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Sulfidization Contemporaneous with Oxidation and Metamorphism in CK6 ChondritesAs the most oxidized chondrites and a group of carbonaceous chondrites spanning the range of petrologic types, CK chondrites occupy an extreme in our understanding of the origin and evolution of chondritic parent bodies. With the proposed linkage of CV and CK chondrites and the suggestion that differentiation of a postulated CV-CK asteroid could have differentiated to form a core and established a magnetic dynamo, CK chondrites are receiving considerable attention. Most of this attention has focused on the similarities between CK3 and CV3 chondrites and the origin of each. We have previously argued that melting of an oxidized core could produce a magnetite-sulfide core, rather than the more conventional metal-sulfide core. In this work, we focus on CK6 chondrites to understand the origin of the most highly metamorphosed members of the group as representative of the material that might differentiate to form such an oxidized core.
Document ID
20180002576
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
McCoy, T. J.
(Smithsonian Institution Washington, DC, United States)
Corrigan, C. M.
(Smithsonian Institution Washington, DC, United States)
Davidson, J.
(Carnegie Institution of Washington Washington, DC, United States)
Schrader, D. L.
(Arizona State Univ. Tempe, AZ, United States)
Righter, K.
(NASA Johnson Space Center Houston, TX, United States)
Date Acquired
April 27, 2018
Publication Date
March 19, 2018
Subject Category
Space Sciences (General)
Report/Patent Number
JSC-E-DAA-TN51567
Report Number: JSC-E-DAA-TN51567
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: The Woodlands, TX
Country: United States
Start Date: March 19, 2018
End Date: March 23, 2018
Sponsors: Lunar and Planetary Inst.
Distribution Limits
Public
Copyright
Public Use Permitted.
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