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Scanning electron microscopy, non-dispersive X-ray analysis and electron microprobe studies of lunar soil, rocks and microbrecciaSilicate glass of composition similar to brown lunar glass was reduced with carbon and hydrogen. The typical complex iron sulfide and metallic iron mound formed by reduction with carbon is zoned. Its interior is metallic iron or a mixture of iron sulfide and metallic iron. The outer layer is pure metallic iron which is generally discontinuous, but the surface of the mound next to the silicate host is iron sulfide. This type of mound commonly has a waist of metallic iron and a void beneath it. The silicate surface of the void is covered with droplets or stringers of iron sulfide. The complex iron sulfide and metallic iron mounds formed by reduction with hydrogen generally are zoned. The outer layer is iron sulfide or a mixture of iron sulfide and metallic iron but the interior is metallic iron and iron sulfide, and the mound material next to the silicate host is iron sulfide. On the surface of some complex mounds, globules of silicate material are present. In one example, the globules consist of particles of aluminum oxide surrounded by silicate material. In turn, the margin of the globules is surrounded by iron sulfide. Dimples are present and surface of the dimples is covered by dendritic sheaths of iron sulfide and isolated metallic iron globules.
Document ID
19730014042
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Carter, J. L.
(Texas Univ. Dallas, TX, United States)
Date Acquired
September 2, 2013
Publication Date
September 28, 1972
Subject Category
Space Sciences
Report/Patent Number
NASA-CR-131870
Report Number: NASA-CR-131870
Accession Number
73N22769
Funding Number(s)
CONTRACT_GRANT: NGR-44-004-116
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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