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Rationale for Landing Sites at Lunar Pyroclastic Deposits · 1/11/2018  · Localized Pyroclastic...

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25 km Rationale for Landing Sites at Lunar Pyroclastic Deposits Lisa Gaddis USGS Astrogeology Science Center Jan 11, 2018 Lunar Science for Landed Missions Workshop Alphonsus crater with 11 pyroclastic vents
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Page 1: Rationale for Landing Sites at Lunar Pyroclastic Deposits · 1/11/2018  · Localized Pyroclastic Deposits Formed by Vulcanian -style eruption Intermittent, violent explosion caused

25km

RationaleforLandingSitesatLunarPyroclastic

Deposits

Lisa GaddisUSGS Astrogeology Science Center

Jan 11, 2018Lunar Science for Landed Missions Workshop

Alphonsuscraterwith11pyroclasticvents

Page 2: Rationale for Landing Sites at Lunar Pyroclastic Deposits · 1/11/2018  · Localized Pyroclastic Deposits Formed by Vulcanian -style eruption Intermittent, violent explosion caused

Outline

� Overviewofthelunarpyroclasticdeposits

� Resourcepotential

� ISRU,AccessibilityandTraversability

� Recommendationsforlunarlandingsites

1.11.18 2LUNARSCIENCEFORLANDEDMISSIONSWORKSHOP

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LunarPyroclasticDeposits

Explosivelyemplacedvolcanicdeposits◦ Diffuseboundaries, associationwithvents

Ancient,byassociationwithlunarmaria◦ Mostbasaltseruptedduring theLateImbrian (3.6to3.8BYago)

◦ Hiesinger etal.(2000)cratercounts

Globallydistributed◦ Observedalongmarginsoflunarmaria

◦ Oftenassociatedwithfloor-fractured cratersinfaultedregions

Rangeofsizes(~50,000to3km2):

◦ VeryLarge=50000– 1000(22)

◦ Large=<1000– 400(19)

◦ Medium=<400– 200(12)

◦ Small=<200– 100(18)

◦ VerySmall=<100– 3(16)

31.11.18

87 Gustafson,etal.,2012

}Gaddisetal.,2003

LUNARSCIENCEFORLANDEDMISSIONSWORKSHOP

Alphonsus NE floor ventsKaguya MI color, 20 m/pixel, ~24 km across

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RegionalPyroclasticDeposits� Formedbyfire-fountaining(Head&Wilson,2017)

� Highvolatilecontent(H,H2O,CO,SO2),ballistic

trajectories

� Widelydistributed, ~thindeposits

� Abundantjuvenilematerial� Quenchedglass,crystallinebeads(oftenHiTiO2)

� TypeExamples� TaurusLittrow(Apollo 17)

� RimaBode,SinusAestuum,Sulpicius Gallus

1.11.18 4

Rima Bode Regional Pyroclastic Deposit (~6600 km2)Lunar Orbiter IV 109, ~120 km across

Ap 17 glass &crystalline beads

(G. Ryder)Bennettetal.,2016

LUNARSCIENCEFORLANDEDMISSIONSWORKSHOP

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LocalizedPyroclasticDeposits� FormedbyVulcanian-styleeruption

� Intermittent,violentexplosioncausedbydegassing

nearsurface,disruption ofaplugasmagmarisesin

adike(Head&Wilson,1979)� Volatile:CO-richgasproducedbygraphite

oxidation(Fogel &Rutherford,1995)� Mixedjuvenileandnon-juvenilematerials

� Glass,crystallinebasaltic (HiFeO),fragmentedcountryrock

� TypeExample� Alphonsuscrater� Oppenheimer crater

1.11.18 5

Alphonsus crater,FloorVent#6

KaguyaTerrainCamera

Bennettetal.,2016

LUNARSCIENCEFORLANDEDMISSIONSWORKSHOP

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GloballyDistributed

1.11.18 6LUNARSCIENCEFORLANDEDMISSIONSWORKSHOP

Pyroclasticdeposits (Gaddis etal.,2003;Gustafsonetal.,2012)

Floor-fracturedcraters(Jozwiak etal.,2015)

Fractures/faults(Wilhelms, 1987)

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ResourcePotential

1.11.18 7LUNARSCIENCEFORLANDEDMISSIONSWORKSHOP

• Relativelyunprocessedmaterialsfromdeepwithin the

lunarmantle(~300to400kmdepths)

◦ HighMg/Al,MgO,mg#;lowerAl2O3 andCaO thanmarebasalts

• Interiorcrystalsofolivine, spinel, ilmeniteneedles,etc.

• Uniformgrainsize,~40microns

• Surficialgeochemicalenrichments in>25volatileelements

• e.g.,Au,Ag,Cu,Cd,F,S,Z(McCubbin etal.,2015)

• Contain FeO:16to24wt %

• VariableamountsofTiO2,relatedtocolor

◦ Green:<1to5wt%◦ Yellow:5to9wt %

◦ Orange:9to14wt %◦ Red-black:>14wt%

• 25varieties ofvolcanicglassdescribedbyDelano(1986),severalothersidentifiedsince

Comprisedof‘primitive’glassandquenchedspheres

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ResourcePotential#2

1.11.18 8LUNARSCIENCEFORLANDEDMISSIONSWORKSHOP

IndigenousMagmaticWater

• TheMoonisgenerallyvolatile-depleted

•BUT,recentsampleanalysesofmeltinclusionsin

glasssamplesfromAp15,Ap17foundevidencefor

waterandothermagmaticvolatilespecies

• ~30to36ppmofmagmaticwaterinAp 15glass

beads(Saal etal.,2008)

• Correlationswithothermagmaticelements(Chlorine,

Fluoride, Sulfur)

• Concentrationofvolatilesdecreasedtowardedges,

indicatingtheywerenotcontaminantsfromEarth

• 270-1200ppmH2OinolivinecrystalsfromAp17

(Hauri etal.,2011)

• Fromaprimarylunarmagma

• Sourcewaterabundances of80-440ppm,comparableto

MORBs

• SummarizedbyMcCubbin etal.,2015;Hauri eal.,

2017

Apollo 15 green glass beads about 0.1 mm across

(Ap 15 S79-32188)

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ResourcePotential#3

1.11.18 9LUNARSCIENCEFORLANDEDMISSIONSWORKSHOP

MappingofLunarWater• UseofMoonMineralogyMapper(M3)data,quantitativeanalysisofstrengthofthe2.85-micronband

(ESPAT),mappingofOH- and/orH2O-bearingminerals

• Waterabundancesupto150ppmatlargepyroclasticdeposits,300to400ppmnearvents

ESPAT=effective

singleparticle

absorption

thickness

Milliken&Li,2017

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ResourcePotential#4

1.11.18 10LUNARSCIENCEFORLANDEDMISSIONSWORKSHOP

ExogenousVolatiles• Solar-wind implantedvolatiles(e.g.,H,3He)inmature,Hi-Ti lunarregolith

• Evenlydistributed intop2-3m,requiresheating (300°-900° C)torelease(Fegley &Swindle,

1993)

Fa&Jin,2007

Estimatedconcentrationof3He(ppbbymass) inthelunarregolith

Nearside FarsideCrawford,2015

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In-SituResourceUtilization

1.11.18 11LUNARSCIENCEFORLANDEDMISSIONSWORKSHOP

• Useofin-situlunarresourcescanreducecostsofsurfaceoperations

• H2O~oxygen,drinkingwaterforlifesupport

• H~rocketfuel,reducingagent

• C,N,Scouldsupport lunaragriculture

• PyroclasticdepositsarerichinFeO &TiO2

◦ Extractionofoxygen(>20methodstochoosefrom;Taylor&Carrier,1992)

◦ Reductionofilmeniteispopular;requiresH,energy

• Surveymoderequiresmobility,accessibility,traversability

• Supports horizontalassessmentoffeedstock,estimatesofthicknessandverticaldistributionfromventoutward,determinationofconsistencyofmaterials

• Samplereturnprovidesmoreprecisedeterminationsofcomposition, calibrationforremotemapping

• Ilmenitecontent

• Presenceofolivine

• Indigenouswater

• Surface-correlatedandsolar-wind-implantedvolatiles

FromLarryTaylor

3-DPrintedMoonBase(ESA)

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LunarLandingSites

1.11.18 12LUNARSCIENCEFORLANDEDMISSIONSWORKSHOP

• SKGstobeaddressedatlunarpyroclasticdeposits◦ Understandingplanetaryvolcanicprocesses

◦ UnderstandingtheMoon’sresourcepotential

◦ Understandingthenature&distributionoflunarvolatiles

• Sciencequestions(examples)

• Howoldarethelunarpyroclasticdeposits?

• Aresomeeruptionstylesmorelikelytobeassociatedwith

depositswith indigenouswater?

• Whichdepositscontainolivinethatcanbetiedtodeeplunar

interiororigin?

• Howthick/uniformarethedeposits?Doesthicknessvary?

Howmuchmaterialispresent?

• Whatsites?

• “Blackspot”locations,highiron,titanium,H,H2O,surface-

correlatedvolatiles,water

• Taurus-Littrow,Sulpicius Gallus,RimaBode,Vaporum, etc.

• Humorum

• Aristarchusplateau(Jawinetal.,thissession)

3DSinusAestuum,RimaBode(Kaguya MIdrapedonSLDEM15)

ESPAT(Milliken&Li,2017)

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LunarLandingSites

1.11.18 13LUNARSCIENCEFORLANDEDMISSIONSWORKSHOP

Thanksforlistening!

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LunarLandingSites

1.11.18 14LUNARSCIENCEFORLANDEDMISSIONSWORKSHOP

•ExampleLandingSite:Humorum

• Regionalextent(1500km2),smooth-surfaced,Hi-FeO

• Precursorremotecharacterization

• Highspatialresolution(<100mpp),hyperspectral imagertomap~3

micronabsorptionband

• Characterizeabundance,distributionofmaficmineralsandindigenous

waterindetail

• UseLROCdata(~1mpp)fordepositthickness estimates, boulder&crater

hazards

• UseLOLAdatatodevelopslopemaps

• Rovermission(groundcontactatmultiplesites)

• AlphaParticleX-raySpectrometer: Bulkchemistry

• NeutronSpectrometer:Measurebulkhydrogen,watercontentat

multiplesites

• Pancam colorimager:

• Multispectralmapping(composition)survey

• Observeanychange(s)withtime

• Samplereturn

• Multiplesamplesofmaturesoil,quenchedglass,crystallizedbeads

• Analysisofmagmatic water(abundance,distribution,etc.)

• Ground-truthforremotemeasurements

• Feedstockassessment andviabilityforin-situextraction

Milliken&Li,2017


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