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chondrules of the very first generation in bencubbin/ch-like meteorites que94411 and hammadah al hamra 237: condensation origin at high ambient nebular temperaturesChondrules in QUE94411 and HH 237 formed at high ambient T prior to condensation of Fe,Ni-metal following a large scale thermal event that resulted in complete vaporization of a solar nebula region. These chondrules escaped subsequent remelting.
Document ID
20000081089
Document Type
Conference Paper
Authors
Krot, Alexander N.
(Hawaii Univ. Manoa, HI United States)
Meibom, Anders
(Hawaii Univ. Manoa, HI United States)
Russell, Sara S.
(Museum of Natural History London, United Kingdom)
Young, Edward
(Oxford Univ. Oxford, United Kingdom)
Alexander, Conel M.
(Carnegie Institution of Washington Washington, DC United States)
McKeegan, Kevin D.
(California Univ. Los Angeles, CA United States)
Lofgren, Gary
(NASA Johnson Space Center Houston, TX United States)
Cuzzi, Jeff
(NASA Ames Research Center Moffett Field, CA United States)
Zipfel, Jutta
(Max-Planck-Inst. fuer Chemie Mainz, Germany)
Keil, Klaus
(NASA Ames Research Center Moffett Field, CA United States)
Date Acquired
August 19, 2013
Publication Date
March 1, 2000
Publication Information
Publication: Lunar and Planetary Science XXXI
Subject Category
Lunar and Planetary Science and Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle20000080557Analytic PrimaryLunar and Planetary Science XXXI