Exsolved kirschsteinite in angrite LEW86010 olivine
Mineralogy of kirschsteinite exsolution in olivine from Antarctic meteorite LEW86010 has been studied by single crustal X-ray diffraction technique. The LEW86010 olivine crystals have exsolution lamellae of kirschteinite about 15 microns wide. Determination of crystallographic orientation of exsolve...
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ftnasantrs:oai:casi.ntrs.nasa.gov:19940011937 2023-05-15T13:42:51+02:00 Exsolved kirschsteinite in angrite LEW86010 olivine Miyamoto, Masamichi Mckay, Gordon Takeda, Hiroshi Mikouchi, Takashi Mori, Hiroshi Unclassified, Unlimited, Publicly available JAN 1, 1993 application/pdf http://hdl.handle.net/2060/19940011937 unknown Document ID: 19940011937 Accession ID: 94N16410 http://hdl.handle.net/2060/19940011937 No Copyright CASI ASTROPHYSICS Lunar and Planetary Inst., Twenty-Fourth Lunar and Planetary Science Conference. Part 2: G-M; p 987-988 1993 ftnasantrs 2015-03-15T03:50:47Z Mineralogy of kirschsteinite exsolution in olivine from Antarctic meteorite LEW86010 has been studied by single crustal X-ray diffraction technique. The LEW86010 olivine crystals have exsolution lamellae of kirschteinite about 15 microns wide. Determination of crystallographic orientation of exsolved kirschsteinite in an olivine grain has been made. Weak reflections of exsolved kirschsteinite share common crystallographic orientation with the host olivine. The cell dimensions of the exsolved phase (a - 4.87 plus or minus 0.05A, b - 11.14 plus or minus 0.10A, c - 6.36 plus or minus 0.05A) and intensities were in well accord with those of kirschsteinite previously reported. Oriented section perpendicular to the a axis shows exsolution lamellae in two directions parallel to (031) and (031). The lamellae are up to 10 microns in width and spacings between them are usually 50-100 microns. 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 |
ASTROPHYSICS |
spellingShingle |
ASTROPHYSICS Miyamoto, Masamichi Mckay, Gordon Takeda, Hiroshi Mikouchi, Takashi Mori, Hiroshi Exsolved kirschsteinite in angrite LEW86010 olivine |
topic_facet |
ASTROPHYSICS |
description |
Mineralogy of kirschsteinite exsolution in olivine from Antarctic meteorite LEW86010 has been studied by single crustal X-ray diffraction technique. The LEW86010 olivine crystals have exsolution lamellae of kirschteinite about 15 microns wide. Determination of crystallographic orientation of exsolved kirschsteinite in an olivine grain has been made. Weak reflections of exsolved kirschsteinite share common crystallographic orientation with the host olivine. The cell dimensions of the exsolved phase (a - 4.87 plus or minus 0.05A, b - 11.14 plus or minus 0.10A, c - 6.36 plus or minus 0.05A) and intensities were in well accord with those of kirschsteinite previously reported. Oriented section perpendicular to the a axis shows exsolution lamellae in two directions parallel to (031) and (031). The lamellae are up to 10 microns in width and spacings between them are usually 50-100 microns. |
format |
Other/Unknown Material |
author |
Miyamoto, Masamichi Mckay, Gordon Takeda, Hiroshi Mikouchi, Takashi Mori, Hiroshi |
author_facet |
Miyamoto, Masamichi Mckay, Gordon Takeda, Hiroshi Mikouchi, Takashi Mori, Hiroshi |
author_sort |
Miyamoto, Masamichi |
title |
Exsolved kirschsteinite in angrite LEW86010 olivine |
title_short |
Exsolved kirschsteinite in angrite LEW86010 olivine |
title_full |
Exsolved kirschsteinite in angrite LEW86010 olivine |
title_fullStr |
Exsolved kirschsteinite in angrite LEW86010 olivine |
title_full_unstemmed |
Exsolved kirschsteinite in angrite LEW86010 olivine |
title_sort |
exsolved kirschsteinite in angrite lew86010 olivine |
publishDate |
1993 |
url |
http://hdl.handle.net/2060/19940011937 |
op_coverage |
Unclassified, Unlimited, Publicly available |
geographic |
Antarctic |
geographic_facet |
Antarctic |
genre |
Antarc* Antarctic |
genre_facet |
Antarc* Antarctic |
op_source |
CASI |
op_relation |
Document ID: 19940011937 Accession ID: 94N16410 http://hdl.handle.net/2060/19940011937 |
op_rights |
No Copyright |
_version_ |
1766173646564360192 |