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An Ordinary Chondrite Impactor Composition for the Bosumtwi Impact Structure, Ghana, West Africa: Discussion of Siderophile Element Contents and Os and Cr Isotope DataOsmium isotope data had shown that Ivory Coast tektites contain an extraterrestrial component, but do not allow distinction between chondritic and iron meteorite contamination. PGE abundances of Ivory Coast tektites and impactites and target rocks from the Bosumtwi crater, the source crater of the Ivory Coast tektites, were all relatively high and did not allow to resolve the presence, or identify the nature, of the meteoritic component. However, Cr isotope analyses of an Ivory Coast tektite yielded a distinct 53Cr excess of 0.30+/-0.06, which indicates that the Bosumtwi impactor was an ordinary chondrite.
Document ID
20040058078
Acquisition Source
Johnson Space Center
Document Type
Extended Abstract
Authors
Christian Koeberl
(University of Vienna Vienna, Austria)
Alex Shukolyukov
(Scripps Institution of Oceanography La Jolla, United States)
Günter Lugmair
(Scripps Institution of Oceanography La Jolla, United States)
Date Acquired
August 21, 2013
Publication Date
January 1, 2004
Publication Information
Publication: Lunar and Planetary Science XXXV: Effects of Impacts: Shock and Awe
Publisher: Lunar and Planetary Institute
Subject Category
Geophysics
Meeting Information
Meeting: 35th Lunar and Planetary Science Conference
Location: League City, TX
Country: US
Start Date: March 15, 2004
End Date: March 19, 2004
Sponsors: Lunar and Planetary Institute
Distribution Limits
Public
Copyright
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