
2003
/13/
0018
°51.
5′54
°42.
8′48
1H
5S2
W3
18.3
17.1
1.1
–14
.4V
r2D
ho 5
2103
/14/
0019
°10.
4′54
°52.
2′38
62
L4S3
W3
22.5
200.
8–
195.
1V
r2D
ho 5
2203
/07/
0018
°14.
4′54
°10.
1′18
61
H4
S3W
319
.117
.41.
1–
70.8
Vr2
Dho
523
03/1
0/00
19°2
3.8′
54°4
3.7′
741
H4
S3W
318
.217
.11.
3–
13.1
Vr2
Dho
524
03/1
1/00
19°0
5.9′
54°3
0.0′
204
1L5
S2W
224
.719
.71.
4–
68.2
Vr2
Dho
525
03/0
6/00
18°1
4.3′
54°0
8.2′
501
L5S4
W3
25.1
22.1
1.5
–10
Vr2
Dho
526
03/1
1/00
19°2
0.3′
54°4
0.6′
346
1L6
S2W
325
.222
.51.
5–
26V
r2D
ho 5
2704
/04/
0118
º16.
6′54
º08.
1′17
21
H4
S2W
419
.417
.41.
5–
48.5
Vr7
Dho
528
04/0
4/01
18º2
2.0′
54º0
9.1′
374
1L5
S2W
320
.718
.11.
4–
128
Vr7
A224 S. S. Russell et al.
Tabl
e 4.
Met
eorit
es fr
om O
man
. Continued.
Nam
eD
ate
foun
dLa
titud
e(N
)Lo
ngitu
de(E
)M
ass
(g)
Pcs
Cla
ssSh
ock
WG
Fa (mol
%)
Fs (mol
%)
Wo
(mol
%)
Com
men
tsa
Type
bIn
foc
Dho
529
04/0
4/01
18º2
2.4′
54º0
7.8′
368
3H
5S2
W3
21.2
18.6
1.4
–35
9.1
Vr7
Dho
530
04/0
4/01
18º2
2.2′
54º1
4.0′
240
1L4
S2W
324
.821
.51
–56
Vr7
Dho
531
04/0
5/01
18º2
6.0′
54º0
6.5′
258
1L6
S2W
421
.218
.31.
4–
59.8
Vr7
Dho
532
04/0
8/01
18º2
5.2′
54º1
4.8′
861
H5
S3W
418
.716
.41.
3–
22V
r7D
ho 5
3303
/12/
0018
°10.
7′54
°10.
9′30
82
L6S3
W4
24.8
21.9
–Pr
obab
ly p
r Dho
005
173
Vr2
Dho
534
01/1
1/01
19º1
1.8′
54º4
2.2′
173
1H
5S2
W3
17.7
171.
3–
41.6
Vr1
Dho
535
01/1
1/00
19°2
0.0′
54°4
7.7′
204
Man
yC
hond
U
ng–
––
––
See
sepa
rate
ent
ry49
.5V
r12
Dho
536
01/1
4/01
18º1
9.0′
54º0
8.9′
51
H5
S2W
318
.617
1.5
–4.
2V
r1D
ho 5
3701
/16/
0118
º53.
9′54
º42.
3′14
1H
5S1
W2
18.4
17.5
1.7
–6
Vr1
Dho
538
01/1
8/02
19°2
0.3′
54°3
6.3′
230
1L5
S2W
324
.320
.51.
5–
59.7
Vr4
Dho
539
06/2
3/01
18º1
1.3′
54º1
0.0′
102
1H
5S3
W3
18.7
16.4
0.8
Ca-
Px: F
s5–6
, W
o38–
4548
Vr4
Dho
540
04/0
4/01
18º3
3.6′
54º0
6.3′
104
4E4
S3W
30.
20.
6–
–28
Vr4
Dho
541
2000
18°2
0.06′
54°1
0.84′
1233
.31
H4
S2W
316
.914
.9–
–22
.1B
e2D
ho 5
4220
0018
°48.
50′
54°2
8.33′
43.3
1H
4/5
S2W
316
.915
.3–
–8.
7B
e2D
ho 5
5111
/07/
0118
°43.
037′
54°2
1.54
1′18
11
H5/
6S3
W4
1816
.5–
–20
Mün
2D
ho 5
8007
/13/
0118
°42.
903′
54°1
1.80
9′81
25
LL6
S2W
330
.524
.5–
br20
Mün
2D
ho 5
9907
/15/
0118
°41.
452′
54°4
2.28
8′46
51
L6S4
W4
24.5
21.5
––
20.5
Mün
2D
ho 6
0107
/15/
0118
°41.
283′
54°4
0.72
4′22
61
H6
S3W
320
18–
sv20
Mün
2D
ho 6
1401
/13/
0119
°15.
465′
54°4
6.91
5′19
72
L6S3
W3
2521
––
17M
ün2
Dho
622
01/1
5/01
19º1
3.67
2′54
º51.
221′
601
H4-
anS2
W3–
418
.516
.8–
See
sepa
rate
ent
ry12
Mün
2D
ho 6
3801
/19/
0119
°12.
166′
54°3
9.33
7′10
31
L6S6
W4
25.5
21.5
–sv
, rin
gw.,
calc
. v.
15M
ün2
Dho
691
03/0
2/01
19°2
4.40
3′54
°45.
493′
428
1L5
S3W
2–3
23.5
21.5
–sv
18.5
Mün
2D
ho 6
9501
/16/
0219
°16.
9′54
°49.
8′70
21
H3.
9S1
W2
15.9
15.7
1.4
br w
ith i.
m.
104
Vr2
Dho
696
01/1
7/02
19°1
4.2′
54°4
5.5′
233
1L6
S3W
425
.322
.81.
4–
55.4
Vr2
Dho
697
01/1
7/02
19°2
3.0′
54°3
5.7′
409
1L6
S2W
325
.422
.41.
6–
175
Vr2
Dho
699
11/1
0/02
19°0
6.2′
54°4
9.7′
444
3H
4S2
W1
18.5
16.8
1.4
br w
ith i.
m. c
last
s11
0.3
Vr2
Dho
700
11/1
5/02
19°1
8.5′
54°3
3.1′
2770
12D
io–
––
––
See
sepa
rate
ent
ry35
0V
r9D
ho 7
0101
/15/
0219
°08.
9′54
°48.
2′22
02
L5S3
W4
24.9
21.6
0.9
–10
1.3
Vr2
Dho
702
01/1
5/02
19°0
9.9′
54°4
6.6′
2878
1H
4S2
W3/
418
.716
.81.
6–
606
Vr2
Dho
703
04/0
6/01
19º1
0.4′
54º5
2.5′
205
1L5
S3W
422
.321
.20.
8–
43.1
Vr2
Dho
704
04/0
8/01
18º5
3.5′
54º3
5.2′
280
1L4
S2W
324
.922
.31.
5–
57.5
Vr2
Dho
705
04/1
0/01
18º4
9.0′
54º1
5.7′
283
1L6
S1W
124
.721
.51.
4–
39.7
Vr2
Dho
706
04/1
0/01
19º0
3.2′
54º3
2.0′
255
1H
5S3
W2
18.5
171.
2–
69.2
Vr2
Dho
707
04/0
4/01
18º2
5.5′
54º0
9.6′
205
1L5
S3W
124
.821
.91.
5–
48V
r2D
ho 7
0904
/11/
0118
º23.
1′54
º08.
1′33
62
LL6
S3W
426
.123
.81.
5–
83.9
Vr2
Dho
710
04/1
3/01
18º2
7.6′
54º0
0.4′
182
1L6
S2W
425
.322
.41.
5–
37V
r2D
ho 7
1104
/13/
0118
º29.
9′54
º02.
6′37
01
L5S2
W4
24.4
22.1
1.6
–94
Vr2
Dho
712
04/0
5/01
18º4
1.9′
54º3
6.8′
577
3L6
S2W
225
.121
.91.
4–
179.
2V
r2D
ho 7
1304
/14/
0118
º42.
9′54
º21.
5′36
23
H6
S3W
318
.216
.51.
3–
121.
8V
r2D
ho 7
1404
/25/
0018
°15.
1′54
°25.
5′20
71
H5
S2W
317
.716
.31.
5–
42.8
Vr2
Dho
715
04/2
7/00
18°5
4.0′
54°2
4.0′
252
1LL
4S3
W3
26.7
221.
4–
42V
r2D
ho 7
1606
/25/
0119
º10.
0′54
º35.
0′36
11
LL5
S2W
328
.824
.71.
5–
200
Vr1
Dho
717
06/2
8/01
19º1
9.6′
54º4
7.1′
61
L6S6
W3
23.9
19.8
1.7
sv, r
w4.
3V
r4D
ho 7
1801
/14/
0219
°18.
8′54
°51.
1′38
1L5
S6W
324
.518
.91.
4–
24.9
Vr4
Meteoritical Bulletin No. 87 A225
Tabl
e 4.
Met
eorit
es fr
om O
man
. Continued.
Nam
eD
ate
foun
dLa
titud
e(N
)Lo
ngitu
de(E
)M
ass
(g)
Pcs
Cla
ssSh
ock
WG
Fa (mol
%)
Fs (mol
%)
Wo
(mol
%)
Com
men
tsa
Type
bIn
foc
Dho
719
01/1
6/02
19°1
5.3′
54°4
8.0′
121
L4S4
W3
23.1
19.2
––
5V
r4D
ho 7
2004
/27/
0018
°56.
7′54
°53.
7′39
21
H4
S3W
417
15.6
1.2
–10
2.7
Vr2
Dho
721
04/1
0/01
18º4
7.5′
54º0
9.2′
1360
51
H4
S2W
318
.817
.91.
4–
250
Vr2
Dho
722
01/1
5/01
18º4
1.2′
54º3
2.0′
230
4H
3.9
S2W
416
.315
.61.
2PM
D O
l 5.6
40.3
Vr1
Dho
723
01/1
5/01
18º4
1.0′
54º1
3.1′
166
1H
5S2
W3
18.6
17.5
1.2
–47
.7V
r1D
ho 7
2406
/25/
0119
º08.
8′54
º35.
2′48
1LL
5S1
W2
29.1
24.7
1.4
–21
.7V
r1D
ho 7
2506
/25/
0119
º09.
0′54
º34.
6′14
1H
4S2
W3
19.1
17.1
1.2
–4.
9V
r1D
ho 7
2606
/25/
0119
º20.
5′54
º44.
0′26
22
L6S2
W4
2520
.81.
7–
79.3
Vr1
Dho
727
06/2
5/01
19º2
0.6′
54º4
4.0′
329
1H
5S2
W2
19.4
16.6
1.4
–11
3.7
Vr1
Dho
730
11/0
9/02
19°1
9.5′
54°4
7.5′
108
1Lu
nar
––
––
–Se
e se
para
te e
ntry
22V
r3D
ho 7
3111
/11/
0219
°20.
0′54
°47.
7′36
1Lu
nar
––
––
–Se
e se
para
te e
ntry
7.5
Vr3
Dho
732
11/1
5/02
19°2
4.3′
54°3
4.7′
171
Ach
ond
Ung
––
––
–Se
e se
para
te e
ntry
3.5
Vr1
1
Dho
733
11/1
2/02
18°3
5.3′
54°1
3.8′
981
Luna
r–
––
––
See
sepa
rate
ent
ry20
Vr1
1D
ho 7
3511
/09/
0219
°4.1′
54°4
6.8′
304
+ 77
2C
M2
––
––
–Se
e se
para
te e
ntry
58.8
Vr1
2D
ho 7
4510
/200
018
°53.
182′
54°3
9.27
1′36
001
H4
S1W
318
.116
.41.
1–
20Fr
ei1
Dho
746
10/2
000
18°1
6.53
7′54
°19.
309′
969
1H
6S2
W3
19.4
17.3
1.3
–21
Frei
1D
ho 7
4710
/200
018
°47.
739′
54°4
4.37
2′15
55M
any
L3S2
W4
19.4
(max
23)
13.5
(4.0
–22.
6)1.
2–
27Fr
ei1
Dho
748
10/2
000
18°4
6.29
1′54
°42.
983′
1030
Man
yH
6S2
W3
18.7
17.4
1.4
–27
Frei
1D
ho 7
4910
/200
018
°52.
638′
54°4
6.82
1′17
30M
any
LL6
S3W
330
.225
1.9
–22
Frei
1D
ho 7
5010
/200
018
°50.
270′
54°4
0.27
0′74
22
L6S2
W4
24.6
22.3
4–
20Fr
ei1
Dho
751
10/2
000
18°5
3.52
8′54
°42.
771′
1155
Man
yH
6S3
W3
19.8
15.9
1–
23Fr
ei1
Dho
752
10/2
000
18°4
3.64
6′54
°46.
023′
444
1L6
S4W
423
.921
.21.
7–
20Fr
ei1
Dho
753
10/2
000
18°1
5.95
1′54
°19.
264′
550
1H
3/4
S2W
418
16.1
0.6
–20
Frei
1D
ho 7
5410
/200
018
°51.
220′
54°3
8.82
3′53
81
H4
S2W
417
.616
.60.
9–
21Fr
ei1
Dho
755
10/2
000
18°1
9°20
8′54
°14.
147′
547
1L6
S4W
324
.321
.61.
6–
21Fr
ei1
Dho
756
10/2
000
18°2
5.26
7′54
°35.
312′
362
1H
5S2
/3W
318
.817
.51.
5–
20Fr
ei1
Dho
757
10/2
000
18°5
1.23
0′54
°38.
820′
471
1H
5S2
W4
18.3
17.2
0.9
–21
Frei
1D
ho 7
5810
/200
018
°57.
870′
54°4
5.43
3′25
32
L6S3
W3
24.3
21.5
1.6
–20
Frei
1D
ho 7
5910
/200
018
°43.
876′
54°4
9.20
2′44
13
H4/
5S2
W3
17.3
16.3
1.4
–20
Frei
1D
ho 7
6010
/200
018
°56.
673′
54°4
0.44
2′16
31
L5S4
W2
24.2
21.2
1.5
–21
Frei
1D
ho 7
6110
/200
019
°03.
635′
54°3
1.26
8′10
73
H6
S3W
318
.116
.91.
3–
20Fr
ei1
Dho
762
10/2
000
18°4
5.08
0′54
°43.
145′
235
1H
6S2
W4
18.4
171.
5–
20Fr
ei1
Dho
763
10/2
000
18°5
1.89
5′54
°38.
983′
190
1L5
S2W
222
.820
.41.
4–
20Fr
ei1
Dho
764
10/2
000
18°4
9.83
7′54
°45.
987′
195
5H
5S3
W4
17.9
16.5
1.3
–22
Frei
1D
ho 7
6510
/200
018
°56.
617′
54°4
0.24
0′13
51
L5S4
W3
2421
.21.
5–
20Fr
ei1
Dho
766
10/2
000
18°1
6.65
6′54
°19.
415′
152
2H
6S4
W3
16.9
16.2
1.1
–20
Frei
1D
ho 7
6710
/200
018
°49.
938′
54°4
5.95
0′31
78
H6
S3W
317
.916
.61.
3–
20Fr
ei1
Dho
768
10/2
000
18°4
9.15
7′54
°36.
856′
195
1H
5/6
S2W
318
16.8
1.5
–20
Frei
1D
ho 7
6910
/200
018
°57.
759′
54°4
5.06
5′25
03
L6S4
W3
24.7
21.6
1.7
–20
Frei
1D
ho 7
7010
/200
018
°14.
700′
54°2
4.54
7′37
62
H5/
6S2
W4
18.6
17.2
1.3
–21
Frei
1D
ho 7
7110
/200
018
°51.
007′
54°3
7.39
6′11
41
H5
S2W
317
.416
.21.
4–
20Fr
ei1
Dho
772
10/2
000
19°0
5.13
0′54
°45.
746′
9187
2L6
S5W
324
.221
.31.
5–
21Fr
ei1
Dho
773
10/2
000
18°5
0.83
8′54
°32.
123′
295
1H
5S2
W3
18.6
17.1
1.5
–20
Frei
1D
ho 7
7410
/200
018
°41.
535′
54°3
5.47
1′11
52
L6S4
W3
23.6
20.8
1.6
–21
Frei
1D
ho 7
7510
/200
018
°54.
200′
54°4
2.27
1′21
22
H5
S4W
317
.416
.31
–20
Frei
1
A226 S. S. Russell et al.
Tabl
e 4.
Met
eorit
es fr
om O
man
. Continued.
Nam
eD
ate
foun
dLa
titud
e(N
)Lo
ngitu
de(E
)M
ass
(g)
Pcs
Cla
ssSh
ock
WG
Fa (mol
%)
Fs (mol
%)
Wo
(mol
%)
Com
men
tsa
Type
bIn
foc
Dho
776
10/2
000
18°5
1.72
5′54
°40.
762′
121
1L5
S3W
225
.722
.71.
4–
21Fr
ei1
Dho
777
10/2
000
18°5
0.47
3′54
°45.
384′
102
2LL
6S4
W3
30.5
26.3
2.2
–20
Frei
1D
ho 7
7810
/200
018
°43.
525′
54°4
3.82
9′15
61
Dio
S4W
127
.822
.71.
9Pl
ag: A
n69–
79, s
v20
Frei
1D
ho 7
7910
/200
018
°56.
482′
54°4
1.72
7′12
62
L5S4
W4
23.9
21.1
1.5
–21
Frei
1D
ho 7
8009
/27/
0019
°43.
282′
54°4
0.73
8′18
561
H5/
6S2
W4
18.5
17–
heav
y ca
lc. v
.25
Mün
2D
ho 7
8102
/10/
0018
°34.
281′
54°4
2.88
7′12
0019
H5
S3W
3/4
18.5
16–
calc
. v.
36M
ün2
Dho
782
01/1
0/00
18°2
4.72
7′54
°37.
736′
708
2L6
S4W
3/4
2420
––
37M
ün2
Dho
783
01/1
0/00
18°3
7.22
8′54
°42.
927′
426
1H
6S3
W4
18.5
16.5
–sv
24M
ün2
Dho
784
04/1
0/00
18°5
7.28
3′54
°48.
281′
590
1H
5S2
W4
2018
––
32M
ün2
Dho
785
01/2
6/01
19°4
.941′
54°2
7.13
7′98
.449
1H
4/5
S3W
318
.917
.41.
3–
–B
ern1
Dho
786
01/2
6/01
19°4
.016′
54°3
1.15
9′36
.334
1H
4/5
S2/3
W3
19.3
17.5
1.2
––
Ber
n1D
ho 7
8701
/27/
0119
°1.7
53′
54°3
2.68
4′38
2.49
718
H4
S1/2
W4
17.8
16.4
1.1
––
Ber
n1D
ho 7
8801
/27/
0119
°1.7
69′
54°3
2.66
2′27
4.38
1H
4S4
W3
18.5
16.2
1–
–B
ern1
Dho
789
01/2
7/01
19°2
.275′
54°3
2.22
2′43
0.53
96
L6S5
W4
25.1
21.1
1.5
––
Ber
n1D
ho 7
9001
/27/
0119
°3.9
79′
54°3
1.31
8′20
.445
1H
6S3
/4W
420
.116
.21.
3pr
Dho
032
, 036
, 130
, 13
2, 1
37, 1
39, 1
41,
142
–B
ern1
Dho
791
01/2
7/01
19°4
.166′
54°3
1.28
1′14
6.51
91
H6
S3W
319
.98.
90.
7pr
Dho
030
, 036
, 130
, 13
2, 1
37, 1
39, 1
41,
142
–B
ern1
Dho
792
01/2
7/01
19°4
.106′
54°3
2.10
1′51
9.01
61
H5
S3W
319
.116
.71.
3–
–B
ern1
Dho
793
01/2
7/01
19°2
.510′
54°3
3.38
8′15
1.13
21
H6
S3W
419
.117
.11.
3pr
Dho
030
, 032
, 130
, 13
2, 1
37, 1
39, 1
41,
142
–B
ern1
Dho
794
01/2
8/01
19°3
.097′
54°2
7.80
3′43
1.81
11
H6
S1W
418
.215
.91.
2–
–B
ern1
Dho
795
01/2
8/01
19°2
.922′
54°3
1.74
6′32
.182
1L6
S4W
325
.721
1.6
––
Ber
n1D
ho 7
9601
/28/
0119
°3.5
44′
54°3
2.21
6′24
6.37
71
H4
S3W
417
.516
.21
––
Ber
n1D
ho 7
9701
/28/
0119
°3.6
24′
54°3
2.20
3′13
2.18
91
H6
S3W
2/3
19.4
17.1
1–
–B
ern1
Dho
798
01/2
8/01
19°3
.630′
54°3
2.20
6′18
.425
1H
6S3
W4
20.1
17.2
1.4
pr D
ho 0
30, 3
2, 3
6,
130,
137
, 139
, 141
, 14
2
–B
ern1
Dho
799
01/2
8/01
19°4
.224′
54°3
2.30
3′56
.11
1H
4S2
W3
18.5
17.4
1.4
––
Ber
n1D
ho 8
0001
/28/
0119
°3.7
51′
54°3
3.02
9′55
.884
1L4
S2W
425
.520
.91.
6–
–B
ern1
Dho
801
01/2
8/01
19°3
.341′
54°3
3.06
5′11
9.14
92
H6
S2W
418
.816
.61.
1pr
Dho
30,
032
, 036
, 13
0, 1
32, 1
39, 1
41,
142
–B
ern1
Dho
802
01/2
8/01
19°3
.140′
54°3
2.51
7′19
9.43
31
H6
S3W
219
.818
.21.
4pr
Dho
30,
032
, 036
, 13
0, 1
32, 1
37, 1
41,
142
–B
ern1
Dho
803
01/2
8/01
19°3
.516′
54°3
2.10
2′22
.427
1H
6S3
W4
20.3
17.2
1.5
pr D
ho 3
0, 0
32, 0
36,
130,
132
, 137
, 139
, 14
2
–B
ern1
Dho
804
01/2
8/01
19°3
.693′
54°3
2.07
7′44
.404
2H
6S3
W4
19.5
16.5
1.3
pr D
ho 3
0, 0
32, 0
36,
130,
132
, 137
, 139
, 14
1
–B
ern1
Dho
805
01/2
9/01
18°5
5.15
5′54
°16.
015′
237.
941
1L6
S3W
3/4
25.3
21.4
1.6
––
Ber
n1D
ho 8
0601
/29/
0118
°33.
917′
54°4
.842′
117.
237
1L5
S3W
423
.719
.81.
5–
–B
ern1
Dho
807
01/2
9/01
18°3
0.25
7′54
°5.1
54′
1260
1H
5S1
W2
19.8
17.9
1.3
––
Ber
n1D
ho 8
0801
/30/
0118
°10.
799′
54°1
2.22
0′2.
496
1L6
S5W
424
.220
.31.
5–
–B
ern1
Meteoritical Bulletin No. 87 A227
Tabl
e 4.
Met
eorit
es fr
om O
man
. Continued.
Nam
eD
ate
foun
dLa
titud
e(N
)Lo
ngitu
de(E
)M
ass
(g)
Pcs
Cla
ssSh
ock
WG
Fa (mol
%)
Fs (mol
%)
Wo
(mol
%)
Com
men
tsa
Type
bIn
foc
Dho
809
01/3
1/01
18°3
3.87
0′54
°5.7
76′
25.4
241
L4S2
W3
24.2
20.1
1.6
––
Ber
n1D
ho 8
1001
/31/
0118
°33.
657′
54°5
.990′
82.5
731
H4
S2W
419
.716
.11.
2–
–B
ern1
Dho
811
01/3
1/01
18°3
3.48
6′54
°6.2
34′
19.3
241
H5
S2W
218
.916
1.3
––
Ber
n1D
ho 8
1201
/31/
0118
°33.
744′
54°6
.537′
24.8
671
L5S4
W4
24.4
21.1
1.7
––
Ber
n1D
ho 8
1301
/31/
0118
°32.
982′
54°7
.214′
75.8
691
L5S4
W3
23.5
20.2
1.7
––
Ber
n1D
ho 8
1402
/11/
0118
°57.
732′
54°3
5.40
7′99
.805
1H
5S2
W2
17.2
14.8
1.3
––
Ber
n1D
ho 8
1502
/11/
0118
°57.
732′
54°3
5.40
7′89
.451
1H
5S1
W2
17.8
16.9
1.1
––
Ber
n1D
ho 8
1602
/12/
0118
°58.
754′
54°3
7.69
1′23
.858
1H
5S2
W2
20.4
20.1
1.3
––
Ber
n1D
ho 8
1702
/12/
0119
°1.1
89′
54°3
0.83
9′16
4.75
38
H4
S3W
419
.317
.31.
1–
–B
ern1
Dho
818
02/1
2/01
19°1
.525′
54°3
0.38
0′82
.427
1H
6S1
W3
1916
.41.
7–
–B
ern1
Dho
819
02/1
2/01
19°2
.417′
54°2
9.63
2′72
.135
1 H
4S2
W3
19.2
16.3
1.3
––
Ber
n1D
ho 8
2002
/12/
0119
°2.7
52′
54°2
9.67
1′49
.304
1H
4S4
W3
19.4
171.
2–
–B
ern1
Dho
821
02/1
2/01
19°2
.736′
54°2
9.64
0′13
3.21
65
H4
S4W
418
.816
.51.
3–
–B
ern1
Dho
822
02/1
2/01
19°2
.935′
54°2
9.56
0′39
.296
11L5
S3W
425
21.5
1.6
––
Ber
n1D
ho 8
2302
/12/
0119
°3.0
15′
54°2
9.54
5′23
.329
1H
4S4
W3
19.7
17.2
1–
–B
ern1
Dho
824
02/1
2/01
19°3
.608′
54°3
1.90
9′12
.052
1H
6S3
W4
19.3
16.8
1.3
––
Ber
n1D
ho 8
2502
/12/
0119
°3.6
16′
54°3
2.60
9′50
.441
1H
6S3
W3
20.2
16.3
1.4
––
Ber
n1D
ho 8
2602
/12/
0119
°3.6
27′
54°3
2.62
0′63
.975
1H
6S2
/3W
318
.916
.41.
2–
–B
ern1
Dho
827
02/1
2/01
19°3
.526′
54°3
2.84
3′13
4.98
71
H6
S2W
319
.112
.91.
3–
–B
ern1
Dho
828
02/1
2/01
19°3
.587′
54°3
3.76
1′22
5.86
11
H5
S2W
318
.116
.41.
3–
–B
ern1
Dho
829
02/1
2/01
19°3
.602′
54°3
4.72
8′19
.677
1H
6S3
W4
2018
.81.
4–
–B
ern1
Dho
830
02/1
3/01
19°2
.696′
54°2
8.58
2′15
.676
1H
5S3
W4
18.4
17.3
1.1
––
Ber
n1D
ho 8
3102
/13/
0119
°2.8
78′
54°2
9.34
7′22
.291
1H
4S3
W4
21.7
17.3
1–
–B
ern1
Dho
832
02/1
3/01
19°3
.024′
54°2
9.43
6′7.
839
1H
4/5
S3W
419
.116
.11.
3–
–B
ern1
Dho
833
02/1
3/01
19°3
.201′
54°2
9.59
4′4.
583
1H
4/5
S3W
418
.916
.80.
8–
–B
ern1
Dho
834
02/1
3/01
19°3
.737′
54°2
9.84
1′4.
036
1H
4S4
W4
18.4
16.1
1.2
––
Ber
n1D
ho 8
3502
/15/
0118
°38.
689′
54°0
.236′
160.
091
1H
5S1
/2W
417
.815
.51.
5–
–B
ern1
Dho
836
08/1
5/00
18°2
0.92′
54°1
2.84′
995
1U
reS1
W1
21 (c
ore)
10
(rim
)–
–Se
e se
para
te e
ntry
20.2
NSM
T
Dho
837
2000
18°1
8.35′
54°0
8.98′
900.
11
Ure
S1-2
W1
78–
–Se
e se
para
te e
ntry
20.8
NSM
T
Jidd
at a
l Har
asis
(JaH
)Ja
H 0
2204
/30/
0019
°25.
8′56
°59.
0′65
41
L5S4
W4
23.3
20.6
2.7
–87
.7V
r2Ja
H 0
2304
/29/
0019
°25.
8′56
°18.
9′73
.71
H4
S4W
219
.217
.71.
2–
17.6
Vr1
JaH
024
04/3
0/00
19°2
6.2′
56°4
9.6′
832
1L5
S3W
324
.122
.5–
–12
9V
r1Ja
H 0
2504
/30/
0019
°25.
9′56
°53.
9′38
81
H5
S3W
218
.516
.91.
4–
77.1
Vr2
JaH
052
01/1
3/02
19°1
3.9′
55°1
1.0′
220
1H
6S1
W3
18.9
17.7
1.3
–61
.5V
r2Ja
H 0
5810
/200
019
°48.
371′
56°4
1.22
4′41
80M
any
L6S4
W3
2521
.51.
5–
23Fr
ei1
JaH
059
10/2
000
19°5
6.30
4′56
°47.
341′
884
1H
6S3
W3
18.6
17.3
1.3
–21
Frei
1Ja
H 0
6010
/200
019
°45.
762′
56°4
1.28
2′84
01
L3S2
W4
19.3
(max
22)
16.4
(2.7
–40.
1)1.
1–
20Fr
ei1
JaH
061
10/2
000
19°4
6.53
7′56
°38.
429′
141
1Eu
cS2
W1
–61
.12.
5Pl
ag: A
n 89
–91
20Fr
ei1
JaH
062
10/2
000
19°4
5.35
1′56
°40.
021′
903
1L6
S2W
324
.621
.81.
6–
21Fr
ei1
JaH
063
10/2
000
19°4
5.68
4′56
°38.
675′
444
1H
5S2
W3
18.4
17.2
1.5
–20
Frei
1Ja
H 0
6409
/24/
0019
°38.
174′
55°3
8.63
6′11
408
L6S3
W3
24.5
20.5
––
45M
ün2
JaH
065
04/1
0/00
19°1
5.12
4′56
°21.
820′
1253
1L6
S2W
424
.520
.5–
–46
Mün
2
A228 S. S. Russell et al.
Tabl
e 4.
Met
eorit
es fr
om O
man
. Continued.
Nam
eD
ate
foun
dLa
titud
e(N
)Lo
ngitu
de(E
)M
ass
(g)
Pcs
Cla
ssSh
ock
WG
Fa (mol
%)
Fs (mol
%)
Wo
(mol
%)
Com
men
tsa
Type
bIn
foc
JaH
066
09/2
4/00
19°0
4.82
7′55
°19.
243′
810
1L6
S3W
224
20.5
––
25M
ün2
JaH
067
09/2
5/00
19°1
6.24
9′56
°41.
828′
557
6L6
S4W
425
22–
sv, r
w, p
artly
S6
21M
ün2
JaH
068
09/2
7/00
19°3
9.22
6′55
°48.
275′
686
1H
6S2
W3
1816
.5–
sv, b
r24
Mün
2Ja
H 0
6901
/25/
0119
°20.
751′
56°9
.940′
250.
948
10H
5S1
/2W
419
.817
.72
––
Ber
n1Ja
H 0
7001
/25/
0119
°20.
802′
56°8
.947′
79.8
412
H5
S3W
3/4
18.9
17.5
1.5
––
Ber
n1Ja
H 0
7101
/25/
0119
°19.
996′
56°1
0.49
4′41
5.13
41
H6
S1W
318
.417
.21.
4–
–B
ern1
JaH
072
01/2
5/01
19°2
0.70
5′56
°19.
988′
254.
507
1H
5S2
W3
17.9
16.6
1.2
––
Ber
n1Ja
H 0
7301
/17/
0219
°42′
55°4
4′55
0000
2768
L6S4
W2-
425
.322
.41.
2–
–B
ern1
Jidd
at A
rkad
(JA
)JA
001
03/1
0/00
18°4
3.72
7′56
°23.
239′
672
1L6
S4W
425
21.5
–sv
39M
ün2
JA 0
0202
/10/
0018
°25.
524′
56°4
9.35
7′58
11
H3–
5S2
W2
18.7
± 2
.216
.6 ±
1.5
–br
34M
ün2
Sayh
al U
haym
ir (S
aU)
SaU
085
11/0
1/02
21°0
4.1′
57°1
6.2′
112
3C
V3
––
––
–Se
e se
para
te e
ntry
25V
r14
SaU
086
03/1
6/00
20°4
2.6′
57°0
1.3′
710
1L5
S4W
325
.122
.11.
5–
117.
2V
r2Sa
U 0
8704
/24/
0020
°19.
2′57
°13.
9′17
361
H5
S1W
218
.317
.21.
5–
210
Vr2
SaU
088
01/0
4/00
20°3
1.8′
56°3
9.9′
49.2
1L6
S2W
224
.221
.51.
6–
15.2
Vr1
SaU
089
01/1
7/01
20º5
2.9′
57º1
2.0′
2618
1L/ LL
3.6/
3.
7
S2W
225
18.6
(6.3
–23.
4)0.
3–4.
5Se
e se
para
te e
ntry
315
Vr6
SaU
102
02/0
4/00
20°5
6.1′
57°0
0.7′
119.
51
L5S4
W2
23.1
21.3
1.4
–39
.7V
r1Sa
U 1
0304
/15/
0120
º59.
0′57
º19.
6′50
1L6
S2W
224
.322
1.9
–24
.5V
r1Sa
U 1
0404
/01/
0121
º01.
1′57
º18.
8′13
61
H5
S4W
318
.816
.9–
shoc
k m
.v.
36V
r4Sa
U 1
0501
/04/
0121
º03.
5′57
º17.
5′34
1H
5W
318
.316
–sh
ock-
mel
ted
impa
ct
br9.
4V
r4
SaU
106
03/1
7/00
20°3
2.5′
56°4
1.3′
190
1L4
S3W
324
.421
.71.
4–
32.8
Vr2
SaU
107
04/0
1/01
20º5
5.6′
57º1
5.3′
258
1LL
6S4
W4
2824
.61.
6–
65.5
Vr7
SaU
108
03/3
1/01
21º0
4.0′
57º1
9.0′
161
H6
S4W
317
.715
.51.
2–
13.3
Vr4
SaU
109
01/1
2/02
21°0
5.1′
57°1
6.8′
661
H5
S3W
317
.515
.31.
1–
46.8
Vr4
SaU
110
01/1
2/02
20°5
9.4′
57°1
8.4′
660
1H
6S2
W3
17.8
16.2
1.5
–11
7V
r2Sa
U 1
1101
/12/
0220
°59.
1′57
°17.
8′90
1H
6S4
W3/
417
.916
.91.
4–
59.5
Vr2
SaU
112
01/1
9/02
21°0
2.6′
57°1
7.8′
233
1H
5S4
W3/
417
.415
.71
–56
.9V
r2Sa
U 1
1303
/31/
0121
º03.
6′57
º15.
9′32
61
H5
S2W
417
.416
.31.
4–
93.3
Vr2
SaU
114
04/0
2/01
21º0
2.8′
57º1
5.3′
191
4L5
S4W
425
21.7
1.5
–54
Vr2
SaU
115
04/0
2/00
20°2
7.6′
56°4
0.5′
224
1H
6S3
W3
17.7
16.6
1–
58V
r2Sa
U 1
1604
/30/
0020
°32.
5′56
°40.
8′31
41
L6S3
W1
2521
.11.
5–
69.4
Vr2
SaU
120
11/1
7/02
21°0
0.2′
57°1
9.3′
751
Mar
tian
––
––
–Se
e se
para
te e
ntry
15.8
Vr2
SaU
132
12/2
8/01
21°0
4′05
.9′′
57°1
8′56
.3′′
12.3
41
H5
–W
318
.216
.11.
8i.m
.2.
6B
art4
SaU
133
12/2
8/01
20°5
9′55
.2′′
57°1
7′40
.8′′
853
1L5
S3-4
W1
24.9
20.8
1.8
i.m.
20.5
Bar
t5Sa
U 1
3412
/28/
0121
°02′
01.1′′
57°1
9′14
.3′′
190.
582
H5/
6S3
W4
1815
.81
–25
.3B
art5
SaU
135
12/2
9/01
21°0
3′53
.3′′
57°1
6′24
.8′′
7.76
1L5
–W
325
.421
.11.
5i.m
.1.
5B
art4
SaU
136
12/2
9/01
21°0
3′58
.9′′
57°1
6′03
.3′′
129
1H
5–
W4
17.9
15.8
1.2
–18
.7B
art6
SaU
137
12/2
9/01
21°0
4′16
.6′′
57°0
6′06
.3′′
8.07
1L6
–W
324
.720
.81.
5i.m
.1.
5B
art4
SaU
138
12/3
0/01
21°1
1′01
.4′′
57°1
2′36
.3′′
57.3
71
H5
S4W
218
.816
.61.
9i.m
. br
11.4
Bar
t5Sa
U 1
3912
/30/
0121
°11′
13.1′′
57°1
2′31
.2′′
101.
181
H4/
5S4
W4
18.8
16.1
1.6
–29
.1B
art5
SaU
140
12/3
0/01
21°1
2′27
.7′′
57°1
2′40
.9′′
2517
1L4
/5S6
W1
24.7
21.4
1.5
i.m.,
rw–
Bar
t7Sa
U 1
4101
/01/
0221
°03′
46.4′′
57°1
8′56
.2′′
9.87
1H
5S2
W3
18.9
16.4
1.1
–1.
9B
art5
Meteoritical Bulletin No. 87 A229
Tabl
e 4.
Met
eorit
es fr
om O
man
. Continued.
Nam
eD
ate
foun
dLa
titud
e(N
)Lo
ngitu
de(E
)M
ass
(g)
Pcs
Cla
ssSh
ock
WG
Fa (mol
%)
Fs (mol
%)
Wo
(mol
%)
Com
men
tsa
a Abb
revi
atio
ns: b
r = b
recc
iate
d; c
alc
= ca
lcite
; i.m
. = im
pact
mel
t; m
ask
= m
aske
lyni
te; m
v =
mel
t vei
ns; p
r = p
aire
d; rw
= ri
ngw
oodi
te; s
v =
shoc
k ve
ined
; v =
vei
ns.
Type
b
b Whe
re n
o ty
pe sp
ecim
en w
eigh
t is g
iven
, the
ent
ire m
ass i
s at t
he in
stitu
te w
here
the
clas
sific
atio
n w
as m
ade.
Info
c
c See
“A
bbre
viat
ions
for a
naly
sts a
nd sp
ecim
ent l
ocat
ions
.”
SaU
142
01/0
1/02
21°0
2′33
.5′′
57°1
7′51
.6′′
137.
361
L4S4
W2
2520
.41.
7m
etal
/sul
fide
mel
t24
.7B
art5
SaU
143
01/0
1/02
21°0
3′25
.3′′
57°1
7′59
.0′′
142.
432
L4S2
W4
2522
1.9
–19
.6B
art5
SaU
144
01/0
3/02
21°0
0′26
.7′′
57°1
5′59
.7′′
135.
22
L5S2
–3W
424
.720
.81.
8i.m
.20
.6B
art5
SaU
145
01/0
4/02
21°0
2′54
.0′′
57°1
8′33
.0′′
70.2
91
H5
S4W
318
.916
.32.
2i.m
.13
Bar
t5Sa
U 1
4601
/04/
0221
°03′
05.7′′
57°1
8′41
.2′′
33.2
52
H4
S6W
218
.516
.31.
2i.m
. br
7B
art5
SaU
148
01/0
4/02
21°0
2′20
.7′′
57°1
8′36
.6′′
131.
51
L4S4
W2
24.5
20.5
1.2
i.m.
22.6
Bar
t5Sa
U 1
4901
/04/
0221
°02′
18.9′′
57°1
7′37
.8′′
19.5
51
H4
S3–4
W2
18.8
191.
3i.m
.4.
4B
art5
SaU
150
08/1
0/02
20°5
9'31
.3′′
57°1
9′11
.7′′
107.
71
Mar
tian
S5–
––
–Se
e se
para
te e
ntry
17.7
Bar
t5Sa
U 1
5101
/05/
0221
°02′
14.0′′
57°1
7′24
.7′′
87.9
1L4
/5S
6W
125
.421
.81.
4m
.v.,
rw, m
ask
18B
art5
SaU
152
01/0
5/02
21°0
2′12
.9′′
57°1
7′23
.6′′
963
1L4
S 4
W1
24.9
21.5
1.6
i.m.
20.7
Bar
t5Sa
U 1
5301
/04/
0221
°02′
16.8′′
57°1
7′34
.2′′
103.
281
L4/5
S 3
W1
25.5
21.1
1.5
–19
Bar
t5Sa
U 1
5920
0121
°01.
03′
57°1
9.22′
163
1H
4S1
W3
16.7
15.4
––
21.9
Be5
SaU
160
10/2
000
20°0
9.14
4′56
°42.
174′
185
2L6
S4W
423
.420
.91.
5–
20Fr
ei1
SaU
161
10/2
000
20°0
9.47
3′56
°43.
229′
263
1H
6S2
W3
18.6
17.3
1.3
–20
Frei
1Sa
U 1
6210
/200
020
°07.
379′
56°4
3.42
4′38
7L6
S4W
322
.719
.95
–8
Frei
1Sa
U 1
6301
/22/
0121
°2.2
22′
57°1
9.61
1′18
77.3
0136
H5
S1/2
W3/
418
.816
1.4
––
Ber
n1Sa
U 1
6401
/22/
0120
°59.
012′
57°1
2.06
1′33
1.46
93
H6
S1/2
W4
10.2
17.4
1.8
––
Ber
n1Sa
U 1
6501
/23/
0121
°1.2
11′
57°1
2.68
8′45
7.15
23
L5S3
W4
27.1
20.7
1.3
––
Ber
n1Sa
U 1
6601
/23/
0121
°1.2
38′
57°1
2.78
6′38
5.20
12
H5
S1/2
W4
19.3
16.8
1.1
––
Ber
n1Sa
U 1
6702
/10/
0121
°10.
073′
56°3
2.48
2′68
.035
2L6
S4W
3/4
24.2
21.1
1.2
––
Ber
n1Sa
U 1
6802
/10/
0121
°6.3
10′
56°5
9.77
8′24
.726
3H
4S4
W4
19.1
18.5
1.1
––
Ber
n1Sa
U 1
6901
/16/
0220
°34.
391′
57°1
9.4′
206.
454
1Lu
nar
––
––
–Se
e se
para
te e
ntry
–B
ern1
Shal
imSh
alim
002
09/2
3/00
18°4
2.43
7′55
°43.
281′
1248
1L6
S4W
424
.521
–br
, sv
36M
ün2
Shal
im 0
0303
/21/
0118
°10.
940′
55°3
0.11
0′10
350
50H
5S1
/2W
318
.616
.71.
4–
–B
ern1
Shi∏s
rSh
i∏sr 0
0608
/03/
0018
°24.
