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Riddles about the origin and thermal history of the moonMagmatic differentiation of the moon's interior, confirmed through calculations of thermal history, was studied. It appears that differentiation was a result of the moon's initial temperature whose origin remains unknown. In solving this problem, convective models of the moon were considered as well as a two layered differentiated model of the moon, operative over the past 3.5 billion years. The high content of long lived radioactive elements present was investigated in explaining the moon's current thermal properties. The controversy concerning the true nature of magmatic differentiation continues to be unsolved.
Document ID
19780005005
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Levin, B. Y.
(Academy of Sciences (USSR) Moscow, Ussr)
Mayeva, S. V.
(Academy of Sciences (USSR) Moscow, Ussr)
Date Acquired
August 9, 2013
Publication Date
January 1, 1977
Publication Information
Publication: NASA, Washington The Soviet-Am. Conf. on Cosmochem. of the Moon and Planets, pt. 1
Subject Category
Astrophysics
Accession Number
78N12948
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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