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Thermomagnetic analysis of meteorites, 2: C2 chondritesSamples of all eighteen of the known C2 chondrites were analyzed thermomagnetically. For eleven of these, initial Fe3O4 content is low(generally 1%) and the J sub s-T curves are irreversible. The heating curves show variable and erratic behavior, whereas the cooling curves appear to be that of Fe3O4. The saturation moment after cooling is greater (up to 10 times larger) than it is initially. This behavior is interpreted to be the result of the production of magnetite from a thermally unstable phase--apparently FeS. Four of the remaining 7 C2 chondrites contain Fe3O4 as the only significant magnetic phase: initial magnetite contents range from 4 to 13 percent. The remaining three C2 chondrites contain iron or nickel-iron in addition to Fe3O4. These seven C2 chondrites show little evidence of the breakdown of a thermally unstable phase.
Document ID
19740018171
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Watson, D. E.
(Geological Survey Boulder, CO, United States)
Larson, E. E.
(Geological Survey Boulder, CO, United States)
Herndon, J. M.
(Geological Survey Boulder, CO, United States)
Rowe, M. W.
(Geological Survey Boulder, CO, United States)
Date Acquired
September 3, 2013
Publication Date
January 1, 1974
Subject Category
Space Sciences
Report/Patent Number
NASA-CR-138507
Accession Number
74N26284
Funding Number(s)
CONTRACT_GRANT: NGR-06-003-181
CONTRACT_GRANT: NSF GP-18716
CONTRACT_GRANT: NGR-44-001-152
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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