9′53
°59.
3′43
21
L3.9
S3W
311
.3–2
7.9
8.2–
27.7
1.1
–17
2V
r2Sh
i∏sr 0
0801
/18/
0218
°32.
5′53
°59.
9′24
41
L5S3
W3
25.4
21.7
1.5
Prob
. pr S
hi 0
1030
.9V
r2Sh
i∏sr 0
0910
/04/
0118
º33.
8′53
º55.
6′18
51
H4
S2W
317
.816
.51.
2–
55V
r2Sh
i∏sr 0
1012
/200
118
°33.
0′53
°58.
2′17
604
16L4
/6S3
W3
24.1
21.4
1.5
Prob
. pr S
hi 0
0835
01V
r2Sh
i∏sr 0
1110
/04/
0118
º33.
5′53
º54.
8′47
819
L4S2
W3
2522
2.1
–13
3V
r2Sh
i∏sr 0
1502
/02/
0118
°32.
945′
53°5
5.37
4′34
09.2
9720
L5S2
W4
24.4
21.1
1.5
––
Ber
n1Sh
i∏sr 0
1602
/02/
0118
°26.
304′
53°5
8.13
5′84
.481
1H
5S3
W4
18.8
16.7
1.4
––
Ber
n1Sh
i∏sr 0
1702
/14/
0118
°25.
393′
53°3
6.54
3′12
.83
1H
4S5
W4
1916
.71.
2–
–B
ern1
Shi∏s
r 018
02/1
5/01
18°3
2.24
0′53
°55.
987′
116.
538
1L6
S1W
425
.521
.21.
4–
–B
ern1
Shi∏s
r 019
02/1
5/01
18°3
2.85
0′53
°53.
610′
1332
.725
4H
4S3
W3
19.7
171.
3–
–B
ern1
Shi∏s
r 020
02/1
5/01
18°3
3.55
6′53
°53.
493′
2200
.715
4H
4–6
S1W
319
.117
.41.
3br
; pr S
hi 0
21–
Ber
n1Sh
i∏sr 0
2102
/15/
0118
°36.
272′
53°5
3.25
4′13
5.22
61
H4–
6S1
W4
18.7
16.1
1.1
br, p
r Shi
020
–B
ern1
Um
m a
s Sam
im (U
aS)
UaS
002
02/0
4/01
21º1
9.4′
56º2
5.3′
1048
1H
5S1
W2
18.3
171.
4–
52V
r2U
aS 0
0304
/01/
0121
º19.
2′56
º25.
0′99
11
H3.
7S1
W4
16.1
13.9
71.
1–
156
Vr5
A230 S. S. Russell et al.
Tabl
e 5.
Sah
aran
met
eorit
es fr
om A
lger
ia.a
a See
“A
bbre
viat
ions
for a
naly
sts a
nd sp
ecim
en lo
catio
ns.”
Nam
eD
ate
foun
dLa
titud
e(N
)Lo
ngitu
de
(E)
Mas
s(g
)Pc
s.C
lass
Shoc
kW
GFa (m
ol%
)Fs (m
ol%
)W
o(m
ol%
)C
omm
ents
Type
Info
Acf
erA
cfer
056
–27
°28′
3°53′
129
1L4
S3W
1/2
23.5
20–
–20
Mün
3A
cfer
321
2001
27°3
2.73′
4°03
.67′
157
1H
5S5
W3
17.1
15.1
1.4
–22
Ha1
Acf
er 3
2220
0127
°33.
55′
4°05
.58′
251
L5S4
W1
20.5
181.
3–
7H
a1A
cfer
323
2001
27°3
0.18′
3°52
.77′
117
1LL
5S3
W3
29.5
25.3
1.8
–30
Ha1
Acf
er 3
2712
/21/
0127
°44′
4°26′
745.
223
H5
–W
220
.318
.2–
–36
.3Pa
8A
cfer
328
12/2
2/01
27°4
4′4°
13′
180.
071
CV
3–
––
––
see
sepa
rate
ent
ry20
.0Pa
9A
cfer
329
12/2
3/01
27°3
5′4°
06′
3000
06
L4/5
–W
024
.121
.5–
–12
3.7
Pa8
Acf
er 3
3012
/23/
0127
°39′
4°02′
490
1L6
–W
125
.622
.1–
–25
.4Pa
8A
cfer
331
12/2
3/01
27°3
5′4°
01′
750
10C
M2
––
––
–se
e se
para
te e
ntry
22.6
Pa9
Acf
er 3
3212
/23/
0127
°44′
4°08′
115.
021
CO
3–
––
––
see
sepa
rate
ent
ry20
.1Pa
9A
cfer
333
12/2
6/01
27°3
4′4°
04′
489
5C
O3
––
––
–se
e se
para
te e
ntry
25.4
Pa9
Acf
er 3
3405
/09/
0227
°39′
4°23′
211.
251
L6S5
/6W
024
.521
.7–
–27
.0Pa
8A
cfer
335
05/0
9/02
27°4
4′4°
26′
261
1H
4S5
W1
18.3
16.8
––
27.2
Pa8
Acf
er 3
3605
/10/
0227
°37′
4°04′
1940
04
L3.8
S3W
36–
232–
20–
–21
.0Pa
9A
cfer
337
05/1
0/02
27°4
1′4°
16′
360
1L3
.8W
10.
5–23
3–29
––
21.0
Pa9
Acf
er 3
3805
/11/
0227
°43′
4°16′
377.
64
H6
S5/6
W1
19.9
17.9
––
41.8
Pa8
Acf
er 3
3905
/11/
0227
°33′
4°12′
400
1H
5W
019
.016
.9–
–25
.7Pa
9A
cfer
340
05/1
2/02
27°3
5′4°
18′
173.
151
L5W
024
.120
.5–
–25
.9Pa
9A
cfer
347
12/2
001
27°4
1′4°
18′
1165
1L3
S2W
41–
261–
29–
–11
65Sn
3A
cfer
348
12/2
4/01
27°5
8.76′
4°16
.69′
8750
1L5
S2W
224
.620
.7–
–87
50Pr
3A
cfer
349
12/2
5/01
27°5
0.44′
4°18
.86′
298
1H
6S3
W3
18.0
16.1
––
298
Pr3
Acf
er 3
5012
/26/
0127
°40.
32′
4°31
.58′
128
1H
4S3
W2
19.9
16.8
––
128
Pr3
Acf
er 3
5112
/200
127
°42′
4°08′
211
1L6
S3W
425
.120
.6–
–21
1Pr
3A
cfer
352
12/2
001
27°4
6′4°
01′
873
1L5
S4W
424
.620
.6–
–87
3Pr
3
Agu
emou
rA
guem
our 0
1712
/25/
0127
°24′
4°21′
1000
1L6
–W
125
.622
.1–
–48
.7Pa
8
Tane
zrou
ft (T
nz)
Tnz
003
11/1
1/89
~25°
27′
~0° 3
3′14
21
H4
S1W
316
.816
.5–
–19
.83
Vr1
Tnz
054
05/1
5/02
25°2
6′0°
24′
576.
43
H5
–W
218
.316
.0–
–98
.0Pa
8Tn
z 05
505
/16/
0225
°24′
0°25′
251.
41
H4
–W
318
.216
.5–
–21
.0Pa
8Tn
z 05
605
/16/
0225
°29′
0°09′
151.
12
H6
–W
320
.318
.3–
–20
.7Pa
8Tn
z 05
715
/16/
0225
°16′
0°09′
5400
1C
4–
––
––
–11
0.0
Pa9
Tnz
059
15/1
8/02
25°1
3′0°
13′
156.
42
L5S5
/6W
125
.821
.4–
–26
.1Pa
8Tn
z 06
015
/19/
0225
°17′
0°12′
3650
1LL
4S5
W3
28.6
24.4
––
49.0
Pa8
Tnz
061
15/1
9/02
25°1
8′0°
12′
651
L3.9
–W
00–
324–
36–
–13
.1Pa
9
Meteoritical Bulletin No. 87 A231
Tabl
e 6.
Sah
aran
met
eorit
es fr
om E
gypt
.a
a See
“A
bbre
viat
ions
for a
naly
sts a
nd sp
ecim
en lo
catio
ns.”
Nam
eD
ate
foun
dLa
titud
e(N
)Lo
ngitu
de(E
)M
ass
(g)
Pcs.
Cla
ssSh
ock
WG
Fa (mol
%)
Fs (mol
%)
Type
Info
Gre
at S
and
Sea
(GSS
)G
SS 0
1912
/199
925
°32′
12′′
25°3
9′28′′
1200
0>8
0LL
6S2
W3/
427
.422
.515
3.6
Pa6
Tabl
e 7.
Sah
aran
met
eorit
es fr
om L
ibya
.a
Nam
eD
ate
foun
dLa
titud
e(N
)Lo
ngitu
de(E
)M
ass
(g)
Pcs.
Cla
ssSh
ock
WG
Fa (mol
%)
Fs (mol
%)
Wo
(mol
%)
Com
men
tsa
Type
Info
b
Dar
al G
ani (
DaG
)D
aG 6
6411
/00
27°1
4′16
°07′
137
2L4
S2/3
W2
23.5
21–
–20
.6Sn
1D
aG 6
7311
/00
27°1
4′16
°07′
961
L4/5
S3W
324
21–
–19
Sn1
DaG
870
2000
26°5
4.66′
16°2
7.41′
262
1H
3/4
S3W
319
.115
.71.
2–
20H
a1D
aG 8
7119
9827
°00.
76′
16°1
6.67′
166
2L6
S3W
225
.122
.21.
3–
21H
a1D
aG 8
7319
9927
°21.
89′
16°1
0.42
136
1L6
S3W
324
.319
.71.
7–
22H
a1D
aG 8
7420
0027
°02.
51′
16°2
4.30
64.6
1U
reS3
med
ium
19.0
125.
8br
ecci
ated
lit
holo
gy11
Ha1
17.5
16.4
6.1
gran
ular
lith
olog
yD
aG 8
7519
9826
°55.
17′
16°4
0.80′
585
1H
5S3
W3
19.1
16.4
1.4
–20
Ha1
DaG
878
11/0
027
°14′
16°0
758
1L4
S3W
224
21–
–11
.3Sn
1D
aG 8
7911
/00
27°0
8′16
°28′
261
Ure
––
––
–Se
e se
para
te e
ntry
5Sn
1D
aG 8
8011
/00
27°0
5′16
°07
131
1H
6S5
W1
1716
–i.m
. br
20.1
Sn1
DaG
881
11/0
027
°26′
16°1
2′86
1H
ow–
––
––
See
sepa
rate
ntry
17.6
Sn1
DaG
882
11/0
027
°14′
16°0
6′42
1LL
5-6
S3W
230
26–
br8.
3Sn
1D
aG 8
9411
/00
27°1
4′16
°06′
781
L3/4
S3W
226
22–
–14
.9Sn
1D
aG 8
9611
/00
~27°
45′
~16°
53′
22.6
1A
chon
d un
g–
––
––
See
sepa
rate
ent
ry5.
442
Sn1
DaG
915
11/0
027
°21′
16°1
1′74
01
How
––
––
–Se
e se
para
te e
ntry
23.1
Sn1
DaG
916
11/0
027
°15′
16°0
8′18
33
L4/5
S4W
125
21–
–22
.4Sn
1D
aG 9
1711
/00
27°1
5′16
°08′
522
H4/
5S2
W2
2018
––
11.8
Sn1
DaG
918
11/0
027
°12′
16°0
5′20
011
H3–
5S3
W2
2–17
3–15
–br
38.6
Sn1
DaG
919
11/0
027
°13′
16°0
8′10
61
H5
S2W
218
16–
–16
.1Sn
1D
aG 9
2011
/00
27°1
3′16
°09′
106
1H
4S2
W2
1713
––
24.2
Sn1
DaG
921
11/0
027
°08′
16°1
2′12
31
H5
S3W
120
18–
br, v
17.4
Sn1
DaG
922
11/0
026
°57′
16°2
3′25
32
L6S4
W1
2623
–v
20.4
Sn1
DaG
924
11/0
027
°02′
16°2
1′54
1L6
S3W
325
22–
–10
.8Sn
1D
aG 9
2511
/00
27°0
5′16
°15′
931
H4
S2W
317
15–
–21
.5Sn
1D
aG 9
2611
/00
27°1
1′16
°16′
243
1H
6S1
W4
1815
–br
26.4
Sn1
DaG
927
11/0
026
°59′
16°3
5′36
71
H6
S1W
419
17–
–21
Sn1
DaG
928
11/0
026
°54′
16°3
6′96
1H
3/4
S1W
317
–18
10–1
8–
–15
.9Sn
1D
aG 9
2911
/00
26°5
7′16
°27′
119
1H
3S1
W2
17–1
910
–18
––
17.3
Sn1
DaG
930
11/0
027
°02′
16°2
6′56
01
H5
S3W
2/3
1917
––
25Sn
1
A232 S. S. Russell et al.
Tabl
e 7.
Sah
aran
met
eorit
es fr
om L
ibya
. Con
tinue
d.
Nam
eD
ate
foun
dLa
titud
e(N
)Lo
ngitu
de(E
)M
ass
(g)
Pcs
Cla
ssSh
ock
WG
Fa (mol
%)
Fs (mol
%)
Wo
(mol
%)
Com
men
tsTy
peIn
fo
DaG
931
11/0
027
°07′
16°2
8′14
04
L6S3
W3
2319
––
21.6
Sn1
DaG
932
11/0
027
°24′
16°1
4′
232
How
––
––
–Se
e se
para
te e
ntry
3.5
Sn1
DaG
933
11/0
027
°05′
16°0
4′17
01
H4
S3W
218
16–
–21
.4Sn
1D
aG 9
3411
/00
27°0
5′16
°01′
542
H6
S2/3
W5
2019
––
15.8
Sn1
DaG
935
11/0
027
°08′
16°0
1′37
61
H5
S2W
419
17–
–21
.3Sn
1D
aG 9
3611
/00
27°1
3′16
°07′
522
1H
3–5
S2–3
W2
1816
–2–
br, v
20.2
Sn1
DaG
937
11/0
027
°14′
16°0
9′13
61
L4S4
W1
2219
––
19.6
Sn1
DaG
938
11/0
027
°15′
16°1
1′54
1H
6S1
W2
2018
––
11.5
Sn1
DaG
939
11/0
027
°23′
16°0
3′36
71
L6S3
W2
2320
–v
25.7
Sn1
DaG
940
11/0
027
°30′
16°1
2′21
01
L6S3
/4W
2/3
2622
––
16.2
Sn1
DaG
941
11/0
027
°34′
16°1
2′57
1H
6S3
W1
1716
––
10.7
Sn1
DaG
957
1998
26°5
3.73′
16°3
4.99′
369
2L4
S4W
224
20.2
1.6
–20
Ha1
DaG
958
1999
26°5
7.40′
16°2
0.85′
542
Man
yL5
S4W
325
.921
.71.
5–
21H
a1D
aG 9
5919
9926
°57.
95′
16°2
0.88′
164
1H
4S3
W3
18.4
15.9
1.1
–17
Ha1
DaG
960
1999
26°5
2.54′
16°4
0.82′
392
1L6
S3W
325
212.
8–
20H
a1D
aG 9
6519
9826
°56.
49′
16°2
5.27′
216
1LL
5S3
W2
26.7
23.0
1.4
–31
Ha1
DaG
966
1998
26°5
3.78′
16°3
4.77′
204
1L4
S3W
224
.520
.91.
9–
25H
a1D
aG 9
6719
9826
°53.
35′
16°3
3.04′
468
1L5
S4W
225
.622
.82.
5–
25H
a1D
aG 9
6819
9926
°53.
56′
16°3
4.60′
351
1L5
S4W
225
.622
.22.
0–
26H
a1D
aG 9
7519
9927
°19.
63′
16°1
3.00′
27.5
51
Mar
tian
––
––
–Se
e se
para
te e
ntry
8.5
Be2
DaG
976
1999
27°0
3.25′
16°2
3.25′
32.0
31
Ure
pm
––
––
–Se
e se
para
te e
ntry
7.8
Be2
DaG
977
2000
27°0
5.00′
16°2
2.00′
171
Ure
S3m
od15
.1
(8.6
–22.
0)16
––
3.6
Be5
DaG
978
1999
27°1
6.84′
16°2
4.34′
44.4
1C
3S1
W0/
129
.1
(17.
4–31
.8)
12.4
(2
.9–2
1.7)
––
9.5
Be2
DaG
979
12/1
2/00
27°2
7.01′
16°1
1.20′
2483
6L6
S2W
125
.120
.81.
7–
25PC
U1
DaG
980
3/20
0126
°50.
24′
16°3
6.82′
93
3H
4S1
W2
19.1
16.8
1.7
–38
PCU
1D
aG 9
8210
/11/
0027
°12.
69′
16°2
5.92′
177
1H
5S3
W3
19.8
17.4
––
19.6
Ham
1D
aG 9
8303
/23/
0226
°44.
25′
16°5
3.97′
933
1Eu
c pm
––
––
–Se
e se
para
te e
ntry
281
Ham
1D
aG 9
9501
/03/
0127
°10.
35′
16°2
3.17′
56.1
21
Euc
––
––
–Se
e se
para
te e
ntry
11.6
Be2
DaG
996
05/1
4/99
––
12.3
11
Luna
r–
––
––
See
sepa
rate
ent
ry2.
5B
e2D
aG 9
9719
99~2
6°55′
~16°
40′E
500
1H
6S5
W4
2018
–br
182
Sn2
DaG
998
1999
27°1
0.46′
15°5
5.23′
3522
6C
O3
S2W
30.
3–80
1–48
––
33.4
Be2
DaG
999
4/14
/00
27°0
1.55′
16°2
1.95′
2106
Man
yU
re p
m–
––
––
See
sepa
rate
ent
ry20
.8B
e2
Meteoritical Bulletin No. 87 A233
Tabl
e 7.
Sah
aran
met
eorit
es fr
om L
ibya
. Con
tinue
d.
Nam
eD
ate
foun
dLa
titud
e(N
)Lo
ngitu
de(E
)M
ass
(g)
Pcs
Cla
ssSh
ock
WG
Fa (mol
%)
Fs (mol
%)
Wo
(mol
%)
Com
men
tsa
a Abb
revi
atio
ns: b
r = b
recc
iate
d; im
br =
impa
ct m
elt b
recc
ia; m
os =
mos
aici
zed;
sv =
shoc
k ve
ins;
pm
= p
olym
ict;
ung
= un
grou
ped.
Type
Info
b
b See
“A
bbre
viat
ions
for a
naly
sts a
nd sp
ecim
en lo
catio
ns.”
DaG
100
019
9727
°00.
81′
16°2
1.95′
17.9
21
Ure
pm
––
––
–Se
e se
para
te e
ntry
4.2
Be6
DaG
100
119
9927
°22.
61′
16°1
8.14′
132
1H
6S2
W3
18.8
16.5
––
132
Pr2
DaG
100
219
9927
°21.
08′
16°1
5.22′
370
1H
5S2
W3
18.8
16.5
––
370
Pr2
DaG
100
319
9927
°16.
70′
16°1
6.63′
236
2H
5S1
W4
19.3
17.2
––
236
Pr2
DaG
100
419
9927
°15.
51′
16°0
5.54′
287
1H
5S1
W2
19.6
17.2
––
132
Pr2
DaG
100
519
9927
°11.
41′
16°1
8.50′
477
5H
4S3
W3
18.7
16.8
––
477
Pr2
DaG
101
13/
2/99
27°0
2′35′′
16°2
4′42′′
38.0
52
L5–
W1
25.7
20.2
––
7.0
Vr1
6D
aG 1
012
3/3/
9927
°09′
08′′
16°2
8′59′′
14.8
1H
5–
W1
18.9
16.7
––
3.0
Vr1
7D
aG 1
013
3/3/
9927
°09′
08′′
16°3
1′02′′
20.3
22
L4-5
–W
224
.119
.4–
br1.
0V
r16
DaG
101
43/
5/99
27°3
4′17′′
16°1
0′30′′
239
1H
5–
W3
18.6
16.5
––
20V
r16
DaG
101
53/
7/99
27°2
5′35′′
16°1
6′27′′
247
1H
5–
W3
19.5
16.7
––
20V
r17
DaG
101
83/
9/99
27°3
7′54′′
16°0
5′13′′
181.
882
H5
–W
118
.116
.0–
–20
Vr1
6D
aG 1
019
3/9/
9927
°34′
17′′
16°0
5′00′′
104.
11
L5–
W2
24.2
21.3
––
20V
r16
DaG
102
24/
25/0
1~2
7°05′
~16°
15′
33.6
1LL
7–
––
––
See
sepa
rate
ent
ry7
Vr1
8D
aG 1
023
1999
27°1
.55′
16°2
3.27′
149
1U
re p
m–
––
––
See
sepa
rate
ent
ry20
.75
NSM
T
Ham
mad
ah a
l Ham
ra (H
aH)
HaH
291
2000
29°0
4.71′
13°0
7.87′
130
1L5
S3W
325
.83
21.7
41.
62–
25H
a1H
aH 3
1420
0128
°39.
28′
13°2
7.53′
1470
Man
yLL
6S5
W1/
229
.824
.7–
br21
.9B
e2H
aH 3
152/
2001
29°1
6.23′
11°3
2.40′
609
1L6
S2W
324
.920
.7–
–60
9Pr
3H
aH 3
162/
2001
29°2
0.38′
11°3
7.46′
176
1L6
S5W
324
.921
.2–
–17
6Pr
3H
aH 3
1720
0129
°21.
