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The source of sublimates on the Apollo 15 green and Apollo 17 orange glass samplesElemental analyses of the thin film of micromounds which coat the surfaces of Apollo 15 green glass and Apollo 17 orange glass are reported. It is thought that Zn, Ga, Pb, Cu, Tl, S, F, and Cl condensed as a sublimate on the outside surface of these glass particles in lava fountains about 3.4 and 3.6 b.y. ago (Apollos 15 and 17, respectively). The heavy metals enriched in these samples may have been mobilized in a halide- and sulfide-rich vapor, while the source of these elements and of the glass may be a sulfide- and halide-rich pyroxenite inside the moon. The isotopic composition of lead on the surface of individual particles was determined, and the composition is considered with respect to the evolution of the source region. The lead on the surfaces is similar to lead that has been mixed into other soils and breccias at nearby sites.
Document ID
19780062787
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Meyer, C., Jr.
(NASA Lyndon B. Johnson Space Center Houston, TX, United States)
Mckay, D. S.
(NASA Lyndon B. Johnson Space Center Houston, TX, United States)
Anderson, D. H.
(NASA Lyndon B. Johnson Space Center Houston, TX, United States)
Butler, P., Jr.
(NASA Johnson Space Center Houston, Tex., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1975
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: March 17, 1975
End Date: March 21, 1975
Accession Number
78A46696
Distribution Limits
Public
Copyright
Other

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