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Single agglutinates: A comparative study of compositions of agglutinitic glass, whole-grain, bulk soil, and FMRPrevious workers on single agglutinates have variously interpreted the composition of agglutinitic glass to represent impact melts of (1) bulk soil, (2) mixed components in finer sizes, and (3) microtargets. Separately, Papike has argued in favor of fusion of the finest fraction of bulk soils. Thirty-four single agglutinates were hand-picked from the mature Apollo 16 soil 61181 (I(sub s)/FeO = 82) and the FMR and chemical composition (INAA for Fe, Sc, Sm, Co, Ni, and Cr) of each agglutinate particle were measured. Thirteen of these single agglutinates were selected for electron beam microanalysis and imaging. Less than 1 micron spots were analyzed (for Na, Mg, Al, Si, P, S, K, Ca, Ti, Cr, Mn, Fe, Ni, and Ba) on pure glassy areas (approximately ten in each particle) selected on the basis of optical and BSE images (avoiding all clasts and inclusions) with an electron microprobe to obtain average glass compositions of each single agglutinate.
Document ID
19940030895
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Basu, A.
(Indiana Univ. Bloomington, IN., United States)
Robinson, R.
(Indiana Univ. Bloomington, IN., United States)
Mckay, D. S.
(NASA Lyndon B. Johnson Space Center Houston, TX, United States)
Blanchard, D. P.
(NASA Lyndon B. Johnson Space Center Houston, TX, United States)
Morris, R. V.
(NASA Lyndon B. Johnson Space Center Houston, TX, United States)
Wentworth, Susan J.
(NASA Lyndon B. Johnson Space Center Houston, TX, United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1994
Publication Information
Publication: Lunar and Planetary Inst., The Twenty-Fifth Lunar and Planetary Science Conference. Part 1: A-G
Subject Category
Lunar And Planetary Exploration
Accession Number
94N35401
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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