06′
11°3
5.58′
105
2EL
4–
––
––
See
sepa
rate
ent
ry10
5Pr
3H
aH 3
182/
2001
29°2
2.71′
11°3
2.78′
141
L5S2
/3W
324
.821
.9–
–14
Pr3
HaH
319
2/20
0129
°08.
43′
11°5
3.77′
303
1H
5S1
W2
18.9
17.0
––
303
Pr3
HaH
320
2/20
0128
°58.
24′
12°1
2.36′
7823
104
H6
S3W
318
.117
.1–
–78
23Pr
3H
aH 3
212/
2001
29°0
2.17′
11°3
0.39′
100
1H
5S2
W3
18.9
17.0
––
100
Pr3
HaH
322
2/20
0129
°05.
36′
12°2
5.62′
152
2H
6S2
W3
19.6
17.1
––
152
Pr3
HaH
323
2/20
0129
°10.
95′
12°1
5.71′
358
5H
4S3
W2
17.5
15.9
––
358
Pr3
HaH
324
1999
28°5
1.24′
12°3
1.34′
307
1L4
S3W
325
.021
.1–
–30
7Pr
2H
aH 3
2519
9928
°46.
07′
12°4
3.59′
129
3H
5S1
W3
18.9
17.8
––
129
Pr2
HaH
326
1999
28°3
9.14′
12°2
3.13′
978
L4S2
W2
25.0
20.7
––
97Pr
2H
aH 3
2719
99–
–29
1H
5S3
W4
18.4
16.4
––
29Pr
2Ja
lu11
/1/0
027
°57.
5′21
°41.
0′15
0000
Man
yL6
S3W
125
.421
.5–
–86
Pa6
Kuf
ra10
/99
24°2
8.40′
23°0
2.60′
344
1H
5S3
W3
19.3
18.6
1.2
–22
Ha2
Reb
iana
10/9
924
°58.
70′
21°5
3.10′
459
1L/
LL5
S3W
326
.222
.41.
4–
29H
a2
A234 S. S. Russell et al.
Tabl
e 8.
Met
eorit
es fr
om M
oroc
co a
nd s
urro
undi
ng c
ount
ries.
a
Nam
ePo
ssib
le o
rigin
/ ps
eudo
nym
bLa
titud
e(N
)cLo
ngtit
ude
(W)c
Dat
efo
undd
Mas
s(g
)Pc
s.C
lass
Shoc
kW
GFa (m
ol%
)Fs (m
ol%
)C
omm
ents
Mag
Suse
Plac
epu
rcha
sed
Type
Spec
(g)
Info
f
Nor
thw
est A
fric
a (N
WA
)N
WA
167
Azh
akan
,A
lger
ia–
–P
1999
611
H4
S2W
317
.717
.1pr
ob. p
aire
d w
ith
NW
A 1
68–
Tago
unite
25.4
Vr1
5
NW
A 1
68A
zhak
an,
Alg
eria
––
P 19
9958
1H
4S2
W3
18.9
17.2
prob
. pai
red
with
N
WA
167
–Ta
goun
ite23
Vr1
5
NW
A 1
73A
nbdu
r–
–P
2000
68.1
1H
5S3
W2
18.5
18.1
–Ta
goun
ite33
.3V
r15
NW
A 1
74A
nbdu
r–
–P
2000
177.
61
H4
S3W
218
.617
.9–
–Ta
goun
ite72
Vr1
5N
WA
175
Anb
dur
––
P 20
0074
1L5
S3W
425
.321
.3–
––
25V
r1N
WA
426
Saha
ra–
–19
9912
601
L6S3
W1
25.0
± 0
.1–
––
–32
La1
NW
A 4
27A
lger
ia–
–P
2001
4120
1L6
S3W
224
.8 ±
0.2
––
––
139
La2
NW
A 4
28M
oroc
co–
–P
2001
655
1L6
S1W
124
.5 ±
0.8
––
––
29La
2N
WA
429
Mor
occo
––
P 20
0191
11
L6S2
W3
24.8
± 0
.2–
––
–31
La2
NW
A 4
30M
oroc
co–
–P
2001
323
1L6
S4W
424
.4 ±
0.4
––
––
35La
2N
WA
455
–26
°47.
04′
12°5
0.01′
2001
811
H4
S2W
212
.515
.4–
––
16.3
Be1
NW
A 4
56–
26°4
7.04′
12°5
0.01′
2001
359
1H
5/6
S3W
319
.215
.9–
––
25.4
Be1
NW
A 4
57–
31°2
2.09′
04°0
1.01′
2001
175
2H
6S4
W0/
119
.316
.5–
––
20.8
Be1
NW
A 4
58–
26°4
7.04′
12°5
0.01′
2001
387
4L6
S4W
225
21.1
––
–22
.7B
e1N
WA
459
–31
°22.
09′
04°0
1.01′
2001
300
1H
3S2
W3
16.3
15–
––
21.5
Be1
0.3–
27.8
3.3–
20.3
NW
A 4
60–
31°2
2.09′
04°0
1.01′
2001
655
1H
6S2
W3
18.5
16.6
––
–20
.8B
e1N
WA
461
–26
°47.
04′
12°5
0.01′
2001
171
1H
5S2
W3
18.1
16.2
––
–20
.9B
e1N
WA
462
–26
°47.
04′
12°5
0.01′
2001
40.5
1L6
S6W
224
.921
sv, r
w–
–9
Be1
NW
A 4
63–
26°4
7.04′
12°5
0.01′
2001
151
L6S6
W3
24.5
21.1
sv, r
w–
–3.
3B
e1N
WA
464
–31
°22.
09′
04°0
1.01′
2001
159
1H
3S2
W2/
315
.414
.3–
––
21.7
Be1
1.0–
24.4
4.1–
16.7
NW
A 4
65–
26°4
7.04′
12°5
0.01′
2001
413.
51
H5
S1W
319
.116
.9–
––
23.7
Be1
NW
A 4
66–
31°2
2.09′
04°0
1.01′
2001
461
L6S5
W3
24.5
20.8
––
–9.
2B
e1N
WA
779
Bou
dnib
~31°
50′
~3°4
0'19
99~2
001
CV
3–
–2.
2–46
.21–
20Se
e no
te 1
––
10K
1N
WA
821
Ksa
r es S
ouk
31°5
8′4°
25′
P 10
/200
05.
11
H3.
8S2
W1
9.7
± 1.
5–
––
–1.
2La
3N
WA
822
Ksa
r es S
ouk
31°5
8′4°
25′
P 10
/200
064
.51
H6
S2W
320
.2–
––
–17
.7La
3N
WA
823
Ksa
r es S
ouk
31°5
8′4°
25′
P 10
/200
071
.21
L4S1
W2
25.6
± 0
.3–
––
–16
La3
NW
A 8
63–
––
2000
139
1H
5–
–18
.417
.0 ±
1.3
––
–24
CU
1N
WA
900
––
–20
0161
61
L3–6
S2W
125
± 4
.521
± 2
br, s
v–
Erfo
ud31
Mün
3N
WA
904
––
–P
6/20
0126
399
50L5
S3W
124
.9 ±
0.4
––
–Za
gora
21La
4N
WA
924
––
–P
6/20
0135
55
H5
S2W
218
.2 ±
0.5
––
–M
’ham
id23
.1La
4N
WA
925
––
–P
6/20
0189
73
H3.
8S1
W2
18.2
± 0
.1–
––
M’h
amid
20.5
La4
NW
A 9
98M
oroc
co/
Alg
eria
––
09/2
001
456
1M
artia
n–
––
–Se
e se
para
te e
ntry
–Tu
cson
, AZ
40U
WS1
NW
A 1
053
––
–P
2001
108
1L6
S2W
2–3
26.5
22.5
––
Erfo
ud20
Mün
1N
WA
105
8–
––
P 20
0118
01
Prim
. ac
hond
S2W
26.
58
See
note
2–
Erfo
ud22
Mün
1
NW
A 1
062
––
–P
2001
112
1H
4S2
W2–
315
.514
––
Erfo
ud20
.5M
ün1
NW
A 1
067
––
–P
2001
118
1E6
–W
4–
<1no
relic
chon
drul
es–
Erfo
ud20
.5M
ün1
NW
A 1
109
––
–P
11/2
001
1530
3Eu
c pm
––
––
See
sepa
rate
ent
ry–
Erfo
ud21
UW
S2N
WA
117
5–
––
P 01
/200
259
01
L5S3
W2–
325
.521
––
Gue
lmim
23M
ün2
NW
A 1
176
––
–P
01/2
002
150
1L5
S2W
325
.520
.5–
–Za
gora
23M
ün2
NW
A 1
177
––
–P
01/2
002
101
CR
2S2
W1–
21–
3 (P
eak)
1–3
(Pea
k)ca
lc. v
.–
Zago
ra2.
1M
ün2
NW
A 1
185
Mor
occo
––
P 20
0110
51
H5
S4W
1/2
19.1
19.6
sv, m
p5.
35Er
foud
25.9
Pa1
Meteoritical Bulletin No. 87 A235
Tabl
e 8.
Met
eorit
es fr
om M
oroc
co a
nd s
urro
undi
ng c
ount
ries.
a Con
tinue
d.
Nam
ePo
ssib
le o
rigin
/ ps
eudo
nym
bLa
titud
e(N
)cLo
ngtit
ude
(W)c
Dat
efo
undd
Mas
s(g
)Pc
s.C
lass
Shoc
kW
GFa (m
ol%
)Fs (m
ol%
)C
omm
ents
Mag
Suse
Plac
epu
rcha
sed
Type
Spec
(g)
Info
f
NW
A 1
186
Mor
occo
––
P 20
0119
61
H~5
/6S4
W4
––
–5.
01Er
foud
22.2
Pa1
NW
A 1
187
Mor
occo
––
P 20
0119
01
H4/
5S2
W2
20.6
18.2
See
note
3; n
ativ
e C
u5.
22Er
foud
21.6
Pa1
NW
A 1
188
Mor
occo
––
P 20
0182
.61
H~4
/5S2
W3
––
–4.
99Er
foud
21.3
Pa1
NW
A 1
189
Mor
occo
––
P 20
0111
41
L~3.
8–6
S2/3
W1
––
See
note
44.
62Er
foud
26.8
Pa1
NW
A 1
190
Mor
occo
––
P 20
0122
.91
CR
2–
W5
––
–4.
66Er
foud
5.3
Pa1
NW
A 1
195
Safs
af–
–P
02/2
002
315
1M
artia
n–
––
–Se
e se
para
te e
ntry
–Za
gora
10U
WS1
NW
A 1
196
–30
°48.
48′
5°51
.35′
2001
431
L4/5
S5W
0/1
2421
.1–
––
12.4
Be1
NW
A 1
198
Kem
Kem
––
2001
141
Euc
–W
0/1
–42
.2Pl
ag: A
n91.
8–
–3.
4B
e1N
WA
124
3M
oroc
co–
–P
2002
35.9
1L~
5–
W4
––
–4.
55Er
foud
7.6
Pa1
NW
A 1
244
Mor
occo
––
P 20
0225
.61
L~3.
8–6
S2/3
W1
2414
.8–2
1.5
See
note
44.
69Er
foud
7.3
Pa1
NW
A 1
245
Mor
occo
––
P 20
0240
.41
L~3.
8–6
S2/3
W1
––
See
note
44.
75Er
foud
16Pa
1N
WA
124
6M
oroc
co–
–P
2002
44.3
1L~
3.8–
6S2
/3W
1–
–Se
e no
te 4
4.69
Erfo
ud8.
3Pa
1N
WA
124
7M
oroc
co–
–P
2002
27.6
1L3
.8S2
W1
2420
.2–2
4.3
abun
dant
ch
ondr
ules
4.66
Erfo
ud4.
5Pa
1
NW
A 1
248
Mor
occo
––
P 20
0210
21
L~3.
8–6
S2/3
W1
––
See
note
44.
70Er
foud
21.6
Pa1
NW
A 1
249
Mor
occo
––
P 20
0264
.81
L~3.
8–6
S2/3
W1
––
See
note
44.
74Er
foud
14.2
Pa1
NW
A 1
251
Mor
occo
––
P 20
0212
21
H5/
6S2
W2
18.5
17.4
See
note
5;
nativ
e C
u5.
29Er
foud
28.5
Pa1
NW
A 1
252
Mor
occo
––
P 20
0292
1H
5/6
S2W
217
.216
See
note
55.
33Er
foud
19.6
Pa1
NW
A 1
253
Mor
occo
––
P 20
0250
1H
~4/5
S2W
2–
–Se
e no
te 3
5.29
Erfo
ud13
Pa1
NW
A 1
255
Mor
occo
––
P 20
0279
41
L~6
S4W
4–
––
4.76
Erfo
ud54
.4Pa
1N
WA
125
6M
oroc
co–
–P
2002
421
Ure
–W
49.
1–17
.9–
br;
4.52
Erfo
ud7.
7Pa
1C
px: F
s12.
4–14
.7W
o12.
2–7.
9N
WA
125
7M
oroc
co–
–P
2002
172
1H
~4/5
S2W
2–
––
5.25
Erfo
ud41
.8Pa
1N
WA
125
8M
oroc
co–
–P
2002
721
L~5/
6–
W4
––
–4.
43Er
foud
15.5
Pa1
NW
A 1
259
Mor
occo
––
P 20
0212
01
L3.8
–6S2
/3W
124
.520
.3Se
e no
te 4
4.57
Erfo
ud30
.2Pa
1N
WA
126
0M
oroc
co–
–P
2002
2518
27L3
.8–6
S6W
124
.520
.9Se
e no
te 4
4.66
Erfo
ud58
.2Pa
1N
WA
126
1M
oroc
co–
–P
2002
118
1L~
5S3
W2
––
–4.
84Er
foud
23.2
Pa1
NW
A 1
262
Mor
occo
––
P 20
0218
01
L~5
S3W
2–
––
4.76
Erfo
ud23
.2Pa
1N
WA
126
3M
oroc
co–
–P
2002
74.4
1L~
4S1
W2
––
–4.
77Er
foud
20.5
Pa1
NW
A 1
264
Mor
occo
––
P 20
0280
1L4
–6S4
W1
24.9
21.5
sv4.
80Er
foud
15Pa
1N
WA
126
5M
oroc
co–
–P
2002
198
1L~
6S2
W3
––
–4.
53Er
foud
27.5
Pa1
NW
A 1
266
Mor
occo
––
P 20
0295
.21
L3.8
S2/3
W1
16.9
-25.
77.
8–28
.8br
4.66
Erfo
ud19
.9Pa
1N
WA
126
7M
oroc
co–
–P
2002
200
1L~
5S3
W2
––
–4.
84Er
foud
24.7
Pa1
NW
A 1
268
Mor
occo
––
P 20
0223
61
L~5
S3W
2–
––
4.74
Erfo
ud23
.6Pa
1N
WA
126
9M
oroc
co–
–P
2002
62.2
1L5
S3W
126
.221
.9–
4.85
Erfo
ud11
.3Pa
1N
WA
127
0M
oroc
co–
–P
2002
204
1L~
4/5
S4W
1–
––
4.88
Erfo
ud23
.3Pa
1N
WA
127
1M
oroc
co–
–P
2002
94.2
1L~
6S2
W3
––
–4.
59Er
foud
20.9
Pa1
NW
A 1
273
Mor
occo
––
P 20
0222
0.48
1H
~5S3
W3
––
–5.
13Er
foud
24.8
Pa1
NW
A 1
274
Mor
occo
––
P 20
0213
8.4
1H
~5S3
W3
––
–5.
12Er
foud
28.4
Pa1
NW
A 1
275
Mor
occo
––
P 20
0259
7.1
1L~
6S4
W4
––
–4.
77Er
foud
25.8
Pa1
NW
A 1
276
Mor
occo
––
P 20
0226
61
L~6
S1W
4–
––
4.67
Erfo
ud20
Pa1
NW
A 1
296
Mor
occo
––
Sprin
g20
0181
01
Ang
r–
––
–Se
e se
para
te e
ntry
–B
ouar
fa49
UPV
I1
NW
A 1
430
Tata
––
2001
113
kg1
IIIA
B–
––
–Se
e no
te 6
–M
oroc
co15
2La
5N
WA
143
1–
––
2001
213
1Eu
c pm
––
––
See
note
7–
Mor
occo
20La
6N
WA
145
7–
––
P 02
/200
252
7W
in–
––
–Se
e se
para
te e
ntry
–Za
gora
10U
WS2
A236 S. S. Russell et al.
Tabl
e 8.
Met
eorit
es fr
om M
oroc
co a
nd s
urro
undi
ng c
ount
ries.
a Con
tinue
d.
Nam
ePo
ssib
le o
rigin
/ ps
eudo
nym
bLa
titud
e(N
)cLo
ngtit
ude
(W)c
Dat
efo
undd
Mas
s(g
)Pc
s.C
lass
Shoc
kW
GFa (m
ol%
)Fs (m
ol%
)C
omm
ents
Mag
Suse
Plac
epu
rcha
sed
Type
Spec
(g)
Info
f
NW
A 1
459
––
–P
04/2
002
531
Dio
––
––
See
sepa
rate
ent
ry–
Zago
ra10
UW
S2N
WA
146
3–
––
P 11
/27/
0010
013
Win
––
3.2
± 0.
17.
4 ±
0.4
Opx
: Wo1
.2 ±
.2;
Plag
: A
n12.
6Or4
.6
–Er
foud
975
La7
NW
A 1
464
Zago
ra–
–20
0118
001
Ure
S2lo
w9.
316
––
–22
.4B
e21.
1–22
.77.
9–17
.9N
WA
146
6Sa
c–
–20
0156
Man
yEu
c ub
–ve
ry
low
–49
.2un
brec
ciat
ed;
Plag
: An8
7.3;
sv
––
12B
e2
NW
A 1
467
––
–P
06/2
002
111
1H
4S3
W3/
418
16.5
calc
. v.
–Sa
inte
-Mar
ie22
Mün
2N
WA
146
8–
––
P 06
/200
216
71
H5/
6S3
W3/
419
16.5
calc
. v.
–Sa
inte
-Mar
ie21
Mün
2N
WA
146
9–
––
P 06
/200
211
91
H5/
6S4
W1/
219
.517
br, p
artly
S5
–Sa
inte
-Mar
ie20
Mün
2N
WA
147
0–
––
P 06
/200
265
91
L4S2
W2
26.5
21.5
± 1
.5br
, sv
–Sa
inte
-Mar
ie21
Mün
2N
WA
147
1–
––
P 20
0153
.31
R3/
4S3
W3/
440
± 1
.6–
See
note
8–
Mor
occo
11.5
Mün
3N
WA
147
2–
––
P 20
0110
81
R3/
4S3
W3/
440
± 2
–Se
e no
te 8
–M
oroc
co21
Mün
3N
WA
147
3–
––
P 20
0192
81
L6S4
W1/
225
22br
, par
tly S
5–
Mor
occo
25M
ün3
NW
A 1
474
––
–P
2001
54.2
1H
4–6
S2W
219
.515
br, s
v–
Mor
occo
11M
ün3
NW
A 1
475
––
–P
2001
220
1L6
S3W
2/3
25.5
21.5
sv–
Mor
occo
21M
ün3
NW
A 1
476
––
–P
2001
20.6
2R
3S3
W1
41 ±
2.2
(mx)
––
–M
oroc
co4.
5M
ün3
8 ±
11
(cho
nd)
NW
A 1
477
––
–P
2001
351
R3
S3W
3/4
37 ±
7.8
–sv
–M
oroc
co7
Mün
3N
WA
147
8–
––
P 20
0128
1R
3S3
W1/
239
± 4
.6–
sv–
Mor
occo
6M
ün3
NW
A 1
479
––
–P
2001
79.
31
L6S5
W2
2621
sv–
Mor
occo
16M
ün3
NW
A 1
480
––
–P
2001
29.3
1L6
S3W
2/3
25.5
21.5
––
Mor
occo
6M
ün3
NW
A 1
481
––
–P
12/2
001
242
1L6
S3W
1/2
2621
.5–
–H
ambu
rg20
Mün
3N
WA
148
2–
––
P 12
/200
168
.81
L6S3
W1/
225
.521
.5–
–H
ambu
rg14
Mün
3N
WA
148
3–
––
P 12
/200
110
.41
H5
S3W
219
.517
.5–
–H
ambu
rg2.
2M
ün3
NW
A 1
484
––
–P
12/2
001
16.4
1H
5S3
W1
19.5
17.5
––
Ham
burg
3.4
Mün
3N
WA
148
5–
––
P 01
/200
2~3
0 kg
Man
yL5
–6S4
W1
25.5
21sv
, br,
impa
ct m
elt
brec
cia
clas
ts–
Ris
sani
26M
ün3
NW
A 1
486
––
–P
01/2
002
6000
1H
4S2
W3/
417
.516
calc
. v.
–R
issa
ni25
.5M
ün3
NW
A 1
487
––
–P
01/2
002
1142
1L6
S3W
125
.521
.5sv
–R
issa
ni29
Mün
3N
WA
148
8–
––
P 01
/200
232
51
L6S3
W1
2622
.5–
–R
issa
ni22
Mün
3N
WA
148
9–
––
P 01
/200
219
11
Impa
ct
mel
t br.
