NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Experimental partial melting of the Allende (CV) and Murchison (CM) chondrites and the origin of asteroidal basaltFollowing the investigation of Jurewicz et al. (1991) on the composition of partial melts of eucrites and angrites, this study investigates partial melts of the Allende and Murchison chondrites and details the anhydrous phase relations of both chondrites at 1 atm, under temperatures and oxygen fugacities plausigle for the formation of basaltic meteorites. It was found that, in general, ambient oxygen fugacity exerts a strong influence on the compositions of partial melts of chondrites by controlling the amount of FeO available to the silicate system. At high f(O2), angritic magmas are produced, whereas eucritic melts are produced at low levels of f(O2).
Document ID
19930056653
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Jurewicz, A. J. G.
(NASA Lyndon B. Johnson Space Center Houston, TX, United States)
Mittlefehldt, D. W.
(Lockheed Engineering and Sciences Co. Houston, TX, United States)
Jones, J. H.
(NASA Johnson Space Center Houston, TX, United States)
Date Acquired
August 16, 2013
Publication Date
May 1, 1993
Publication Information
Publication: Geochimica et Cosmochimica Acta
Volume: 57
Issue: 9
ISSN: 0016-7037
Subject Category
Lunar And Planetary Exploration
Accession Number
93A40650
Funding Number(s)
PROJECT: RTOP 152-12-40-24
PROJECT: RTOP 152-13-40-21
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available