NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
The metallic microstructures and thermal histories of severely reheated chondritesThe metallographic structures of eight severely reheated chondrites - Farmington, Ramsdorf, Orvinio, Wickenburg, Lubbock, Rose City, Arapahoe, and Tadjera - were studied using optical, SEM and electron microprobe techniques. The following metallographic criteria were used to estimate the post-shock residual temperature of the chondrites: melted metal-troilite appearance, presence of martensite, phosphorus enrichment of metal and averaging of central metal grain compositions. The presence of phosphides and secondary kamacite are due to slow post-shock cooling rates. Ni rim gradients indicate both extensive remelting of metal grains and relatively fast cooling.
Document ID
19770060129
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Smith, B. A.
(Jones and Laughlin Steel Corp. Aliquippa, Pa., United States)
Goldstein, J. I.
(Lehigh University Bethlehem, Pa., United States)
Date Acquired
August 9, 2013
Publication Date
August 1, 1977
Publication Information
Publication: Geochimica et Cosmochimica Acta
Volume: 41
Subject Category
Lunar And Planetary Exploration
Accession Number
77A42981
Funding Number(s)
CONTRACT_GRANT: NGR-39-007-043
Distribution Limits
Public
Copyright
Other

Available Downloads

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