S2W
122
± 6
.529
.5 ±
4.5
prob
ably
LL-
grou
p:
frag
s ~Fa
30
–R
issa
ni22
Mün
3
NW
A 1
490
––
–P
01/2
002
85.4
1L6
S3W
125
.521
.5sv
–R
issa
ni20
Mün
3N
WA
149
1–
––
P 01
/200
215
51
H4
S2W
2/3
19.5
17.5
––
Ris
sani
26M
ün3
NW
A 1
492
––
–P
01/2
002
72.2
1H
4S2
W1/
217
± 0
.815
.5 ±
1.9
––
Ris
sani
14.5
Mün
3N
WA
149
3–
––
P 01
/200
214
81
L6S4
W1
2623
.5pa
rtly
S5–
Ris
sani
24M
ün3
NW
A 1
494
––
–P
01/2
002
141
1H
5S4
W1/
219
16.5
sv, c
alc.
v.
–R
issa
ni24
Mün
3N
WA
149
5–
––
P 10
/200
165
601
L4–5
S4W
124
.520
.5–
–M
unic
h22
Bar
t1N
WA
149
6–
––
P 10
/200
126
81
H5
S4W
118
.616
.5–
–M
unic
h22
.6B
art1
NW
A 1
497
––
–P
10/2
001
1890
1L5
S4W
124
.621
.4–
–M
unic
h20
.2B
art1
NW
A 1
498
––
–P
10/2
001
357
1H
4S3
W1
19.1
17.3
––
Mun
ich
20.4
Bar
t1N
WA
149
9–
––
P 10
/200
110
021
L5S3
W1
24.2
20.4
––
Mun
ich
20.1
Bar
t1N
WA
150
0–
––
P 20
0033
001
Ure
––
––
See
sepa
rate
ent
ry–
Zago
ra20
Bar
t2N
WA
150
1–
––
P 10
/200
154
21
H5
S3W
118
.916
.5–
–M
unic
h21
.4B
art1
NW
A 1
502
––
–P
10/2
001
1150
1L4
–5S5
W2
24.5
21.1
––
Mun
ich
19.9
Bar
t1N
WA
150
3–
––
P 10
/200
125
51
L4S4
W2
25.6
24.8
––
Mun
ich
19.9
Bar
t1
Meteoritical Bulletin No. 87 A237
Tabl
e 8.
Met
eorit
es fr
om M
oroc
co a
nd s
urro
undi
ng c
ount
ries.
a Con
tinue
d.
Nam
ePo
ssib
le o
rigin
/ ps
eudo
nym
bLa
titud
e(N
)cLo
ngtit
ude
(W)c
Dat
efo
undd
Mas
s(g
)Pc
s.C
lass
Shoc
kW
GFa (m
ol%
)Fs (m
ol%
)C
omm
ents
Mag
Suse
Plac
epu
rcha
sed
Type
Spec
(g)
Info
f
NW
A 1
504
––
–P
10/2
001
748
1L5
S4W
224
.521
––
Mun
ich
22.3
Bar
t1N
WA
150
5–
––
P 10
/200
127
71
L/LL
5S6
W2
2622
.3m
etal
/sul
fide
vein
s, sv
–M
unic
h20
.2B
art1
NW
A 1
507
––
–P
10/2
001
668
1L5
S4W
125
21.2
––
Mun
ich
23.2
Bar
t1N
WA
150
8–
––
P 10
/200
150
21
L5–6
S2W
124
.620
.9–
–M
unic
h23
.1B
art1
NW
A 1
510
––
–P
10/2
001
562
1L5
S5W
224
.820
.8–
–M
unic
h19
.5B
art1
NW
A 1
511
––
–P
10/2
001
198
1L5
S3W
124
.720
.6–
–M
unic
h19
.9B
art1
NW
A 1
512
––
–P
10/2
001
485
1L5
S3W
424
.420
.6–
–M
unic
h30
.3B
art1
NW
A 1
513
––
–P
10/2
001
596
1H
4S3
W1
18.2
16.2
––
Mun
ich
20.5
Bar
t1N
WA
151
4–
––
P 10
/200
154
01
L5S3
W2
24.4
20.6
––
Mun
ich
23.4
Bar
t1N
WA
151
5–
––
P 10
/200
142
31
H4
S2W
220
.714
.9–
–M
unic
h22
.7B
art1
NW
A 1
516
––
–P
10/2
001
530
1L5
––
24.5
20.3
––
Mun
ich
21.2
Bar
t1N
WA
151
7–
––
P 10
/200
127
11
L5–
–24
.520
.9–
–M
unic
h19
.3B
art1
NW
A 1
520
––
–P
10/2
001
406
1L4
/5–
–24
.218
––
Mun
ich
20.4
Bar
t1N
WA
152
2–
––
P 10
/200
130
21
H5
S2W
218
.516
.3–
–M
unic
h20
.4B
art1
NW
A 1
525
––
–P
10/2
001
4889
1L5
S2W
124
.920
.7–
–M
unic
h22
.3B
art1
NW
A 1
535
––
–P
2000
285
1H
5S2
W2
18.6
16.7
––
Zago
ra20
Bar
t3N
WA
153
6–
––
P 20
0027
61
H4
S2W
118
.916
.8–
–Za
gora
20B
art3
NW
A 1
537
––
–P
2000
528
1L5
S4W
125
.121
impa
ct m
elt c
last
–Za
gora
20B
art3
NW
A 1
538
––
–P
2000
280
1LL
4S2
W2
26.9
21.9
––
Zago
ra23
.6B
art3
NW
A 1
539
––
–P
2000
156.
21
L4S3
W2
2520
.8–
–Za
gora
24.2
Bar
t3N
WA
154
0–
––
P 20
0013
01
L5S3
W2
24.7
21.1
––
Zago
ra20
.1B
art3
NW
A 1
541
––
–P
2000
54.7
1L5
S3W
224
.720
.9–
–Za
gora
11B
art3
NW
A 1
542
––
–P
2000
661
L5S2
W2
2421
.4–
–Za
gora
12B
art3
NW
A 1
543
––
–P
2000
58.1
1H
4S1
W1
19.4
17.1
––
Zago
ra12
.3B
art3
NW
A 1
545
––
–P
2000
209
1H
5S1
W2
18.6
16.7
––
Zago
ra21
.8B
art3
NW
A 1
547
Mor
occo
/A
lger
ia–
–P
2002
164.
51
LL4
S2W
329
.724
.2–
––
33.2
MP1
NW
A 1
548
Mor
occo
/A
lger
ia–
–P
2002
331.
61
LL4
S2W
329
.624
.1ca
lc. v
.–
–31
.4M
P1
NW
A 1
549
Mor
occo
/A
lger
ia–
–P
2002
482.
71
LL5–
6S2
W3
31.3
25.6
br–
–31
.1M
P1
NW
A 1
550
SW A
lger
ia–
–P
2002
~8 k
gSe
vera
lLL
5S4
W0/
131
.325
.7sv
––
>20
MP1
NW
A 1
551
NW
of Z
agor
a–
–P
2002
809.
21
LL5
S4W
226
.522
sv–
–32
.3M
P1N
WA
155
8A
oufo
us–
–19
9838
51
CK
5/6
––
29–
Ol:
0.5–
0.6
wt%
N
iO; M
t: ~4
wt%
C
r2O
3
20V
n1–
–
NW
A 1
559
Mor
occo
––
P 20
0028
41
CK
3–
–1–
40–
See
note
9–
Zago
ra
20V
n1N
WA
156
0M
oroc
co–
–P
1999
822
1C
K4/
5–
–37
–m
t; re
frac
tory
in
clus
ion
–Er
foud
20V
n1
NW
A 1
561
Mor
occo
––
P 19
9919
81
H5
–hi
gh19
.117
––
Zag
20V
n1N
WA
156
2M
oroc
co–
–P
2000
380
1LL
6–
high
32.8
26.7
––
Erfo
ud20
Vn1
NW
A 1
563
Ham
ara
––
2000
2950
4C
K5
––
29.8
–Se
e no
te 1
0–
–20
Vn1
NW
A 1
564
––
–19
9850
01
L5S4
W2
23.7
22–
––
21.2
2V
r1N
WA
156
5–
––
1999
200
6H
4S2
W1
17.8
15.2
––
–19
.39
Vr1
NW
A 1
566
––
–P
12/2
001
159
1R
3.8
S2W
441
± 3
24 ±
6–
–Er
foud
23M
ün2
NW
A 1
567
––
–P
1/20
0222
1C
R2
S2W
20–
4 (P
eak)
0–4
(Pea
k)–
–Er
foud
4.5
Mün
2N
WA
156
8–
––
P 1/
2002
371
LL6
S2W
231
26br
, sv
–Er
foud
10M
ün2
NW
A 1
569
––
–P
2001
614
1U
re–
––
–Se
e se
para
te e
ntry
–Er
foud
20.4
NA
U1
NW
A 1
570
Zago
ra–
–20
0128
1Eu
cm
od.
very
lo
w–
56.6
Plag
: An9
3.5,
mon
omic
t br
ecci
ated
––
4.8
Be2
A238 S. S. Russell et al.
Tabl
e 8.
Met
eorit
es fr
om M
oroc
co a
nd s
urro
undi
ng c
ount
ries.
a Con
tinue
d.
Nam
ePo
ssib
le o
rigin
/ ps
eudo
nym
bLa
titud
e(N
)cLo
ngtit
ude
(W)c
Dat
efo
undd
Mas
s(g
)Pc
s.C
lass
Shoc
kW
GFa (m
ol%
)Fs (m
ol%
)C
omm
ents
Mag
Suse
Plac
epu
rcha
sed
Type
Spec
(g)
Info
f
NW
A 1
571
Zago
ra–
–20
0183
21
L5S2
W1/
224
.120
.5–
–22
.5B
e2N
WA
157
2Za
gora
––
2001
382
1L6
S4W
224
.720
.9–
––
20.5
Be2
NW
A 1
573
Mor
occo
––
2002
781
LS5
W1
24.3
20.4
impa
ct m
elt r
ock
––
17.7
Be2
NW
A 1
574
Zago
ra–
–20
0121
0.5
1H
5S4
W1
18.3
16.4
––
–20
.5B
e2N
WA
157
5M
aurit
ania
––
2002
230
1L6
S4W
223
.420
.4–
––
21.2
Be2
NW
A 1
576
Mau
ritan
ia–
–20
0255
01
L6S4
W2
24.1
20.4
sv, m
p–
–21
.7B
e2N
WA
157
7Za
gora
––
2002
112
6L6
S6W
224
20.3
rw, s
v–
–21
.1B
e2N
WA
157
8Er
foud
31°3
6′04
°23′
2001
1549
1L6
S4W
323
.920
––
–23
.6B
e3N
WA
157
9Er
foud
31°3
0′04
°51′
2001
5200
1L5
S4W
224
.220
.4–
––
22.6
Be3
NW
A 1
580
Erfo
ud31
°20′
04°0
0′20
0157
001
L6S4
W2
24.2
20.8
sv–
–25
.2B
e3N
WA
158
1Er
foud
31°2
3′04
°15′
2001
5020
01
L6S4
W2
24.4
20.2
––
–21
.1B
e3N
WA
158
2M
oroc
co–
–20
0234
51M
any
L6S4
W3
23.5
20.4
––
–31
.2B
e2N
WA
158
3M
oroc
co–
–20
01/2
002
78M
any
R3.
9–
––
–Se
e se
para
te e
ntry
––
15.6
Be2
NW
A 1
584
––
P 20
0232
501
LL5
S2W
128
.325
.2Pl
ag: A
b 76O
r 8;
Met
: Fe 6
3Ni 39
–M
oroc
co50
JSC
1
NW
A 1
585
––
P200
277
1R
5S2
W1
38.8
32.4
Plag
: Ab 8
6Or 8
–Er
foud
15JS
C1
NW
A 1
586
––
P 06
/200
240
01
Ure
––
––
See
sepa
rate
ent
ry–
Mor
occo
21.9
MIT
1N
WA
158
7–
–P
2000
50M
any
H4
S2W
1/2
18.2
14.9
––
–10
.7V
r1N
WA
158
8–
–P
2000
300
1H
3.8
S3W
0/1
17.4
16.6
Ol:
PMD
12.
7–
–21
Vr1
5.4–
20.3
6.0–
21.6
NW
A 1
589
––
P 20
0073
1H
5S3
W1
18.1
14.9
––
–15
.7V
r1N
WA
159
0Za
gora
––
2001
125.
41
LL5–
6S2
W3
28.7
23.7
––
–32
.9M
P2N
WA
159
1Ta
goun
ite–
–20
0125
4.8
1LL
5–6
S3W
328
.623
.7sv
––
24.2
MP2
NW
A 1
592
Aou
li–
–20
0111
271
L4S2
W2
21.3
15.9
––
–43
.3M
P2N
WA
159
3Ta
lsin
t–
–20
0118
7.4
1L5
/6S1
W2
24.2
20.3
––
–23
.9M
P2N
WA
159
4B
oum
ia–
–20
0128
5.7
1L6
S4W
224
.220
.3–
––
29.9
MP2
NW
A 1
595
Tals
int
––
2001
80.3
1L6
S4W
123
.720
.2–
––
14.9
MP2
NW
A 1
596
Zago
ra–
–20
0113
3.2
1L6
S5W
224
20.1
sv–
–27
.6M
P2N
WA
159
7Za
gora
––
2001
267.
71
L6S4
W1/
224
.120
.8sv
––
33.6
MP2
NW
A 1
598
Zago
ra–
–20
0124
6.1
1L6
S4W
1/2
24.4
20.8
––
–31
.1M
P2N
WA
159
9Ta
ta–
–20
0122
2.1
1H
4S4
W1
18.1
16.2
sv–
–31
.4M
P2N
WA
160
0Ta
goun
ite–
–20
0116
5.9
1H
5S2
W3
1815
.4–
––
28.9
MP2
NW
A 1
601
Zago
ra–
–20
0111
6.7
1H
5S4
W17
.916
.4–
––
31.3
MP2
NW
A 1
602
Bou
rfa
––
2001
143.
81
H5–
6S3
W2
17.8
15.8
––
–25
.6M
P2N
WA
160
3Ta
ta–
–20
0110
21
H5–
6S3
W2
18.5
16.5
––
–23
.6M
P2N
WA
160
4Ta
lsin
t–
–20
0112
9.6
1H
5S2
W2
17.6
15.2
br, s
v–
–27
.6M
P2N
WA
160
5Ta
ta–
–20
0110
0.4
1H
6S4
W0
18.3
15.7
––
–20
.3M
P2N
WA
160
6–
–20
0111
9.9
1H
4S2
W1
18.8
12.7
––
–26
.8M
P2N
WA
160
7B
ourf
a–
–20
0126
6.3
1H
6S4
W1
18.4
16.6
––
–28
.9M
P2N
WA
160
8B
ourf
a–
–20
0127
3.4
1H
4–6
S1W
211
.815
.8–
––
22.7
MP2
NW
A 1
609
Tago
unite
––
2001
359.
41
H4–
6S1
W2
16.7
15.9
––
–32
.8M
P2N
WA
161
0G
oura
ma
––
2001
158.
81
H6
S4W
018
.215
.8–
––
29.3
MP2
NW
A 1
644
––
–P
2001
21
41
Euc
pm–
––
–Se
e se
para
te e
ntry
––
20M
IT1
NW
A 1
646
––
–P
9/20
0225
91
Euc
cm–
––
–Se
e se
para
te e
ntry
–Za
gora
20U
WS2
NW
A 1
647
––
–P
9/20
0231
31
Euc
ub–
––
–Se
e se
para
te e
ntry
–Er
foud
20U
WS2
Meteoritical Bulletin No. 87 A239
Tabl
e 8.
Met
eorit
es fr
om M
oroc
co a
nd s
urro
undi
ng c
ount
ries.
a Con
tinue
d.
Nam
ePo
ssib
le o
rigin
/ ps
eudo
nym
bLa
titud
e(N
)cLo
ngtit
ude
(W)c
Dat
efo
undd
Mas
s(g
)Pc
s.C
lass
Shoc
kW
GFa (m
ol%
)Fs (m
ol%
)C
omm
ents
Mag
Suse
Plac
epu
rcha
sed
Type
Spec
(g)
Info
f
NW
A 1
648
––
–P
10/2
002
803
2D
io p
m–
––
–Se
e se
para
te e
ntry
–Za
gora
20U
WS2
NW
A 1
651
––
–P
2002
19.8
1LL
6S4
W1
28.6
24–
–M
oroc
co4
Be4
NW
A 1
652
––
–P
2002
68.3
1L
–W
124
.221
impa
ct m
elt r
ock
–M
oroc
co14
.40
Be4
NW
A 1
653
––
–P
2002
376
1H
ow–
––
–Se
e se
para
te e
ntry
–Za
gorr
a21
Be2
NW
A 1
654
––
–P
2002
491
Euc
ub–
––
–Se
e se
para
te e
ntry
–Za
gorr
a11
.30
Be2
NW
A 1
655
––
–P
2002
50.9
1C
O3
S2W
221
.72.
9–
–Za
gorr
a14
.1B
e20.
8–55
.20.
9–5.
5N
WA
165
6–
––
P 20
0243
1L6
S4W
124
.421
sv–
Zago
rra
11.5
Be2
NW
A 1
657
––
–P
2002
468
1L6
S4W
224
.520
.4–
–O
urgl
a,
Alg
erie
n21
.5B
e2
NW
A 1
658
––
–P
2002
1345
.50
6L3
–6–
––
–Se
e se
para
te e
ntry
–Za
gorr
a20
.5B
e2N
WA
165
9–
––
P 20
0230
1H
5S4
W1
18.7
16.3
––
Zago
rra
6.6
Be2
NW
A 1
660
––
–P
2002
287
1H
4S2
W1/
218
.216
.1–
–M
ahbe
s21
.6B
e2N
WA
166
1–
––
P 20
0212
3.4
1L3
/4S2
W3
22.6
15.8
––
Mah
bes
20.3
Be2
10–2
0.2
NW
A 1
662
––
–P
2002
124.
61
L6S6
W1/
224
.620
.7rw
, sv
–M
ahbe
s20
.6B
e2N
WA
166
3–
––
P 20
0280
.11
H5
S2W
318
.816
.6–
–M
ahbe
s16
.5B
e2N
WA
166
4Ta
belb
ala,
Alg
eria
~29°
32′
~3°1
1′20
0263
101
How
––
––
See
sepa
rate
ent
ry–
–25
8V
n2
NW
A 1
666
––
–P
10/2
002
320
1Eu
c pm
––
––
See
sepa
rate
ent
ry–
Den
ver
20U
WS1
NW
A 1
667
––
–P
10/2
002
1005
1D
io–
–29
.3–3
0.2
22.6
–25.
0C
hro:
Cr(
Cr+
Al)
= 0.
89–
Den
ver
20.8
UW
S1
NW
A 1
668
––
–P
10/2
002
710
1R
5–
–38
.930
.2aw
arui
te:
72%
Ni
–D
enve
r23
.6U
WS1
NW
A 1
669
Al M
ala’
ika
––
P 01
/01/
0336
1M
artia
n–
––
–Se
e se
para
te e
ntry
–Er
foud
7.4
UPV
I2N
WA
167
2–
––
P 9/
10/0
212
.75
Euc
ub–
––
59.6
fine-
grai
ned
–D
enve
r2.
6U
WS1
NW
A 1
692
––
–P
10/2
002
857
1H
5S1
W1
17.8
17–
–Sa
fsaf
21N
AU
2N
WA
169
3–
––
P 10
/200
283
1H
5S1
W2/
319
.117
.5–
–Sa
fsaf
15N
AU
2N
WA
169
5–
––
P 20
0161
41
How
––
––
See
sepa
rate
ent
ry–
Mor
occo
21N
AU
1N
WA
169
8–
––
P 3/
2002
698.
01
L5S1
W2
25.1
20.8
––
Erfo
ud50
.4Pr
1N
WA
169
9–
––
P 3/
2002
350.
01
L4/5
S2W
325
21–
–Er
foud
34.9
Pr1
NW
A 1
700
––
–P
3/20
0295
.01
L5S4
W3
23.4
19.8
––
Erfo
ud32
.1Pr
1N
WA
170
1–
––
P 3/
2002
225.
01
LL5
––
––
See
sepa
rate
ent
ry–
Erfo
ud20
.4Pr
1N
WA
170
2–
––
P 3/
2002
220.
01
H6
S4W
317
.718
.2–
–Er
foud
35.0
Pr1
NW
A 1
703
––
–P
3/20
02 2
64.0
1L6
S4W
324
.720
.7–
–Er
foud
23.7
Pr1
NW
A 1
704
––
–P
3/20
02 1
66.0
1H
5S3
W4
17.7
17.1
––
Erfo
ud20
.3Pr
1N
WA
170
5–
––
P 3/
2002
110.
01
L5S2
W3
22.6
19.8
––
Erfo
ud19
.2Pr
1N
WA
170
6–
––
P 3/
2002
148.
01
L6S3
W3
23.7
20.2
––
Erfo
ud23
.5Pr
1N
WA
170
7–
––
P 3/
2002
522.
