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Analysis of Lunar Highland Regolith Samples from Apollo 16 Drive Core 64001/2 and Lunar Regolith Simulants - An Expanding Comparative DatabaseWe present modal data from QEMSCAN(registered TradeMark) beam analysis of Apollo 16 samples from drive core 64001/2. The analyzed lunar samples are thin sections 64002,6019 (5.0-8.0 cm depth) and 64001,6031 (50.0-53.1 cm depth) and sieved grain mounts 64002,262 and 64001,374 from depths corresponding to the thin sections, respectively. We also analyzed lunar highland regolith simulants NU-LHT-1M, -2M, and OB-1, low-Ti mare simulants JSC-1, -lA, -1AF, and FJS-1, and high-Ti mare simulant MLS-1. The preliminary results comprise the beginning of an internally consistent database of lunar regolith and regolith simulant mineral and glass information. This database, combined with previous and concurrent studies on phase chemistry, bulk chemistry, and with data on particle shape and size distribution, will serve to guide lunar scientists and engineers in choosing simulants for their applications. These results are modal% by phase rather than by particle type, so they are not directly comparable to most previously published lunar data that report lithic fragments, monomineralic particles, agglutinates, etc. Of the highland simulants, 08-1 has an integrated modal composition closer than NU-LHT-1M to that of the 64001/2 samples, However, this and other studies show that NU-LHT-1M and -2M have minor and trace mineral (e.g., Fe-Ti oxides and phosphates) populations and mineral and glass chemistry closer to these lunar samples. The finest fractions (0-20 microns) in the sieved lunar samples are enriched in glass relative to the integrated compositions by approx.30% for 64002,262 and approx.15% for 64001,374. Plagioclase, pyroxene, and olivine are depleted in these finest fractions. This could be important to lunar dust mitigation efforts and astronaut health - none of the analyzed simulants show this trend. Contrary to previously reported modal analyses of monomineralic grains in lunar regolith, these area% modal analyses do not show a systematic increase in plagiociase/pyroxene as size fraction decreases.
Document ID
20090014122
Acquisition Source
Marshall Space Flight Center
Document Type
Conference Paper
Authors
Schrader, Christian M.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Rickman, Doug
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Stoeser, Doug
(Geological Society of America New York, NY, United States)
Wentworth, Susan J.
(NASA Johnson Space Center Houston, TX, United States)
Botha, Pieter WSK
(Intellection Corp. Westminster, CO, United States)
Butcher, Alan R.
(Intellction pty Ltd Queensland, Australia)
McKay, David
(NASA Johnson Space Center Houston, TX, United States)
Horsch, Hanna
(Intellction pty Ltd Queensland, Australia)
Benedictus, Aukje
(Intellction pty Ltd Queensland, Australia)
Gottlieb, Paul
(Intellction pty Ltd Queensland, Australia)
Date Acquired
August 24, 2013
Publication Date
October 5, 2008
Subject Category
Geophysics
Report/Patent Number
MSFC-2144
Meeting Information
Meeting: Joint Meeting of the Geological Society of America and the Soil Science Society of America/Geological Society of America (GSA)
Location: Orlando, FL
Country: United States
Start Date: October 5, 2008
End Date: October 9, 2008
Distribution Limits
Public
Copyright
Other

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