The natural thermoluminescence of Antarctic meteorites and their terrestrial ages and orbits: A 2010 update

Abstract– We have examined the relationship between natural thermoluminescence (TL) and 26 Al in 120 Antarctic meteorites in order to explore the orbital history and terrestrial ages of these meteorites. Our results confirm the observations of Hasan et al. (1987) which were based on 23 meteorites. F...

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Published in:Meteoritics & Planetary Science
Main Authors: SEARS, Derek W. G., YOZZO, Jordan, RAGLAND, Christina
Format: Article in Journal/Newspaper
Language:English
Published: Wiley 2011
Subjects:
Online Access:http://dx.doi.org/10.1111/j.1945-5100.2010.01139.x
https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1111%2Fj.1945-5100.2010.01139.x
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spelling crwiley:10.1111/j.1945-5100.2010.01139.x 2024-06-23T07:47:32+00:00 The natural thermoluminescence of Antarctic meteorites and their terrestrial ages and orbits: A 2010 update SEARS, Derek W. G. YOZZO, Jordan RAGLAND, Christina 2011 http://dx.doi.org/10.1111/j.1945-5100.2010.01139.x https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1111%2Fj.1945-5100.2010.01139.x https://onlinelibrary.wiley.com/doi/pdf/10.1111/j.1945-5100.2010.01139.x en eng Wiley http://onlinelibrary.wiley.com/termsAndConditions#vor Meteoritics & Planetary Science volume 46, issue 1, page 79-91 ISSN 1086-9379 1945-5100 journal-article 2011 crwiley https://doi.org/10.1111/j.1945-5100.2010.01139.x 2024-06-11T04:52:21Z Abstract– We have examined the relationship between natural thermoluminescence (TL) and 26 Al in 120 Antarctic meteorites in order to explore the orbital history and terrestrial ages of these meteorites. Our results confirm the observations of Hasan et al. (1987) which were based on 23 meteorites. For most meteorites there was a positive correlation between natural TL and 26 Al, reflecting their similarity in decay rate under Antarctic conditions and thus in terrestrial age. For a small group with low TL and high 26 Al a small perihelion was proposed. Within this group, natural TL decreases with terrestrial age as determined by 36 Cl measurements, although the rate of TL decay is faster (half‐life approximately 10 ka) and the ages that can be determined are smaller (<200 ka) than for most meteorites. The faster decay rate and lower natural TL levels are a reflection of recent exposure to higher radiation doses and higher temperatures, since this history would populate less stable TL traps with smaller electron densities. We sort the 120 meteorites by perihelion and terrestrial age. The normal perihelion group range up to approximately 1000 ka and the small perihelion group range up to approximately 200 ka. An intermediate perihelion group tends to have short terrestrial ages (20–60 ka). There is acceptable agreement between most (34 out of 43) of our present terrestrial age estimates and those determined by isotopic means, the exceptions reflecting complex irradiation histories, long burial times in the Antarctic, or other issues. Article in Journal/Newspaper Antarc* Antarctic Wiley Online Library Antarctic The Antarctic Meteoritics & Planetary Science no no
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language English
description Abstract– We have examined the relationship between natural thermoluminescence (TL) and 26 Al in 120 Antarctic meteorites in order to explore the orbital history and terrestrial ages of these meteorites. Our results confirm the observations of Hasan et al. (1987) which were based on 23 meteorites. For most meteorites there was a positive correlation between natural TL and 26 Al, reflecting their similarity in decay rate under Antarctic conditions and thus in terrestrial age. For a small group with low TL and high 26 Al a small perihelion was proposed. Within this group, natural TL decreases with terrestrial age as determined by 36 Cl measurements, although the rate of TL decay is faster (half‐life approximately 10 ka) and the ages that can be determined are smaller (<200 ka) than for most meteorites. The faster decay rate and lower natural TL levels are a reflection of recent exposure to higher radiation doses and higher temperatures, since this history would populate less stable TL traps with smaller electron densities. We sort the 120 meteorites by perihelion and terrestrial age. The normal perihelion group range up to approximately 1000 ka and the small perihelion group range up to approximately 200 ka. An intermediate perihelion group tends to have short terrestrial ages (20–60 ka). There is acceptable agreement between most (34 out of 43) of our present terrestrial age estimates and those determined by isotopic means, the exceptions reflecting complex irradiation histories, long burial times in the Antarctic, or other issues.
format Article in Journal/Newspaper
author SEARS, Derek W. G.
YOZZO, Jordan
RAGLAND, Christina
spellingShingle SEARS, Derek W. G.
YOZZO, Jordan
RAGLAND, Christina
The natural thermoluminescence of Antarctic meteorites and their terrestrial ages and orbits: A 2010 update
author_facet SEARS, Derek W. G.
YOZZO, Jordan
RAGLAND, Christina
author_sort SEARS, Derek W. G.
title The natural thermoluminescence of Antarctic meteorites and their terrestrial ages and orbits: A 2010 update
title_short The natural thermoluminescence of Antarctic meteorites and their terrestrial ages and orbits: A 2010 update
title_full The natural thermoluminescence of Antarctic meteorites and their terrestrial ages and orbits: A 2010 update
title_fullStr The natural thermoluminescence of Antarctic meteorites and their terrestrial ages and orbits: A 2010 update
title_full_unstemmed The natural thermoluminescence of Antarctic meteorites and their terrestrial ages and orbits: A 2010 update
title_sort natural thermoluminescence of antarctic meteorites and their terrestrial ages and orbits: a 2010 update
publisher Wiley
publishDate 2011
url http://dx.doi.org/10.1111/j.1945-5100.2010.01139.x
https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1111%2Fj.1945-5100.2010.01139.x
https://onlinelibrary.wiley.com/doi/pdf/10.1111/j.1945-5100.2010.01139.x
geographic Antarctic
The Antarctic
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The Antarctic
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Antarctic
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Antarctic
op_source Meteoritics & Planetary Science
volume 46, issue 1, page 79-91
ISSN 1086-9379 1945-5100
op_rights http://onlinelibrary.wiley.com/termsAndConditions#vor
op_doi https://doi.org/10.1111/j.1945-5100.2010.01139.x
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