01
L4S2
W3
24.8
20.7
––
Erfo
ud26
.5Pr
1N
WA
170
8–
––
P 3/
2002
11.1
1L5
S2W
324
.220
.4–
–Er
foud
2.2
Pr2
NW
A 1
713
––
–P
01/2
002
1073
1L6
S4W
125
.521
.5sv
–R
issa
ni31
Mün
3N
WA
171
4–
––
P 01
/200
269
71
H4/
5S3
W1
1917
sv–
Ris
sani
27M
ün3
NW
A 1
715
––
–P
01/2
002
361
1L6
S4W
125
21.5
sv, r
w, p
artly
S6
–R
issa
ni24
Mün
3N
WA
171
6–
––
P 01
/200
218
51
L5/6
S4W
125
.521
.5–
–R
issa
ni26
Mün
3N
WA
171
7A
tar,
Mau
ritan
ia~2
1°N
~13°
WP
12/2
002
6032
1LL
5–6
S4W
130
.525
sv, b
r, fr
ags o
f im
-pa
ct m
elt b
recc
ias
–H
ambu
rg21
Mün
3
NW
A 1
718
––
–P
12/2
002
858
1L6
S5W
1/2
25.5
21.5
sv–
Ham
burg
25M
ün3
A240 S. S. Russell et al.
Tabl
e 8.
Met
eorit
es fr
om M
oroc
co a
nd s
urro
undi
ng c
ount
ries.
a Con
tinue
d.
Nam
ePo
ssib
le o
rigin
/ ps
eudo
nym
bLa
titud
e(N
)cLo
ngtit
ude
(W)c
Dat
efo
undd
Mas
s(g
)Pc
s.C
lass
Shoc
kW
GFa (m
ol%
)Fs (m
ol%
)C
omm
ents
Mag
Suse
Plac
epu
rcha
sed
Type
Spec
(g)
Info
f
NW
A 1
757
Mor
occo
/A
lger
ia b
orde
r–
–20
0136
11
CO
3.5
S1W
30.
5–51
.81.
04–3
0.18
~30%
mat
rix,
man
y sm
all C
AIs
37.5
Erfo
ud–
Pa2
NW
A 1
758
Bou
dnib
are
a,
Mor
occo
––
08/2
001
66.4
1C
M2
S1W
10.
5–47
.21.
6tro
ilite
+
pent
land
ite–
Erfo
ud11
.1Pa
2
NW
A 1
759
Bou
dnib
are
a,
Mor
occo
––
06/2
001
10.1
1Eu
c pm
S3W
027
.8–3
9.5
–Se
e no
te 1
1–
Erfo
ud2
Pa2
NW
A 1
760
Bou
dnib
are
a,
Mor
occo
––
10/2
001
20.3
2Eu
c m
S4W
0–
–Se
e no
te 1
2–
Erfo
ud4
Pa2
NW
A 1
761
Ric
h ar
ea,
Mor
occo
––
2001
4560
1H
6S3
W3
19.9
17.4
orie
nted
ston
e–
Erfo
ud20
Pa2
NW
A 1
762
Ric
h ar
ea,
Mor
occo
––
2001
205.
51
L5S3
W1
25.5
21.4
nativ
e C
u–
Erfo
ud25
.2Pa
2
NW
A 1
763
Bou
dnib
are
a,
Mor
occo
––
10/2
001
57.1
1C
V3
S0W
00.
3–34
.90.
7–2.
3m
any
CA
Is–
Erfo
ud11
Pa2
NW
A 1
764
Zelm
ou, A
lger
ia–
–10
/200
125
517
Euc
mS3
W1
––
See
note
13;
br
–Er
foud
20.8
Pa2
NW
A 1
765
Ris
sani
are
a,
Mor
occo
––
2001
395
2LL
5S5
W1
28.9
23.3
sv–
Erfo
ud21
.2Pa
2
NW
A 1
766
Tals
int a
rea,
M
oroc
co–
–09
/200
136
9428
L6S4
W1
24.3
20.1
larg
est s
tone
64
5 g
–Er
foud
37Pa
2
NW
A 1
767
Tard
a, M
oroc
co–
–20
0113
Seve
ral
Euc
mS4
W1
–63
.1Se
e no
te 1
4; m
p–
Erfo
ud2.
6Pa
2N
WA
176
8M
oroc
co–
–20
029.
41
Euc
pmS3
/4W
1–
25.1
See
note
15
–Er
foud
1.8
Pa2
NW
A 1
770
Mor
occo
––
2002
221
LL3.
3S2
W2
1.3–
35.5
2.8–
29.1
inte
rlock
ed c
hon-
drul
es, r
are m
atrix
–Er
foud
4.5
Pa2
NW
A 1
771
Mor
occo
,A
lger
ia–
–20
017.
5Se
vera
lEu
c m
S3W
1–
–Se
e no
te 1
6–
Erfo
ud1.
5Pa
2
NW
A 1
774
Mor
occo
––
2002
714
1R
3.8–
6S4
W3
7.6–
40.1
0.4–
39.8
See
note
17;
br
–Er
foud
20Pa
2N
WA
177
5M
oroc
co–
–20
0225
Seve
ral
Mar
tian
W1/
236
.7-5
0.6
–Se
e no
te 1
8–
Erfo
ud4.
7Pa
2N
WA
177
6Za
gora
, M
oroc
co–
–20
0280
Seve
ral
CR
2S1
W2/
31.
1–33
.71.
9–35
.6Se
e no
te 1
9–
Erfo
ud16
Pa2
NW
A 1
777
Sobt
i, A
lger
ia–
–20
0210
551
Euc
pmS3
W1
–26
.5–5
0.7
See
note
20;
br
–Er
foud
20Pa
2N
WA
177
8D
akhl
a,
Wes
tern
Sa-
hara
,Mor
occo
––
2002
9500
0Se
vera
lL6
S1W
324
.422
.310
ston
es o
ver
1 kg
–Er
foud
20.6
Pa2
NW
A 1
779
Mor
occo
/A
lger
ia b
orde
r–
–20
0285
71
L5S5
W0
24.6
20.5
sv–
Erfo
ud20
Pa2
NW
A 1
780
Mor
occo
––
2002
25.5
71
Ure
W2
21.5
–se
e N
ote
21–
Erfo
ud5.
5Pa
2N
WA
178
1M
oroc
co–
–04
/01/
0010
21
H6
S5W
218
.816
.3–
–R
issa
ni39
Pa3
NW
A 1
782
M'H
amm
id,
Mor
occo
––
11/2
000
163
1U
re–
W3
21.7
–se
e N
ote
22–
Mor
occo
20.5
Pa3
NW
A 1
783
Tafh
raou
t are
a,
Mor
occo
––
11/0
1/00
413
1L3
.7S4
W4
31.1
–36.
916
.2-2
4.8
sv–
Mor
occo
20Pa
3
NW
A 1
784
Mor
occo
––
04/0
1/00
18
41
R4/
5S1
W3
40–
Ol:
NiO
0.2
1%–
Taou
z20
.5Pa
3N
WA
178
7M
oroc
co–
–02
/02
655.
71
L3.8
–5S2
W2
25.8
20.5
–26.
4–
–M
oroc
co25
.9Pa
4N
WA
178
8M
oroc
co–
–20
0135
.41
L3.8
–5S3
/4W
222
–27.
621
–23.
4br
–M
oroc
co35
.4Pa
5N
WA
179
1M
oroc
co–
–20
0090
01
L6S2
W3
24.8
20.7
––
Sain
te-M
arie
48.4
2Pa
6N
WA
179
2–
––
10/2
002
391
H5
S1W
218
.916
.8–
–Sa
fsaf
9.4
NA
U3
NW
A 1
793
––
–10
/200
258
51
L3S3
W1
23.4
19.5
––
Safs
af21
.1N
AU
3N
WA
179
4–
––
10/2
002
398
1LL
5S2
W1
30.2
24.3
––
Safs
af20
.0N
AU
3N
WA
179
5M
aurit
ania
––
2002
3300
0M
any
H5
S2W
418
.316
––
–21
.9B
e2N
WA
179
6M
aurit
ania
––
2002
2200
0M
any
H5
S3W
317
.415
.6–
––
20.6
Be2
NW
A 1
797
Mau
ritan
ia–
–20
0218
000
Man
yH
5S2
W1
1816
––
–21
Be2
Meteoritical Bulletin No. 87 A241
Tabl
e 8.
Met
eorit
es fr
om M
oroc
co a
nd s
urro
undi
ng c
ount
ries.
a Con
tinue
d.
Nam
ePo
ssib
le o
rigin
/ ps
eudo
nym
bLa
titud
e(N
)cLo
ngtit
ude
(W)c
Dat
efo
undd
Mas
s(g
)Pc
s.C
lass
Shoc
kW
GFa (m
ol%
)Fs (m
ol%
)C
omm
ents
Mag
Suse
Plac
epu
rcha
sed
Type
Spec
(g)
Info
f
NW
A 1
798
Mau
ritan
ia–
–20
0214
000
Man
yH
6S3
W2
17.1
15.3
––
–20
.6B
e2N
WA
179
9M
ahbe
s, M
oroc
co–
–20
0217
3.7
1L6
S4W
324
.520
.2–
––
20.6
Be2
NW
A 1
800
Mah
bes,
Mor
occo
––
2002
62.8
1H
4/5
S3W
317
.912
.7–
––
12.9
Be2
NW
A 1
801
Mah
bes,
Mor
occo
––
2002
264
1L4
S2W
122
.218
.7–
––
20.7
Be2
NW
A 1
802
Mah
bes,
Mor
occo
––
2002
518
1H
6S2
W1
18.3
16br
––
20.9
Be2
NW
A 1
803
Zago
ra–
–20
0298
.55
H5
S2W
117
.916
––
21.7
Be2
NW
A 1
804
Erfo
ud–
–20
021.
41
H5/
6S4
W2
18.3
16.1
br, s
v, m
p–
–22
.9B
e2N
WA
180
5M
oroc
co–
–20
0210
2.4
1L6
S2W
223
.819
.8–
––
21.6
Be4
NW
A 1
806
Mor
occo
––
2002
40.0
11
H3
S2W
219
.29.
7br
––
8.3
Be2
0.4–
84.2
1.2–
27.9
NW
A 1
811
Mor
occo
––
Unk
300
1LL
6S3
W1
2824
––
–24
Vr1
NW
A 1
812
Wes
tern
Sah
ara
––
Win
ter
2002
13.1
1LL
3.8
S1W
327
.3
(18.
3– 1
.0)
4.2–
23.1
Ol:
PMD
11.
3–
–2.
9V
r1
NW
A 1
813
Wes
tern
Sah
ara
––
Win
ter
2001
/270
1Eu
c pm
––
––
See
sepa
rate
ent
ry–
–14
Vr1
NW
A 1
814
––
–19
9915
61
Ben
cub-
bin-
like
––
––
See
sepa
rate
ent
ry–
–21
.0Pa
7
a Mos
t of t
hese
met
eorit
es w
ere
purc
hase
d fr
om M
oroc
can
deal
ers.
If in
form
atio
n w
as su
pplie
d by
a d
eale
r abo
ut w
here
the
spec
imen
may
hav
e be
en c
olle
cted
, thi
s is n
oted
inst
ead
of th
e la
titud
e an
d lo
ngitu
de.
Mos
t of t
he c
olle
ctio
n lo
catio
ns c
anno
t be
verif
ied.
b Met
eorit
es m
ay h
ave
been
sold
und
er so
me
of th
ese
nam
es o
r num
bers
. The
se a
re N
OT
reco
gniz
ed b
y th
e N
omen
clat
ure
Com
mitt
ee a
nd so
me
are
not u
niqu
ely
asso
ciat
ed w
ith th
e m
eteo
rite
clas
sifie
d in
this
tabl
e. O
nly
the
NW
A n
umbe
r sho
uld
be u
sed.
c Coo
rdin
ates
of p
lace
of s
uppo
sed
orig
in; n
ot a
ll re
ports
may
be
trust
wor
thy,
and
the
Nom
encl
atur
e C
omm
ittee
lack
s the
reso
urce
s to
inve
stig
ate.
d“P”
indi
cate
s a d
ate
of p
urch
ase,
oth
ers a
re re
porte
d da
tes o
f fin
d.A
bbre
viat
ions
: br =
bre
ccia
ted;
cal
c. v
. = c
alci
te v
eins
; mp
= m
elt p
ocke
ts; r
w =
ring
woo
dite
; sv
= sh
ock
vein
s.(1
) Oliv
ine
com
posi
tions
in ty
pe 1
cho
ndru
les,
Fa2.
2–20
, mea
n Fa
2.22
± 2
.9 (n
= 1
20);
in ty
pe 2
cho
ndru
les,
Fa30
–40,
mea
n Fa
34.8
± 7
.6 (n
= 8
0); o
livin
e in
mat
rix is
Fa 4
6.2
± 3.
6 (n
= 11
4); N
i in
met
al u
p to
30
wt%
;bu
lk c
hem
istry
ver
y si
mila
r to
Alle
nde
exce
pt fo
r dep
letio
n of
Ni a
nd C
o; fe
w sm
all C
AIs
; ver
y w
ell d
efin
ed c
hond
rule
s. (2
) pro
babl
y a
win
onai
te b
ut w
ith O
isot
opes
that
are
mor
e 16
O-r
ich
than
typi
cal:
18O
= 3.
57‰
, 17O
= 1
.33‰
, 17 0
= –0
.53‰
; man
y re
lict c
hond
rule
s. (3
) NW
A 1
187
and
NW
A 1
253
are
prob
ably
pai
red.
(4) N
WA
118
9, N
WA
124
4, N
WA
124
5, N
WA
124
6, N
WA
124
8, N
WA
124
9, N
WA
125
9an
d N
WA
126
0 ar
e pr
obab
ly p
aire
d. (5
) NW
A 1
251
and
1252
are
pro
babl
y pa
ired.
(6) C
o 5.
02 m
g/g,
Ni 7
8.9
mg/
g, C
u 16
7 µg
/g, G
a 18
.5 µ
g/g,
As
4.45
µg/
g, W
1.0
1 µg
/g, I
r 3.9
0 µg
/g, P
t 12.
3 µg
/g, A
u0.
664
µg/g
. (7)
low
-Ca
px: W
o 3.3
–13.
4, m
g# =
36–
68 m
ol%
hig
h-C
a px
, En 3
1Wo 4
4; Pl
ag, A
n 84.
7–92
.0; i
lmen
ite, M
gO =
0.5
7–0.
62 w
t.%. (
8) N
WA
127
1 an
d 12
72 a
re p
roba
bly
paire
d. (9
) Mt;
Ol:
<0.1
–0.4
wt%
NiO
; CA
Is a
nd fl
uffy
oliv
ine
aggr
egat
es. (
10) M
t; O
l: ~0
.5 w
t% N
iO; f
luffy
oliv
ine
aggr
egat
es; c
alc.
v. (
11) C
px: F
s 22.
2–48
.5W
o 9.1
–41.
3; Pl
ag: A
n 94.
7;SiO
2; co
arse
gab
broi
c te
xtur
e. (1
2) C
px: F
s 48.
6–53
.2W
o 7.4
–
13.7
; Pla
g: A
n 90.
9; Si
O2;
fine-
grai
ned.
(13)
Cpx
: Fs 3
0.6–
60.4
Wo 4
–40.
6; Pl
ag: A
n 88.
1. (1
4) C
px: F
s 27.
3–59
.6W
o 5.4
–46.
6; Pl
ag: A
n 90.
4. (1
5) C
px: F
s 43.
2–27
.8W
o 24.
5–42
.9; P
lag:
An 9
3.6.
(16)
Cpx
: Fs 6
0.4–
31.2
Wo 4
.2–3
7.4;
Plag
:A
n 89.
5. (1
7) C
px: F
s 29.
6–15
.7W
o 9.3
–39.
5; O
l: N
iO 0
.12.
(18)
bas
altic
sher
gotti
te; z
oned
oliv
ine p
heno
crys
ts in
a fin
e-gr
aine
d gr
ound
mas
s of c
ompl
exly
zone
d pi
geon
ite an
d ho
mog
enou
s mas
kely
nite
; Cpx
: Fs 2
4.33
–
36.3
8Wo 8
.89–
28.7
8; m
aske
lyni
te: A
n 51.
23A
b 46.
49; p
aire
d w
ith N
WA
106
8, 1
110
and
1183
. (19
) met
al-r
ich
chon
drul
es, s
mal
l CA
Is in
sul
fide-
rich
mat
rix; p
aire
d w
ith N
WA
801
Pla
g: A
n 85.
2. (2
0) C
px: F
s 28.
2–
57.1
Wo 4
2.5–
7; Pl
ag: A
b 92.
(21)
Cpx
: Fs 6
.7–1
8.1W
o 12.
5–4.
4, C
r 2O
3 1.0
–1.3
; Ol:
Cr 2
O3 0
.66–
0.81
, CaO
0.3
4. (2
2) C
px: F
s 9.4
Wo 8
.2, C
r 2O
3 1.1
; Ol:
CaO
0.2
8–0.
32, C
r 2O
3 0.5
1–0.
75.
e Mag
Sus
: giv
es th
e de
cim
al lo
garit
hm o
f mag
netic
susc
eptib
ility
(in
10−9
m3 k
g−1 )
. Acc
ordi
ng to
Roc
hette
et a
l. (2
003)
, thi
s par
amet
er (a
mea
sure
of t
he a
mou
nt o
f met
al) s
houl
d be
in th
e ra
nge
5.1–
5.5
for H
,4.
6–5.
0 fo
r L, 3
.6–4
.5 fo
r LL.
On
the
othe
r han
d, a
dec
reas
e of
abo
ut 0
.1 p
er W
G is
obs
erve
d.f S
ee “
Abb
revi
atio
ns fo
r ana
lyst
s and
spec
imen
loca
tions
.”
A242 S. S. Russell et al.
Tabl
e 9.
Sah
aran
met
eorit
es fr
om N
iger
.
Nam
eD
ate
foun
dLa
titud
e(N
)Lo
ngtit
ude
(E)
Mas
s(g
)Pi
eces
Cla
ssSh
ock
WG
Fa (mol
%)
Fs (mol
%)
Com
men
ts
Type
spec
(g
)In
foa
a See
“A
bbre
viat
ions
for a
naly
sts a
nd sp
ecim
en lo
catio
ns.”
Adr
ar B
ous
11/2
001
~20°
30′
~9°0
0′36
01
EL5
–W
2–
1.23
–41
.3Pa
10A
resh
ima
03/0
2/99
18°1
2.74′
10°1
0.66′
114.
31
LL3.
7S3
W1
5–31
10–2
6–
114.
3Pa
11Ta
sséd
et00
110
/12/
0118
°04.
10′
6°40
.10′
560
1H
5S3
W1
17.3
15.1
001,
002
, and
003
ar
e pro
babl
y pa
ired
27.5
Ham
2
002
10/1
4/01
18°1
4.22′
6°31
.19′
9.4
1H
5S3
W1
17.6
15.6
–2.
16H
am2
003
10/1
4/01
18°1
8.02′
6°30
.41′
12.5
1H
5S3
W1
17.8
–3.
54H
am2
Poin
t B
erlie
t11
/200
120
°32.
22′
9°32
.27′
4200
01
H5
S1W
219
.017
.2–
24.3
Pa10
Ségu
édin
e20
0220
°49.
10′
12°5
8.40′
444
1H
6S3
W1
18.1
16.3
–14
.2B
e7Ti
ffa 0
0702
/15/
0120
°12.
07′
11°3
5.22′
9250
1H
5S1
/2W
118
.617
.1–
102.
2Pa
11
Meteoritical Bulletin No. 87 A243
Tabl
e 10
. Met
eorit
es fr
om th
e Sa
hara
, loc
atio
ns u
nkno
wn.
Nam
eFo
und
Latit
udea
a The
geo
grap
hic
coor
dina
tes o
f the
se m
eteo
rites
hav
e no
t bee
n di
sclo
sed
by th
e fin
der.
List
ed a
re th
e of
fset
s rel
ativ
e to
a se
cret
orig
in.
Long
itude
aM
ass
(g)
Piec
esC
lass
Shoc
kW
GFa (m
ol%
)Fs (m
ol%
)C
omm
ents
b
b Abb
revi
atio
ns: b
r–br
ecci
ated
; v–v
eine
d.
Type
spec
(g)
Info
c
c See
“A
bbre
viat
ions
for a
naly
sts a
nd sp
ecim
en lo
catio
ns.”
