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Collisional and dynamical processes in moon and planet formationResearch on a variety of dynamical processes relevant to the formation of planets, satellites and ring systems is discussed. The main focus is on studies of accretionary formation of early protoplanets using a numerical model, structures and evolution of ring systems and individual bodies within planetary rings, and theories of lunar origin.
Document ID
19870013954
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Chapman, C. R. (Planetary Science Inst. Tucson, AZ, United States)
Davis, D. R. (Planetary Science Inst. Tucson, AZ, United States)
Weidenschilling, S. J. (Planetary Science Inst. