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Experimental studies of lunar exosphere O.I. Korablev 1, A.A. Petrukovich 1, E. Quémerais 2, V.I....

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Experimental studies of lunar exosphere O.I. Korablev 1 , A.A. Petrukovich 1 , E. Quémerais 2 , V.I. Gnedykh 1 , K.I. Marchenkov 1 1 Space research Institute (IKI), Moscow 2 LATMOS, Guyancourt, France
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Page 1: Experimental studies of lunar exosphere O.I. Korablev 1, A.A. Petrukovich 1, E. Quémerais 2, V.I. Gnedykh 1, K.I. Marchenkov 1 1 Space research Institute.

Experimental studies of lunar exosphere

O.I. Korablev1, A.A. Petrukovich1, E. Quémerais2, V.I. Gnedykh1, K.I. Marchenkov1

1 Space research Institute (IKI), Moscow2 LATMOS, Guyancourt, France

Page 2: Experimental studies of lunar exosphere O.I. Korablev 1, A.A. Petrukovich 1, E. Quémerais 2, V.I. Gnedykh 1, K.I. Marchenkov 1 1 Space research Institute.

Brief history• Pre-Apollo searches:

– Polarization measurements: Fessenkov, Dollfus 10-9-10 bar

– Radioccultations (Mariner 7) : <3 10-9 H; 8 10-10 He; 8 10-12 Ar

– Lunar Transient Phenomena

• Apollo– SIDE: Suprathermal ion detector: 20Ne and 40Ar

detections– Cathode gauges: N2 assumption: 2 107cm-3 day …

2 105cm-3 night– LACE mass spectrometer: Ar, He H2O, CH4, N2,CO,

CO2– α-particle spectrometers (A15): 222Rn, 210Po– Orbital mass spectrometers (A15-16)– UV spectrometer (A17)

• Ground-based discovery of K and Na [Potter & Morgan 1988]

Hodges 1985

Page 3: Experimental studies of lunar exosphere O.I. Korablev 1, A.A. Petrukovich 1, E. Quémerais 2, V.I. Gnedykh 1, K.I. Marchenkov 1 1 Space research Institute.

Sodium and Potassium

Potter & Morgan 1988

Images of the lunar sodium exosphere during total lunar eclipses Mendillo et al 1999

Page 4: Experimental studies of lunar exosphere O.I. Korablev 1, A.A. Petrukovich 1, E. Quémerais 2, V.I. Gnedykh 1, K.I. Marchenkov 1 1 Space research Institute.

Sodium and Potassium II

Page 5: Experimental studies of lunar exosphere O.I. Korablev 1, A.A. Petrukovich 1, E. Quémerais 2, V.I. Gnedykh 1, K.I. Marchenkov 1 1 Space research Institute.

Mechanisms

Stern 1999

Sprague et al1992

Page 6: Experimental studies of lunar exosphere O.I. Korablev 1, A.A. Petrukovich 1, E. Quémerais 2, V.I. Gnedykh 1, K.I. Marchenkov 1 1 Space research Institute.

Mechanisms

Lucey 2009

Page 7: Experimental studies of lunar exosphere O.I. Korablev 1, A.A. Petrukovich 1, E. Quémerais 2, V.I. Gnedykh 1, K.I. Marchenkov 1 1 Space research Institute.

Stern 1999

Page 8: Experimental studies of lunar exosphere O.I. Korablev 1, A.A. Petrukovich 1, E. Quémerais 2, V.I. Gnedykh 1, K.I. Marchenkov 1 1 Space research Institute.

Recent space observations

• SARA /Chandrayan-1: low energy neutral atom sensor 10 eV – 3.3 keV and ion mass spectrometer (10 eV – 15 keV)

• UPI-TVIS/SELENE: UV and visible (Na D2, OI) narrow-band imager

• LAMP/MRO

Page 9: Experimental studies of lunar exosphere O.I. Korablev 1, A.A. Petrukovich 1, E. Quémerais 2, V.I. Gnedykh 1, K.I. Marchenkov 1 1 Space research Institute.

UV-spectrometry from space

LRO/LAMP:-Spectral range 57–196 nm-Observation of the LCROSS plume-Mapping of lunar poles in L-alpha

LADEE mission: NASA 2012-UVS : 200–800 nm-NMS

Page 10: Experimental studies of lunar exosphere O.I. Korablev 1, A.A. Petrukovich 1, E. Quémerais 2, V.I. Gnedykh 1, K.I. Marchenkov 1 1 Space research Institute.

UV-spectrometry from Luna Globe Orbiter LEVUS: Lunar Exosphere EUV/UV

spectrometer

• On the basis of PHEBUS/Bepi Colombo• French PI of PHEBUS: Eric Quémerais, 2 co-PIs• Detectors from Japan (customized Hamamatsu design)• Scanner system from IKI/Russia• LEVUS = spare of PHEBUS provided by France with interfaces

and scanner modified by IKI. IKI provides all prototypes for Luna Globe.

Page 11: Experimental studies of lunar exosphere O.I. Korablev 1, A.A. Petrukovich 1, E. Quémerais 2, V.I. Gnedykh 1, K.I. Marchenkov 1 1 Space research Institute.

LEVUS : Science objectives

• To detect/reduce upper limits of expected components of the lunar exosphere

• To study the sources, sinks and transport mechanisms of exosphere species

• To explore the EUV range, not covered so far• To map the surface in the UV range• To study the solar wind and its interaction with the moon• UV observatory: comets,…• Terrestrial exosphere (geocorona)

Page 12: Experimental studies of lunar exosphere O.I. Korablev 1, A.A. Petrukovich 1, E. Quémerais 2, V.I. Gnedykh 1, K.I. Marchenkov 1 1 Space research Institute.

LEVUS:

• EUV channel: 55–155 nm• FUV channel: 145–315 nm• 2 PMTs: 404, 422 nm: K, Ca lines• Scanner 360°

Page 13: Experimental studies of lunar exosphere O.I. Korablev 1, A.A. Petrukovich 1, E. Quémerais 2, V.I. Gnedykh 1, K.I. Marchenkov 1 1 Space research Institute.

LEVUS optical scheme and detectors

Page 14: Experimental studies of lunar exosphere O.I. Korablev 1, A.A. Petrukovich 1, E. Quémerais 2, V.I. Gnedykh 1, K.I. Marchenkov 1 1 Space research Institute.

Detectability of exospheric components

Page 15: Experimental studies of lunar exosphere O.I. Korablev 1, A.A. Petrukovich 1, E. Quémerais 2, V.I. Gnedykh 1, K.I. Marchenkov 1 1 Space research Institute.

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