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Opaque mineralogy - Apollo 17, rock 75035Rock 75035 is a medium-grained, holocrystalline, subophitic ilmenite basalt collected from the rim of Camelot Crater, and is believed to represent the subfloor basalts of the Taurus-Littrow valley. The rock consists of the major minerals pyroxene (45%), plagioclase (31%), and ilmenite (17%). Minor minerals include cristobalite (about 5%), troilite, native Fe, tranquillityite, baddeleyite, zirconolite, and rare ulvospinel. No olivine or armalcolite was observed in the specimen 75035,76. Mineralogically and chemically, as well as in age, this rock is similar to others collected from Camelot and other stations during the Apollo 17 mission. These rocks are almost identical to the Type B ilmenite basalts of Mare Tranquillitatis.
Document ID
19750055513
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Meyer, H. O. A.
Boctor, N. Z.
(Purdue University West Lafayette, Ind., United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1974
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: March 18, 1974
End Date: March 22, 1974
Accession Number
75A39585
Funding Number(s)
CONTRACT_GRANT: PAHC-0213
CONTRACT_GRANT: NGR-15-005-157
CONTRACT_GRANT: ARPA GH-33574A1
Distribution Limits
Public
Copyright
Other

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