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H-chondrites - Trace element clues to their originRNAA is used to determine the abundances of 20 trace elements in four H4, two H3, two H5, and two H6 chondrites from the British Museum, as a contribution to a multiple-method study of these objects. The results are presented in tables and graphs and analyzed in terms of the inhomogeneity of the parent bodies and the depletion of volatiles in the higher petrologic types. Features observed include siderophile depletion in H3 chondrites; systematic variation of siderophile abundance pattern with petrologic type; volatile depletion as a primary feature; mineralogy consistent with accretion at 420-500 K; and the factor-analysis groupings siderophiles (Os, Re, Ir, Ni, Pd, Au, and Ge), volatiles (Ag, Br, In, Cd, Bi, and Tl), and alkalis (Rb and Cs).
Document ID
19850043689
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Morgan, J. W.
(U.S. Geological Survey, Reston, VA; Chicago, University Chicago, IL, United States)
Janssens, M.-J.
(Geological Survey Reston, VA, United States)
Anders, E.
(Chicago, University Chicago, IL, United States)
Takahashi, H.
(Furukawa Electric Co., Tokyo, Japan; Chicago, University Chicago, IL, United States)
Hertogen, J.
(Leuven, Katholieke Universiteit Louvain, Belgium; Chicago, University, Chicago, IL, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1985
Publication Information
Publication: Geochimica et Cosmochimica Acta
Volume: 49
ISSN: 0016-7037
Subject Category
Lunar And Planetary Exploration
Accession Number
85A25840
Funding Number(s)
CONTRACT_GRANT: NAG9-52
CONTRACT_GRANT: NGL-14-001-167
Distribution Limits
Public
Copyright
Other

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