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The natural thermoluminescence of meteorites. III - Lunar and basaltic meteoritesNatural thermoluminescence (TL) data were obtained to investigate recent thermal and radiation histories of the lunar meteorite MacAlpine Hills 88104/5 and 65 eucrites, howardites, diogenites, and mesosiderites. All these meteorites have low levels of natural TL compared to chondrites, which is primarily because they display anomalous fading. Some meteorites have especially low natural TL which must reflect heating within the last 100,000-1,000,000 y. The parameters for TL decay were determined assuming plausible values for cosmic ray dose rate and that the natural TL of MAC88104/5 was totally drained by ejection from the moon. The obtained parameters for TL decay suggest that the moon-earth transit times for MAC88104 and MAC88105 were 2,000 and 1,800 y, respectively, compared with 19,000 and 2,500 y for Y791197 and ALHA81005, respectively.
Document ID
19920032190
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Sears, Derek W. G.
(Arkansas Univ. Fayetteville, AR, United States)
Benoit, Paul H.
(Arkansas Univ. Fayetteville, AR, United States)
Sears, Hazel
(Arkansas Univ. Fayetteville, AR, United States)
Batchelor, J. D.
(Arkansas Univ. Fayetteville, AR, United States)
Symes, Steve
(Arkansas, University Fayetteville, United States)
Date Acquired
August 15, 2013
Publication Date
November 1, 1991
Publication Information
Publication: Geochimica et Cosmochimica Acta
Volume: 55
ISSN: 0016-7037
Subject Category
Lunar And Planetary Exploration
Accession Number
92A14814
Funding Number(s)
CONTRACT_GRANT: NSF DPP-88-17569
CONTRACT_GRANT: NAG9-81
CONTRACT_GRANT: NSF CME-89-00501
Distribution Limits
Public
Copyright
Other

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