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Petrology of lunar rocks from the Sea of FertilityBased on a comparative analysis of the petrochemistry of an integrated sample of gabbro basalts and a fine fraction from regolith returned by Luna 16 automatic station from the Sea of Fertility, with the mean compositions of various types of mare basalts, anorthosites, and regolith from the Sea of Tranquillity and the Ocean of Storms, with reference to several data on rare elements, the nature of the fine fractions is discussed. It is shown that the integrated sample of gabbro basalt from the coarse fraction in the lower part of the core can be represented as a mixture of mare basalts of the Sea of Tranquillity and nonmare basalts of the krip type in the ratio of about 3 to 2. It is confirmed that the compositions of the Apollo 11 and Apollo 12 regolith are complementary with the compositions of basalts and anorthosites of the Sea of Tranquillity and the Ocean of Storms.
Document ID
19750003751
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Pavlenko, A. S.
(Kanner (Leo) Associates Redwood City, CA, United States)
Tarasov, L. S.
(Kanner (Leo) Associates Redwood City, CA, United States)
Shevaleyevskiy, I. D.
(Kanner (Leo) Associates Redwood City, CA, United States)
Ivanov, A. V.
(Kanner (Leo) Associates Redwood City, CA, United States)
Date Acquired
August 8, 2013
Publication Date
October 1, 1974
Publication Information
Publication: Lunar Soil From the Sea of Fertility (NASA-TT-F-15881)
Subject Category
Lunar And Planetary Exploration
Accession Number
75N11823
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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