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Black ordinary chondrites - An analysis of abundance and fall frequencyBlack ordinary chondrite meteorites sample the spectral effects of shock on ordinary chondrite material in the space environment. Since shock is an important regolith process these meteorites provide insight into the spectral properties of the regoliths on ordinary chondrite parent bodies. To determine how common black chondrites are in the meteorite collection and, by analogy, the frequency of shock-alteration in ordinary chondrites, several of the world's major meteorite collections were examined to identify black chondrites. Over 80 percent of all cataloged ordinary chondrites were examined and, using an optical definition, 61 black chondrites were identified. Black chondrites account for approximately 13.7 percent of ordinary chondrite falls. If the optically altered gas-rich ordinary chondrites are included the proportion of falls that exhibit some form of altered spectral properties increases to 16.7 percent. This suggests that optical alteration of asteroidal material in the space environment is a relatively common process.
Document ID
19920044032
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Britt, Daniel T.
(Arizona, University Tucson, United States)
Pieters, Carle M.
(Brown University Providence, RI, United States)
Date Acquired
August 15, 2013
Publication Date
December 1, 1991
Publication Information
Publication: Meteoritics
Volume: 26
ISSN: 0026-1114
Subject Category
Lunar And Planetary Exploration
Accession Number
92A26656
Funding Number(s)
CONTRACT_GRANT: NAGW-748
CONTRACT_GRANT: NAGW-28
Distribution Limits
Public
Copyright
Other

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