Trapped noble gases indicate lunar origin for Antarctic meteorite
The isotopic abundances of the noble gases (He, Ne, Ar, Kr, Xe) are reported for Antarctic ALHA 81005. It contains solar wind-implanted gases whose absolute and relative concentrations are quite similar to lunar regolith samples but not to other meteorites. ALHA 81005 also contains a large excess Ar...
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ftnasantrs:oai:casi.ntrs.nasa.gov:19830065649 2023-05-15T13:35:32+02:00 Trapped noble gases indicate lunar origin for Antarctic meteorite Bogard, D. D. Johnson, P. Unclassified, Unlimited, Publicly available Sep 1, 1983 http://ntrs.nasa.gov/search.jsp?R=19830065649 unknown http://ntrs.nasa.gov/search.jsp?R=19830065649 Accession ID: 83A46867 Copyright Other Sources 91 Geophysical Research Letters; 10; Sept 1983 ftnasantrs 2012-02-15T15:32:57Z The isotopic abundances of the noble gases (He, Ne, Ar, Kr, Xe) are reported for Antarctic ALHA 81005. It contains solar wind-implanted gases whose absolute and relative concentrations are quite similar to lunar regolith samples but not to other meteorites. ALHA 81005 also contains a large excess Ar-40 component which is identical to the component in lunar fines implanted from the lunar atmosphere. Large concentrations of cosmogenic Ne-21, Kr-82, and Xe-126 in ALHA 81005 indicate a total cosmic ray exposure age of at least 200 million years. The noble gas data alone are strong evidence for a lunar origin of this meteorite. Other/Unknown Material Antarc* Antarctic NASA Technical Reports Server (NTRS) Antarctic |
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Open Polar |
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NASA Technical Reports Server (NTRS) |
op_collection_id |
ftnasantrs |
language |
unknown |
topic |
91 |
spellingShingle |
91 Bogard, D. D. Johnson, P. Trapped noble gases indicate lunar origin for Antarctic meteorite |
topic_facet |
91 |
description |
The isotopic abundances of the noble gases (He, Ne, Ar, Kr, Xe) are reported for Antarctic ALHA 81005. It contains solar wind-implanted gases whose absolute and relative concentrations are quite similar to lunar regolith samples but not to other meteorites. ALHA 81005 also contains a large excess Ar-40 component which is identical to the component in lunar fines implanted from the lunar atmosphere. Large concentrations of cosmogenic Ne-21, Kr-82, and Xe-126 in ALHA 81005 indicate a total cosmic ray exposure age of at least 200 million years. The noble gas data alone are strong evidence for a lunar origin of this meteorite. |
format |
Other/Unknown Material |
author |
Bogard, D. D. Johnson, P. |
author_facet |
Bogard, D. D. Johnson, P. |
author_sort |
Bogard, D. D. |
title |
Trapped noble gases indicate lunar origin for Antarctic meteorite |
title_short |
Trapped noble gases indicate lunar origin for Antarctic meteorite |
title_full |
Trapped noble gases indicate lunar origin for Antarctic meteorite |
title_fullStr |
Trapped noble gases indicate lunar origin for Antarctic meteorite |
title_full_unstemmed |
Trapped noble gases indicate lunar origin for Antarctic meteorite |
title_sort |
trapped noble gases indicate lunar origin for antarctic meteorite |
publishDate |
1983 |
url |
http://ntrs.nasa.gov/search.jsp?R=19830065649 |
op_coverage |
Unclassified, Unlimited, Publicly available |
geographic |
Antarctic |
geographic_facet |
Antarctic |
genre |
Antarc* Antarctic |
genre_facet |
Antarc* Antarctic |
op_source |
Other Sources |
op_relation |
http://ntrs.nasa.gov/search.jsp?R=19830065649 Accession ID: 83A46867 |
op_rights |
Copyright |
_version_ |
1766066913277902848 |