Geochemistry and petrography of the MacAlpine Hills lunar meteorites
MacAlpine Hills 88104 and 88105, anorthositic lunar meteorites recovered form the same area in Antartica, are characterized. Petrographic studies show that MAC88104/5 is a polymict breccia dominated by impact melt clasts. It is better classified as a fragmental breccia than a regolith breccia. The b...
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1991
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ftnasantrs:oai:casi.ntrs.nasa.gov:19920032184 2023-05-15T14:15:47+02:00 Geochemistry and petrography of the MacAlpine Hills lunar meteorites Lindstrom, Marilyn M. Mckay, David S. Wentworth, Susan J. Martinez, Rene R. Mittlefehldt, David W. Wang, Ming-Sheng Lipschutz, Michael E. Unclassified, Unlimited, Publicly available Nov 1, 1991 http://ntrs.nasa.gov/search.jsp?R=19920032184 unknown http://ntrs.nasa.gov/search.jsp?R=19920032184 Accession ID: 92A14808 Copyright Other Sources 91 Geochimica et Cosmochimica Acta; 55; 3089-310 1991 ftnasantrs 2012-02-15T19:26:01Z MacAlpine Hills 88104 and 88105, anorthositic lunar meteorites recovered form the same area in Antartica, are characterized. Petrographic studies show that MAC88104/5 is a polymict breccia dominated by impact melt clasts. It is better classified as a fragmental breccia than a regolith breccia. The bulk composition is ferroan and highly aluminous (Al2O3-28 percent). Other/Unknown Material antartic* NASA Technical Reports Server (NTRS) MacAlpine Hills ENVELOPE(160.500,160.500,-84.217,-84.217) |
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Open Polar |
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NASA Technical Reports Server (NTRS) |
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ftnasantrs |
language |
unknown |
topic |
91 |
spellingShingle |
91 Lindstrom, Marilyn M. Mckay, David S. Wentworth, Susan J. Martinez, Rene R. Mittlefehldt, David W. Wang, Ming-Sheng Lipschutz, Michael E. Geochemistry and petrography of the MacAlpine Hills lunar meteorites |
topic_facet |
91 |
description |
MacAlpine Hills 88104 and 88105, anorthositic lunar meteorites recovered form the same area in Antartica, are characterized. Petrographic studies show that MAC88104/5 is a polymict breccia dominated by impact melt clasts. It is better classified as a fragmental breccia than a regolith breccia. The bulk composition is ferroan and highly aluminous (Al2O3-28 percent). |
format |
Other/Unknown Material |
author |
Lindstrom, Marilyn M. Mckay, David S. Wentworth, Susan J. Martinez, Rene R. Mittlefehldt, David W. Wang, Ming-Sheng Lipschutz, Michael E. |
author_facet |
Lindstrom, Marilyn M. Mckay, David S. Wentworth, Susan J. Martinez, Rene R. Mittlefehldt, David W. Wang, Ming-Sheng Lipschutz, Michael E. |
author_sort |
Lindstrom, Marilyn M. |
title |
Geochemistry and petrography of the MacAlpine Hills lunar meteorites |
title_short |
Geochemistry and petrography of the MacAlpine Hills lunar meteorites |
title_full |
Geochemistry and petrography of the MacAlpine Hills lunar meteorites |
title_fullStr |
Geochemistry and petrography of the MacAlpine Hills lunar meteorites |
title_full_unstemmed |
Geochemistry and petrography of the MacAlpine Hills lunar meteorites |
title_sort |
geochemistry and petrography of the macalpine hills lunar meteorites |
publishDate |
1991 |
url |
http://ntrs.nasa.gov/search.jsp?R=19920032184 |
op_coverage |
Unclassified, Unlimited, Publicly available |
long_lat |
ENVELOPE(160.500,160.500,-84.217,-84.217) |
geographic |
MacAlpine Hills |
geographic_facet |
MacAlpine Hills |
genre |
antartic* |
genre_facet |
antartic* |
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Other Sources |
op_relation |
http://ntrs.nasa.gov/search.jsp?R=19920032184 Accession ID: 92A14808 |
op_rights |
Copyright |
_version_ |
1766288077217595392 |