Saha
ra98
120
1998
z+0°
04′1
0′′
w+0
°16′
02′′
138
1L6
S2W
426
.022
.3–
19.7
Pa12
9815
419
98z+
0°07′3
2′′
w+0
°17′
46′′
817
1H
5S2
W3
17.5
16.2
–27
8.3
Pa12
9832
819
99z+
0°05′0
5′′
w+0
°23′
04′′
187
1L4
S4W
225
.520
.3–
26.7
Pa12
9846
519
98z+
0°08′5
4′′
w+0
°28′
21′′
226
1L4
S3/S
4W
224
.721
.3–
22Pa
1298
532
1998
z+0°
08′1
9′′
w+0
°28′
38′′
258
1L4
S2W
125
.520
.7–
20.6
Pa12
9857
319
98z+
0°06′1
0′′
w+0
°16′
01′′
175
1L3
.8S3
W1
25.9
19.7
br20
.3Pa
1298
804
1998
z+0°
06′3
2′′
w+0
°16′
15′′
621
H4
S1W
3/4
17.7
17.2
–13
.0Pa
1299
029
1999
z+0°
08′4
1′′
w+0
°08′
20′′
250
1L6
S4W
124
.8 ±
0.9
20.3
± 0
.2br
, v21
Bar
t899
067
1999
z+0°
09′5
0′′
w+0
°28′
02′′
207
1H
3.8
S2W
220
.112
.5–
19.5
–99
070
1999
z+0
°09′
52′′
w+0
°29′
13′′
1780
1H
3.8–
6S2
W2
18.7
21.1
br27
Pa12
9916
219
99z+
0°09′4
2′′
w+0
°29′
01′′
144
1H
6S2
W1/
220
.817
.8v
21.7
Pa12
9920
919
99z+
0°11′3
3′′
w+0
°02′
01′′
230
1L5
–6S4
W1
24.6
± 0
.620
.3 ±
0.6
br, v
21B
art9
9932
719
99z+
0°09′3
0′′
w+0
°28′
16′′
3320
1H
6S1
W3
19.6
17.2
–25
Pa12
9933
019
99z+
0°09′4
0′′
w+0
°28′
36′′
14.7
1LL
3.5
S1W
2/3
0.7–
211–
20–
3.0
Pa12
9955
019
99z+
0°06′1
5′′
w+0
°16′
06′′
213
1L4
S3W
225
.622
.4–
21.2
Pa12
9957
219
99z+
0°06′3
1′′
w+0
°15′
51′′
730
1H
6S1
W1/
219
.817
.7–
44Pa
1299
603
1999
z+0°
04′0
8′′
w+0
°20′
39′′
476
1L6
S4W
124
.0 ±
1.1
20.3
± 0
.8br
, v20
Bar
t10
0001
920
00z+
0°12′0
0′′
w+0
°26′
30′′
1665
1L3
.8S3
W3
24.4
21.0
–30
Pa12
0017
720
00z+
0°06′8
7′′
w+0
°09′
25′′
121
C3/
4–
––
–Se
e se
para
te e
ntry
4Pa
1200
181
2000
z+0°
07′0
2′′
w+0
°09′
26′′
191
1H
4-6
S3W
220
.817
.2br
22Pa
12
A244 S. S. Russell et al.
App
endi
x 1.
Rec
ently
des
crib
ed m
eteo
rites
from
the
U.S
. AN
SMET
exp
editi
ons.
a
Nam
ebC
lass
Mas
s (g
)W
eath
%Fa
%Fs
Pairi
ngIc
ecR
ef
BTN
003
01H
3.3
33.7
7B
8–38
5–21
(3)
2525
(2)
BTN
003
02H
3.3
37.0
6B
1–32
4–19
0030
125
25(2
)B
TN 0
0303
H3.
315
.81
B1–
302–
1900
301
2525
(2)
BTN
003
04LL
670
9A
––
–25
26(1
)B
TN 0
0305
L531
6.4
B–
––
–26
(1)
BTN
003
06L5
66.9
5B
/C–
––
2526
(1)
BTN
003
07L6
130.
05B
––
––
26(1
)B
TN 0
0308
L510
.69
C–
––
2525
(2)
BTN
003
09L5
24.0
8B
––
–25
25(2
)B
TN 0
0310
LL6
20.6
1A
/B–
––
–26
(1)
CR
E 01
400
HO
W14
1.3
B–
21–5
3–
–26
(1)
FIN
001
00H
539
.61
B18
16–
–26
(1)
FIN
001
01H
412
1.79
B18
16–
–26
(1)
FIN
001
02H
578
.11
B19
16–
–26
(1)
FIN
016
00H
587
6.2
B18
16–
–26
(1)
FIN
016
01L6
287.
5B
2420
––
26(1
)FI
N 0
1602
H5
94.8
4B
1916
––
26(1
)FI
N 0
1603
L558
3.8
A24
20–
–26
(1)
FIN
016
04H
518
6.17
B18
16–
–26
(1)
FIN
016
05H
510
2.59
B19
16–
–26
(1)
MET
004
29C
V3
30.4
9B
1–28
1–3
(2)
–25
(2)
MET
004
30C
V3
151.
7B
0–9
0–2
0042
9–
25(2
)M
ET 0
0449
LL6
1192
.3C
––
––
26(1
)M
ET 0
0450
LL6
691.
1B
e–
––
–26
(1)
MET
004
51LL
676
7.2
Be
––
––
26(1
)M
ET 0
0452
H3.
577
4.9
B/C
e2–
197
––
25(2
)M
ET 0
0453
LL6
265.
6B
/C–
––
–26
(1)
MET
004
54LL
648
7B
/C–
––
–26
(1)
MET
004
55L5
489
B25
21–
–25
(2)
MET
004
56H
557
5.5
A/B
1816
––
25(2
)M
ET 0
0456
LL5
575.
5A
/B–
––
–26
(1)
MET
004
57LL
670
9.4
B/C
––
––
26(1
)M
ET 0
0458
LL6
687.
5B
––
–26
26(1
)M
ET 0
0459
LL6
1118
.7B
––
––
26(1
)M
ET 0
0460
H5
700.
5B
1917
––
25(2
)M
ET 0
0461
L651
8B
/C–
––
–25
(2)
MET
004
62L5
590.
7C
––
––
26(1
)M
ET 0
0463
L636
9.9
A/B
––
––
26(1
)M
ET 0
0464
LL6
418.
9A
/B–
––
–26
(1)
MET
004
65L5
516.
4B
/C–
––
–26
(1)
MET
004
66LL
529
6.8
B–
––
–26
(1)
MET
004
67L5
422.
5B
––
––
26(1
)M
ET 0
0468
L536
1.7
B–
––
–26
(1)
MET
004
69L5
273
B/C
––
––
26(1
)M
ET 0
0470
LL6
456.
2B
/C–
––
–26
(1)
MET
004
71L5
367.
1A
/B–
––
–26
(1)
MET
004
72L6
348.
3C
e–
––
–26
(1)
App
endi
x 1.
Rec
ently
des
crib
ed m
eteo
rites
from
the
U.S
. AN
SMET
exp
editi
ons.
a Continued.
Nam
ebC
lass
Mas
s (g
)W
eath
%Fa
%Fs
Pairi
ngIc
ecR
ef
MET
004
73LL
627
0B
––
––
26(1
)M
ET 0
0474
LL5
153.
26A
/B–
––
–26
(1)
MET
004
75LL
636
7.8
B/C
––
––
26(1
)M
ET 0
0476
L543
3.3
B/C
––
––
26(1
)M
ET 0
0477
LL6
474.
2A
/B–
––
–26
(1)
MET
004
78L5
343
A/B
––
––
26(1
)M
ET 0
0479
LL6
315
B/C
––
––
26(1
)M
ET 0
0480
L519
0.49
B–
––
–26
(1)
MET
007
81C
M2
5.36
B0–
303–
600
431
–26
(1)
MET
007
82H
610
.59
C–
––
–26
(1)
MET
007
83EH
426
.25
C–
0–1
0063
6–
26(1
)M
ET 0
0784
H4
7.51
B–
––
–26
(1)
MET
007
85L5
21.2
5C
––
––
26(1
)M
ET 0
0786
L515
.63
B–
––
–26
(1)
MET
007
87H
638
.11
C–
––
–26
(1)
MET
007
88L5
35.2
7B
––
––
26(1
)M
ET 0
0789
LL6
13.8
5B
/C–
––
–26
(1)
MET
007
90L5
35.7
8B
/C–
––
–26
(1)
MET
007
91L5
9.89
A/B
––
––
26(1
)M
ET 0
0792
L549
.59
B/C
––
––
26(1
)M
ET 0
0793
H6
40.0
5B
/C–
––
–26
(1)
MET
007
94LL
660
.88
B–
––
–26
(1)
MET
007
95H
641
.7C
––
––
26(1
)M
ET 0
0796
L544
.7A
/B–
––
–26
(1)
MET
007
97LL
644
.57
B–
––
–26
(1)
MET
007
98H
628
.1C
e–
––
–26
(1)
MET
007
99L5
51.4
2B
/C–
––
–26
(1)
MET
008
00H
OW
1.72
A–
24–6
096
500
–26
(1)
MET
008
01LL
637
.23
A–
––
–26
(1)
MET
008
02H
681
.20
C–
––
–26
(1)
MET
008
03L5
15.4
1B
/C–
––
–26
(1)
MET
008
04LL
619
.35
B–
––
–26
(1)
MET
008
05H
646
.50
C–
––
–26
(1)
MET
008
06L5
13.6
2B
––
––
26(1
)M
ET 0
0807
LL6
38.5
7A
/B–
––
–26
(1)
MET
008
08LL
630
.69
B/C
––
––
26(1
)M
ET 0
0809
LL6
35.8
9B
/C–
––
–26
(1)
MET
008
10C
M2
5.91
B0–
282
0043
1–
26(1
)M
ET 0
0812
IIIA
B4.
96–
––
0040
0–
26(1
)M
ET 0
0820
LL6
32.6
8B
/C–
––
–26
(1)
MET
008
21H
618
.14
C–
––
–26
(1)
MET
008
22L5
5.97
C–
––
–26
(1)
MET
008
23LL
521
.02
B–
––
–26
(1)
MET
008
24H
550
.92
C–
––
–26
(1)
MET
008
25L5
40.3
5C
––
––
26(1
)M
ET 0
0826
LL6
38.1
1C
––
––
26(1
)M
ET 0
0827
LL5
6.96
B–
––
–26
(1)
Meteoritical Bulletin No. 87 A245
App
endi
x 1.
Rec
ently
des
crib
ed m
eteo
rites
from
the
U.S
. AN
SMET
exp
editi
ons.
a Continued.
Nam
ebC
lass
Mas
s (g
)W
eath
%Fa
%Fs
Pairi
ngIc
ecR
ef
MET
008
28LL
52.
78B
––
––
26(1
)M
ET 0
0829
L613
.91
B–
––
–26
(1)
MET
008
34II
IAB
7.05
––
–00
400
–26
(1)
MET
008
55D
IO9.
09B
/C–
27–
–26
(1)
MET
008
64II
IAB
38.0
3–
––
0040
0–
26(1
)M
ET 0
0880
L513
.07
B/C
––
––
26(1
)M
ET 0
0881
H6
23.8
3C
––
––
26(1
)M
ET 0
0882
LL6
36.3
3B
/C–
––
–26
(1)
MET
008
83LL
640
.61
B/C
––
––
26(1
)M
ET 0
0884
H6
9.40
C–
––
–26
(1)
MET
008
85L5
30.9
9C
––
––
26(1
)M
ET 0
0886
LL6
8.75
C–
––
–26
(1)
MET
008
87H
619
.16
C–
––
–26
(1)
MET
008
88L5
21.6
6C
––
––
26(1
)M
ET 0
0889
LL6
36.1
2C
––
––
26(1
)M
ET 0
0890
L537
.63
C–
––
–26
(1)
MET
008
91H
61.
43C
––
––
26(1
)M
ET 0
0892
LL5
25.5
3A
––
–26
26(1
)M
ET 0
0893
L54.
99B
––
––
26(1
)M
ET 0
0894
H6
15.0
8C
––
––
26(1
)M
ET 0
0895
H6
17.9
7C
––
––
26(1
)M
ET 0
0896
L520
.75
C–
––
–26
(1)
MET
008
97L5
20.9
4C
––
––
26(1
)M
ET 0
0898
H6
23.2
8C
––
––
26(1
)M
ET 0
0899
H5
18.0
1C
––
––
26(1
)M
ET 0
0900
L523
.7B
/C–
––
–26
(1)
MET
009
01H
66.
96B
/C–
––
–26
(1)
MET
009
02H
620
.95
B/C
––
––
26(1
)M
ET 0
0903
H5
21.8
2B
/C–
––
–26
(1)
MET
009
04L5
44.9
5B
/C–
––
–26
(1)
MET
009
05II
IAB
3.53
––
–00
400
–26
(1)
MET
009
06H
57.
89B
/C–
––
–26
(1)
MET
009
07LL
639
B/C
––
––
26(1
)M
ET 0
0908
L513
.05
B/C
––
––
26(1
)M
ET 0
0909
H5
7.44
B/C
––
––
26(1
)M
ET 0
0910
LL6
5.06
A/B
––
––
26(1
)M
ET 0
0911
H6
33.4
8B
/C–
––
–26
(1)
MET
009
12H
627
.62
B/C
––
––
26(1
)M
ET 0
0913
H6
17.7
2B
/C–
––
–26
(1)
MET
009
14LL
612
.95
B/C
––
––
26(1
)M
ET 0
0915
LL6
11.4
3B
/C–
––
–26
(1)
MET
009
16H
615
.29
C–
––
–26
(1)
MET
009
17LL
543
.93
B–
––
–26
(1)
MET
009
18L5
15.0
3B
/C–
––
–26
(1)
MET
009
19LL
67.
41B
/C–
––
–26
(1)
MET
009
44L4
19.0
7A
2319
––
26(1
)M
ET 0
0968
L49.
63B
2310
–20
––
26(1
)
App
endi
x 1.
Rec
ently
des
crib
ed m
eteo
rites
from
the
U.S
. AN
SMET
exp
editi
ons.
a Continued.
Nam
ebC
lass
Mas
s (g
)W
eath
%Fa
%Fs
Pairi
ngIc
ecR
ef
MET
001
012
CM
27.
1A
/B0–
234–
500
431
–26
(1)
MET
001
038
Iron
-Ung
3.69
––
–00
428
–26
(1)
MET
001
060
DIO
9.84
C–
19–
–26
(1)
MET
001
087
CM
21.
60A
0–41
0–1
––
26(1
)M
ET 0
0113
6II
IAB
3.21
––
–00
400
–26
(1)
MET
010
70C
M1
40.5
9B
e–
–(3
)–
25(2
)M
ET 0
1071
CM
24.
50B
0–61
2–4
(4)
–25
(2)
MET
010
72C
M2
38.5
0B
0–12
–01
071
–25
(2)
MET
010
73C
M1
15.7
2B
––
0107
0–
25(2
)M
ET 0
1074
CV
346
.20
B0–
90–
2(2
)–
25(2
)M
ET 0
1075
CM
229
.94
B0–
46–
0107
1–
25(2
)M
ET 0
1076
CM
29.
21B
1–36
1–16
(2)
–25
(2)
MET
010
77C
M2
18.9
1C
0–53
1–8
0107
6–
25(2
)M
ET 0
1078
CM
219
.46
B1–
41–
0107
1–
25(2
)M
ET 0
1079
CM
111
.51
B–
–01
070
–25
(2)
MET
010
80C
V3
3.45
B0–
241–
201
074
–25
(2)
MET
010
81EU
C-U
br27
.40
A/B
–26
–56
(2)
–26
(1)
MET
010
82H
OW
22.1
4B
/C–
21–5
796
500
–26
(1)
MET
010
83U
RE
12.6
2B
88
––
25(2
)M
ET 0
1084
DIO
4.29
B30
26–
–26
(1)
MET
010
85U
RE-
An
30.6
1B
–11
––
25(2
)M
ET 0
1086
EUC
-Ubr
2.73
A/B
–28
–56
0108
1–
26(1
)M
ET 0
1087
HO
W28
.41
B26
19–5
296
500
–26
(1)
MET
010
90L4
3.52
C25
21–
–26
(1)
MET
010
91LL
68.
60A
––
––
26(1
)O
DE
0150
0H
552
08.9
B/C
1917
––
26(1
)O
DE
0150
1H
520
.92
B/C
1816
––
26(1
)Q
UE
9942
0LL
52.
08B
––
–F
26(1
)Q
UE
9942
1LL
51.
97B
––
–F
26(1
)Q
UE
9942
2LL
52.
81B
/C–
––
F26
(1)
QU
E 99
423
L60.
68C
––
–F
26(1
)Q
UE
9942
4LL
54.
46B
/C–
––
F26
(1)
QU
E 99
425
H4
0.25
C18
15–
2226
(1)
QU
E 99
426
LL5
2.19
B/C
––
–22
26(1
)Q
UE
9942
7LL
50.
15B
––
–F
26(1
)Q
UE
9942
8LL
54.
66A
/B–
––
F26
(1)
QU
E 99
429
LL5
3.19
B–
––
F26
(1)
QU
E 99
473
EH0.
27B
/C–
1–2
–F
25(2
)Q
UE
9961
0L6
59.5
2A
/B–
––
2425
(2)
QU
E 99
611
L589
.58
B/C
––
–F
25(2
)Q
UE
9961
2LL
564
.30
A/B
––
–F
25(2
)Q
UE
9961
3LL
537
.55
A/B
––
–F
25(2
)Q
UE
9961
4LL
531
.17
A/B
––
–F
25(2
)Q
UE
9961
5LL
546
.92
A/B
––
–F
25(2
)Q
UE
9961
6LL
527
.82
A/B
––
–F
25(2
)Q
UE
9961
7LL
536
.32
A/B
––
–F
25(2
)Q
UE
9961
8LL
527
.04
A/B
––
–F
25(2
)
A246 S. S. Russell et al.
App
endi
x 1.
Rec
ently
des
crib
ed m
eteo
rites
from
the
U.S
. AN
SMET
exp
editi
ons.
a Continued.
Nam
ebC
lass
Mas
s (g
)W
eath
%Fa
%Fs
Pairi
ngIc
ecR
ef
QU
E 99
619
LL5
51.8
3A
/B–
––
F25
(2)
QU
E 99
620
LL5
29.3
2A
/B–
––
F25
(2)
QU
E 99
621
LL5
21.6
3B
––
–F
25(2
)Q
UE
9962
2LL
529
.79
B/C
––
–F
25(2
)Q
UE
9962
3LL
55.
51B
/C–
––
F25
(2)
QU
E 99
624
LL5
4.31
B–
––
F25
(2)
QU
E 99
625
LL5
5.84
B–
––
F25
(2)
QU
E 99
626
LL5
4.86
3B
/C–
––
F25
(2)
QU
E 99
627
LL5
3.42
9B
––
–F
25(2
)Q
UE
9962
8LL
59.
45A
/B–
––
F25
(2)
QU
E 99
629
LL5
6.15
5B
/C–
––
F25
(2)
QU
E 99
650
LL5
1.33
5B
––
–F
25(2
)Q
UE
9965
1LL
53.
636
B–
––
F25
(2)
QU
E 99
652
LL5
2.24
2B
––
–F
25(2
)Q
UE
9965
3LL
54.
845
B–
––
F25
(2)
QU
E 99
654
LL5
5.08
5B
––
–F
25(2
)Q
UE
9965
5LL
52.
292
B–
––
F25
(2)
QU
E 99
656
LL5
3.36
4B
/C–
––
F25
(2)
QU
E 99
657
LL5
1.43
6B
––
–F
25(2
)Q
UE
9965
9LL
57.
339
B–
––
F25
(2)
QU
E 99
660
LL5
10.1
A/B
––
–F
25(2
)Q
UE
9966
1LL
52.
643
A/B
––
–F
25(2
)Q
UE
9966
2LL
512
.787
A/B
––
–F
25(2
)Q
UE
9966
3LL
524
.91
A/B
––
–F
25(2
)Q
UE
9966
4LL
54.
613
B/C
––
–F
25(2
)Q
UE
9966
5LL
56.
561
B/C
––
–F
25(2
)Q
UE
9966
6LL
510
.298
A/B
––
–F
25(2
)Q
UE
9966
7LL
510
.086
A/B
––
–F
25(2
)Q
UE
9966
8LL
514
.96
A/B
––
–F
25(2
)Q
UE
9966
9LL
534
.206
A/B
e–
––
F25
(2)
QU
E 99
670
H5
2.39
7C
––
–F
25(2
)Q
UE
9967
1LL
51.
015
B/C
––
–F
25(2
)Q
UE
9967
2LL
51.
011
B–
––
F25
(2)
QU
E 99
673
LL5
2.18
8B
––
–F
25(2
)Q
UE
9967
4LL
51.
144
B/C
––
–F
26(1
)Q
UE
9968
0C
K5
15.6
77C
e29
21(2
)F
25(2
)Q
UE
9968
1C
K5
3.95
2C
e29
2399
680
F25
(2)
QU
E 99
682
LL5
33.4
25B
/C–
––
F25
(2)
QU
E 99
683
H5
43.2
55C
––
–F
25(2
)Q
UE
9968
4L5
63.8
24C
––
–F
25(2
)Q
UE
9968
5LL
59.
034
B/C
––
–F
25(2
)Q
UE
9968
6LL
518
.1B
/C–
––
F25
(2)
QU
E 99
687
LL5
11.0
88B
/C–
––
F25
(2)
QU
E 99
688
LL6
10.5
86B
––
–F
25(2
)Q
UE
9968
9LL
57.
211
B–
––
F25
(2)
QU
E 99
870
LL5
4.19
8B
––
–F
25(2
)Q
UE
9987
1LL
57.
428
B–
––
F25
(2)
QU
E 99
872
LL5
7.02
7B
––
–F
25(2
)
App
endi
x 1.
Rec
ently
des
crib
ed m
eteo
rites
from
the
U.S
. AN
SMET
exp
editi
ons.
a Continued.
a See
“N
otes
to T
able
2”
in th
e M
eteo
ritic
al B
ulle
tin 7
9 (1
996)
for e
xpla
natio
n of
col
umns
.
Nam
eb
b Abb
revi
atio
ns fo
r met
eorit
e na
mes
: BTN
= B
ates
Nun
atak
s; C
RE
= M
t. C
rean
; FIN
= F
inge
r Rid
ge;
MET
= M
eteo
rite
Hill
s; Q
UE
= Q
ueen
Ale
xand
ra R
ange
; TEN
= T
enta
cle
Rid
ge.
Cla
ssM
ass
(g)
Wea
th%
Fa%
FsPa
iring
Icec
c Ice
fiel
d na
mes
: 22
= W
. Fog
gy B
otto
m M
orai
ne; 2
4 =
Nor
th T
ail's
End
Icef
ield
; 25
= B
ates
Nor
th;
26 =
Low
er V
ee; F
= G
oodw
in N
unat
aks I
cefie
lds;
S =
Mar
e M
eteo
ritic
as.
