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The lunar angular momentum problemFormation of the Moon by classical Darwin-type fission of a rapidly spinning proto-Earth is discussed. The relationship of angular momentum to accretion disks is examined. The co-accretion scenario and Darwin-type fission are compared and evaluated.
Document ID
19850005443
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Weidenschilling, S. J. (Planetary Science Inst. Tucson, AZ, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1984
Publication Information
Publication: Lunar Planetary Inst. Conf. on the Origin of the Moon
Subject Category
Lunar And Planetary Exploration
Accession Number
85N13752
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19850005400Collected WorksConference on the Origin of the Moon
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