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Growth of planetary crustsThe solid planets and satellites mostly have crusts which differ markedly in composition both from their interior, and from primordial solar nebula composition. Primary crusts, mercury, icy crusts, early intense cratering, Mars, Venus, Ganymede, and tertiary crusts are discussed.
Document ID
19880020863
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Taylor, Stuart Ross (Australian National Univ. Canberra, Australia)
Date Acquired
September 5, 2013
Publication Date
January 1, 1988
Publication Information
Publication: Lunar and Planetary Inst., Workshop on the Growth of Continental Crust
Subject Category
Geophysics
Accession Number
88N30247
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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