Ref
QU
E 99
873
LL5
0.20
1B
––
–F
25(2
)Q
UE
9987
4LL
54.
174
B–
––
F25
(2)
QU
E 99
875
LL5
0.8
B–
––
F25
(2)
QU
E 99
876
LL5
7.31
9B
––
–F
25(2
)Q
UE
9987
7LL
516
.791
B–
––
F25
(2)
QU
E 99
878
LL5
2.19
8B
/C–
––
F25
(2)
QU
E 99
879
LL5
4.01
8B
/C–
––
F25
(2)
QU
E 99
880
LL5
5.09
5B
––
–F
25(2
)Q
UE
9988
1LL
57.
309
B–
––
F25
(2)
QU
E 99
882
H5
30.9
B/C
––
–F
25(2
)Q
UE
9988
3LL
54.
938
A/B
––
–F
25(2
)Q
UE
9988
4LL
60.
514
A/B
––
–F
25(2
)Q
UE
9988
5LL
58.
869
A/B
––
–F
25(2
)Q
UE
9988
6C
M2
15.3
1B
0–43
1–
F25
(2)
QU
E 99
887
LL5
13.8
42B
/C–
––
F25
(2)
QU
E 99
888
LL5
6.10
2A
/B–
––
F25
(2)
QU
E 99
889
LL5
12.3
32B
––
–F
25(2
)Q
UE
9989
0LL
541
.863
B/C
––
–F
25(2
)Q
UE
9989
1LL
546
.975
B/C
––
–F
25(2
)Q
UE
9989
2LL
511
.387
B–
––
F25
(2)
QU
E 99
893
LL5
22.1
62B
/C–
––
F26
(1)
QU
E 99
894
LL5
14.6
33B
––
–F
25(2
)Q
UE
9989
5LL
59.
933
B–
––
F25
(2)
QU
E 99
896
LL6
8.79
6B
/C–
––
F25
(2)
QU
E 99
897
LL5
8.33
B–
––
F25
(2)
QU
E 99
898
LL5
6.94
8B
––
–F
25(2
)Q
UE
9989
9LL
512
.516
B–
––
F25
(2)
QU
E 99
900
L511
.511
B–
––
F25
(2)
QU
E 99
901
LL5
7.73
6B
––
–F
25(2
)Q
UE
9990
2LL
51.
34B
/C–
––
F25
(2)
QU
E 99
903
LL5
0.33
7B
/C–
––
F25
(2)
QU
E 99
904
LL5
3.73
2A
/B–
––
F25
(2)
QU
E 99
905
LL5
7.00
5A
/B–
––
F25
(2)
QU
E 99
906
LL5
3.04
3B
––
–F
25(2
)Q
UE
9990
7LL
53.
244
A/B
––
–F
25(2
)Q
UE
9990
8LL
50.
364
C–
––
F25
(2)
QU
E 99
909
LL5
1.39
6A
/B–
––
F25
(2)
QU
E 99
910
LL5
0.49
6B
/C–
––
F25
(2)
QU
E 99
911
LL5
0.75
7B
/C–
––
F25
(2)
QU
E 99
912
LL5
1.01
3B
/C–
––
F25
(2)
TEN
000
01L6
11.1
43B
/C24
21–
–25
(2)
TEN
000
02L6
19.8
47B
/C24
21–
–25
(2)
Meteoritical Bulletin No. 87 A247
App
endi
x 2.
Rec
ently
des
crib
ed m
eteo
rites
from
Jap
anes
e N
IPR
exp
editi
ons.
Nam
eC
lass
Mas
s (g
)W
eath
FaFs
Ref
A-8
8003
6L6
14.3
3B
/C24
.220
.1N
IPR
MN
11(
1)A
-880
042
L610
.86
A/B
24.0
20.6
NIP
R M
N 1
1(1)
A-8
8005
5L6
11.2
9A
/B25
.220
.8N
IPR
MN
11(
1)A
-880
067
H5
61.4
0C
19.2
16.3
NIP
R M
N 1
1(1)
A-8
8006
8H
537
.98
C18
.616
.5N
IPR
MN
11(
1)A
-880
069
H5
43.3
0C
18.6
16.1
NIP
R M
N 1
1(1)
A-8
8007
0H
510
0.55
C18
.816
.2N
IPR
MN
11(
1)A
-880
071
H5
57.4
5C
18.7
16.0
NIP
R M
N 1
1(1)
A-8
8007
2H
525
.66
C18
.816
.2N
IPR
MN
11(
1)A
-880
073
H5
54.9
7C
18.7
16.3
NIP
R M
N 1
1(1)
A-8
8060
1H
428
.70
A18
.316
.0N
IPR
MN
11(
1)A
-880
602
H4
91.3
6B
17.5
15.4
NIP
R M
N 1
1(1)
A-8
8060
4H
524
.19
C18
.215
.9N
IPR
MN
11(
1)A
-880
605
H6
79.2
0B
18.9
16.2
NIP
R M
N 1
1(1)
A-8
8060
6H
519
.14
B/C
18.6
16.1
NIP
R M
N 1
1(1)
A-8
8060
9H
462
.10
B17
.215
.3N
IPR
MN
11(
1)A
-880
613
H3
190.
86A
/B9.
5–20
.71.
0–31
.4N
IPR
MN
11(
1)A
-880
614
H5
11.9
3C
18.4
16.3
NIP
R M
N 1
1(1)
A-8
8061
5H
549
6.51
B18
.416
.2N
IPR
MN
11(
1)A
-880
616
H5
74.3
9B
19.6
16.8
NIP
R M
N 1
1(1)
A-8
8061
7L6
35.4
7A
24.9
20.8
NIP
R M
N 1
1(1)
A-8
8061
8H
416
.07
B/C
17.6
15.7
NIP
R M
N 1
1(1)
A-8
8062
0H
399
.57
A/B
7.6–
28.3
3.4–
20.7
NIP
R M
N 1
1(1)
A-8
8062
1Eu
c48
.62
A–
30.2
–37.
0N
IPR
MN
11(
1)A
-880
622
H4
59.4
8B
17.6
15.4
NIP
R M
N 1
1(1)
A-8
8062
3H
512
.65
B18
.916
.4N
IPR
MN
11(
1)A
-880
624
H3
91.6
8A
/B4.
3–26
.84.
2–23
.0N
IPR
MN
11(
1)A
-880
625
L647
.26
A/B
24.7
20.5
NIP
R M
N 1
1(1)
A-8
8062
6H
623
.58
A/B
19.4
16.9
NIP
R M
N 1
1(1)
A-8
8062
7H
630
.60
B18
.115
.9N
IPR
MN
11(
1)A
-880
628
H4
10.6
2B
17.8
15.5
NIP
R M
N 1
1(1)
A-8
8063
0H
311
.72
A/B
16.6
–27.
014
.6–2
6.3
NIP
R M
N 1
1(1)
A-8
8063
2LL
616
.61
B30
.024
.8N
IPR
MN
11(
1)A
-880
633
H4
553.
61B
/C18
.115
.7N
IPR
MN
11(
1)A
-880
634
H5
41.2
4B
/C18
.716
.4N
IPR
MN
11(
1)A
-880
635
H5
14.7
4B
/C18
.015
.7N
IPR
MN
11(
1)A
-880
636
H4
149.
15B
/C18
.516
.1N
IPR
MN
11(
1)A
-880
637
H4
107.
84B
17.3
15.3
NIP
R M
N 1
1(1)
A-8
8063
8H
499
.31
B17
.415
.3N
IPR
MN
11(
1)A
-880
639
H4
88.6
8B
/C17
.215
.1N
IPR
MN
11(
1)A
-880
640
L67.
18A
/B24
.020
.1N
IPR
MN
11(
1)A
-880
641
H3
154.
23A
/B17
.5–2
2.5
2.7–
23.0
NIP
R M
N 1
1(1)
A-8
8064
2H
436
.49
B/C
18.4
16.0
NIP
R M
N 1
1(1)
A-8
8064
4H
499
.38
B17
.415
.3N
IPR
MN
11(
1)A
-880
645
H4
40.1
0B
17.5
15.1
NIP
R M
N 1
1(1)
A-8
8064
7H
453
.13
B17
.415
.3N
IPR
MN
11(
1)A
-880
648
H4
41.0
1B
/C17
.315
.2N
IPR
MN
11(
1)
App
endi
x 2.
Rec
ently
des
crib
ed m
eteo
rites
from
Jap
anes
e N
IPR
exp
editi
ons.
Continued.
Nam
eC
lass
Mas
s (g
)W
eath
FaFs
Ref
A-8
8064
9H
465
.98
B/C
17.3
15.5
NIP
R M
N 1
1(1)
A-8
8065
2D
io29
.35
B–
22.9
–26.
4N
IPR
MN
11(
1)A
-880
653
H4
16.7
9B
/C18
.516
.4N
IPR
MN
11(
1)A
-880
654
H4
21.1
6B
/C18
.516
.4N
IPR
MN
11(
1)A
-880
655
H4
30.2
0B
/C18
.416
.7N
IPR
MN
11(
1)A
-880
656
H4
133.
17B
/C17
.415
.5N
IPR
MN
11(
1)A
-880
658
H4
34.5
6B
18.0
15.9
NIP
R M
N 1
1(1)
A-8
8065
9L6
83.4
2A
/B24
.720
.6N
IPR
MN
11(
1)A
-880
660
L611
.50
B24
.120
.2N
IPR
MN
11(
1)A
-880
661
H4
128.
91B
/C17
.215
.4N
IPR
MN
11(
1)A
-880
662
H5
27.6
4C
17.9
15.7
NIP
R M
N 1
1(1)
A-8
8066
3LL
620
.35
B29
.323
.6N
IPR
MN
11(
1)A
-880
664
H6
18.9
6B
/C18
.516
.0N
IPR
MN
11(
1)A
-880
665
H5
33.7
7B
/C18
.316
.0N
IPR
MN
11(
1)A
-880
666
L417
.84
A/B
25.1
20.6
NIP
R M
N 1
1(1)
A-8
8066
7L6
38.3
2A
/B25
.020
.5N
IPR
MN
11(
1)A
-880
668
H4
14.1
0B
17.5
15.4
NIP
R M
N 1
1(1)
A-8
8066
9L6
20.4
2A
/B24
.720
.4N
IPR
MN
11(
1)A
-880
671
LL4
20.3
5A
/B27
.622
.4N
IPR
MN
11(
1)A
-880
672
H4
19.9
2B
/C18
.416
.4N
IPR
MN
11(
1)A
-880
673
H6
18.0
0B
/C18
.416
.5N
IPR
MN
11(
1)A
-880
674
H5
18.9
0B
/C18
.816
.2N
IPR
MN
11(
1)A
-880
675
H4
385.
28A
/B16
.914
.9N
IPR
MN
11(
1)A
-880
676
H3
112.
96B
1.1–
26.4
2.4–
29.3
NIP
R M
N 1
1(1)
A-8
8067
9H
438
.77
B18
.515
.9N
IPR
MN
11(
1)A
-880
684
H3
60.2
6A
/B11
.5–2
0.9
6.1–
17.5
NIP
R M
N 1
1(1)
A-8
8068
5H
542
.37
B/C
17.8
15.7
NIP
R M
N 1
1(1)
A-8
8068
6H
522
.50
B17
.915
.5N
IPR
MN
11(
1)A
-880
688
L619
.55
A/B
24.6
20.4
NIP
R M
N 1
1(1)
A-8
8069
1C
K4
28.7
7A
/B30
.125
.9N
IPR
MN
11(
1)A
-880
693
H5
36.6
3B
18.8
16.5
NIP
R M
N 1
1(1)
A-8
8069
4H
410
.36
B18
.315
.9N
IPR
MN
11(
1)A
-880
695
H3
138.
69B
15.8
–20.
516
.3N
IPR
MN
11(
1)A
-880
698
H3
12.9
6A
/B17
.7–2
3.3
6.8–
20.7
NIP
R M
N 1
1(1)
A-8
8070
0H
432
7.50
A/B
18.3
16.0
NIP
R M
N 1
1(1)
A-8
8070
1H
444
.30
A/B
18.1
15.9
NIP
R M
N 1
1(1)
A-8
8070
2Eu
c10
.51
A–
–N
IPR
MN
11(
1)A
-880
703
H5
11.8
7B
18.4
16.0
NIP
R M
N 1
1(1)
A-8
8070
4H
551
.64
B/C
18.6
16.4
NIP
R M
N 1
1(1)
A-8
8070
8L3
33.2
0A
22.5
–24.
313
.2–2
4.8
NIP
R M
N 1
1(1)
A-8
8070
9H
315
.22
A16
.6–2
0.2
4.2–
23.2
NIP
R M
N 1
1(1)
A-8
8071
0H
314
.66
A/B
17.1
–22.
72.
0–21
.0N
IPR
MN
11(
1)A
-880
711
H4
59.5
8A
/B19
.015
.6N
IPR
MN
11(
1)A
-880
712
L611
1.85
A/B
24.4
20.3
NIP
R M
N 1
1(1)
A-8
8071
3H
316
.24
B16
.6–1
7.7
9.0–
19.7
NIP
R M
N 1
1(1)
A-8
8071
5H
519
09.2
5A
/B18
.416
.0N
IPR
MN
11(
1)A
-880
717
H6
41.4
1B
/C18
.616
.2N
IPR
MN
11(
1)
A248 S. S. Russell et al.
App
endi
x 2.
Rec
ently
des
crib
ed m
eteo
rites
from
Jap
anes
e N
IPR
exp
editi
ons.
Continued.
Nam
eC
lass
Mas
s (g
)W
eath
FaFs
Ref
A-8
8071
8C
K5
30.1
8A
/B29
.6–
NIP
R M
N 1
1(1)
A-8
8072
0H
544
.29
B/C
18.5
16.1
NIP
R M
N 1
1(1)
A-8
8072
1H
511
3.20
B/C
18.7
15.9
NIP
R M
N 1
1(1)
A-8
8072
3H
516
.57
B/C
18.6
16.2
NIP
R M
N 1
1(1)
A-8
8072
4H
378
.24
A/B
1.9–
22.9
7.3–
18.1
NIP
R M
N 1
1(1)
A-8
8072
5H
648
.72
A/B
18.6
15.3
NIP
R M
N 1
1(1)
A-8
8072
7L6
11.0
5A
/B24
.120
.4N
IPR
MN
11(
1)A
-880
728
H4
13.0
1A
18.2
15.7
NIP
R M
N 1
1(1)
A-8
8072
9H
323
9.61
A/B
17.6
–23.
212
.4–1
8.6
NIP
R M
N 1
1(1)
A-8
8073
0H
424
.09
B/C
17.7
15.7
NIP
R M
N 1
1(1)
A-8
8073
1H
610
.06
A18
.516
.1N
IPR
MN
11(
1)A
-880
732
L613
.89
A/B
24.1
20.0
NIP
R M
N 1
1(1)
A-8
8073
3H
416
.72
B/C
18.7
16.5
NIP
R M
N 1
1(1)
A-8
8073
4H
444
.19
B/C
18.5
15.8
NIP
R M
N 1
1(1)
A-8
8073
5H
444
2.46
B/C
18.3
15.6
NIP
R M
N 1
1(1)
A-8
8073
6LL
616
.85
A30
.123
.8N
IPR
MN
11(
1)A
-880
737
H4
47.1
4B
/C17
.915
.6N
IPR
MN
11(
1)A
-880
738
L640
.75
A/B
24.4
20.3
NIP
R M
N 1
1(1)
A-8
8074
0H
422
.10
A/B
18.3
16.0
NIP
R M
N 1
1(1)
A-8
8074
1H
529
.83
C18
.015
.8N
IPR
MN
11(
1)A
-880
742
H4
37.1
4B
/C18
.215
.9N
IPR
MN
11(
1)A
-880
743
H5
37.2
6B
/C18
.716
.5N
IPR
MN
11(
1)A
-880
744
H4
154.
38B
/C–
–N
IPR
MN
11(
1)A
-880
745
H3
74.1
0A
9.9–
22.9
2.5–
19.7
NIP
R M
N 1
1(1)
A-8
8074
6H
323
9.71
A/B
16.3
–20.
09.
5–24
.3N
IPR
MN
11(
1)A
-880
747
LL6
246.
41A
/B29
.524
.0N
IPR
MN
11(
1)A
-880
748
H6
23.4
9A
/B19
.016
.4N
IPR
MN
11(
1)A
-880
749
H6
16.6
5A
/B19
.016
.8N
IPR
MN
11(
1)A
-880
752
H6
72.0
1B
/C18
.616
.2N
IPR
MN
11(
1)A
-880
753
L436
.29
A/B
25.7
21.3
NIP
R M
N 1
1(1)
A-8
8075
4H
510
.35
A/B
18.0
15.9
NIP
R M
N 1
1(1)
A-8
8075
5H
411
.90
B17
.115
.1N
IPR
MN
11(
1)A
-880
756
H5
62.3
7B
/C18
.215
.9N
IPR
MN
11(
1)A
-880
757
H4
90.2
8A
/B18
.015
.8N
IPR
MN
11(
1)A
-880
758
H5
80.8
5B
18.9
16.0
NIP
R M
N 1
1(1)
A-8
8075
9H
569
.42
B18
.516
.2N
IPR
MN
11(
1)A
-880
760
H5
68.4
2B
/C18
.416
.2N
IPR
MN
11(
1)A
-880
761
Euc
65.4
4A
––
NIP
R M
N 1
1(1)
App
endi
x 2.
Rec
ently
des
crib
ed m
eteo
rites
from
Jap
anes
e N
IPR
exp
editi
ons.
Continued.
Nam
eC
lass
Mas
s (g
)W
eath
FaFs
Ref
A-8
8076
2H
415
5.30
B/C
17.7
15.6
NIP
R M
N 1
1(1)
A-8
8076
3H
554
.73
B/C
18.5
15.6
NIP
R M
N 1
1(1)
A-8
8076
4H
438
.36
B17
.815
.8N
IPR
MN
11(
1)A
-880
765
H4
60.0
9B
/C17
.915
.7N
IPR
MN
11(
1)A
-880
766
H4
25.2
4B
/C17
.215
.1N
IPR
MN
11(
1)A
-880
767
H4
44.0
1A
17.8
15.5
NIP
R M
N 1
1(1)
A-8
8076
8H
544
.62
B/C
20.1
16.6
NIP
R M
N 1
1(1)
A-8
8076
9L6
47.6
8A
/B24
.420
.4N
IPR
MN
11(
1)A
-880
770
H6
1166
.03
B19
.016
.4N
IPR
MN
11(
1)A
-880
771
H6
35.3
1C
18.7
16.2
NIP
R M
N 1
1(1)
A-8
8077
2L6
69.5
7A
24.1
20.2
NIP
R M
N 1
1(1)
A-8
8077
3H
555
.16
A/B
18.6
16.2
NIP
R M
N 1
1(1)
A-8
8077
4L3
12.2
1A
22.6
–25.
97.
8–22
.4N
IPR
MN
11(
1)A
-880
775
LL6
30.7
6A
/B31
.225
.6N
IPR
MN
11(
1)A
-880
776
H5
153.
78B
/C17
.515
.5N
IPR
MN
11(
1)A
-880
777
H5
105.
15B
/C18
.415
.9N
IPR
MN
11(
1)A
-880
778
H5
53.4
0B
18.5
16.0
NIP
R M
N 1
1(1)
A-8
8077
9H
592
.48
B18
.616
.8N
IPR
MN
11(
1)A
-880
780
LL5
85.5
5A
29.2
23.9
NIP
R M
N 1
1(1)
A-8
8078
1H
481
.85
C17
.815
.5N
IPR
MN
11(
1)A
-880
782
H4
58.2
8B
18.4
16.0
NIP
R M
N 1
1(1)
A-8
8078
4U
re44
.22
A–
–N
IPR
MN
11(
1)A
-880
785
Dio
82.7
2A
–23
.4–.
3N
IPR
MN
11(
1)A
-880
786
H4
47.0
5B
18.2
15.8
NIP
R M
N 1
1(1)
A-8
8078
8H
522
0.13
A/B
17.8
16.5
NIP
R M
N 1
1(1)
A-8
8078
9H
461
.55
B18
.516
.0N
IPR
MN
11(
1)A
-880
790
H4
40.6
0B
18.4
16.1
NIP
R M
N 1
1(1)
A-8
8079
1H
427
.02
B/C
18.3
16.1
NIP
R M
N 1
1(1)
A-8
8079
2H
628
.75
A/B
18.7
16.5
NIP
R M
N 1
1(1)
A-8
8079
3H
367
.01
B15
.2–.
78.
8–22
.2N
IPR
MN
11(
1)A
-880
794
H4
27.9
7B
18.5
16.2
NIP
R M
N 1
1(1)
A-8
8079
5LL
427
.91
A28
.722
.7N
IPR
MN
11(
1)A
-880
796
H5
43.1
4B
/C17
.815
.6N
IPR
MN
11(
1)A
-880
797
H5
43.2
9B
18.1
16.2
NIP
R M
N 1
1(1)
A-8
8079
8H
425
.59
B17
.915
.7N
IPR
MN
11(
1)A
-880
799
H4
21.8
5B
/C18
.315
.8N
IPR
MN
11(
1)A
-880
800
H4
51.5
2B
18.6
15.9
NIP
R M
N 1
1(1)
Y-98
0459
SNC
82.4
6A
15.8
–25.
916
.8–2
6.7
NIP
R M
N 1
1(1)