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The Cr Redox Record of fO2 Variation in Angrites. Evidence for Redox Conditions of Angrite Petrogenesis and Parent BodyAngrites represent some of the earliest stages of planetesimal differentiation. Not surprisingly, there is no simple petrogenetic model for their origin. Petrogenesis has been linked to both magmatic and impact processes. Studies demonstrated that melting of chondritic material (e.g. CM, CV) at redox conditions where pure iron metal is unstable (e.g., IW+1 to IW+2) produced angrite-like melts. Alternatively, angrites were produced at more reducing conditions (
Document ID
20160003474
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Shearer, Charles K.
(New Mexico Univ. Albuquerque, NM, United States)
Bell, Aaron S.
(New Mexico Univ. Albuquerque, NM, United States)
Burger, Paul V.
(New Mexico Univ. Albuquerque, NM, United States)
Papike, James J.
(New Mexico Univ. Albuquerque, NM, United States)
Jones, John
(NASA Johnson Space Center Houston, TX, United States)
Le, Loan
(NASA Johnson Space Center Houston, TX, United States)
Date Acquired
March 16, 2016
Publication Date
March 21, 2016
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-CN-35723
Report Number: JSC-CN-35723
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: The Woodlands, TX
Country: United States
Start Date: March 21, 2016
End Date: March 25, 2016
Sponsors: Lunar and Planetary Inst.
Distribution Limits
Public
Copyright
Public Use Permitted.
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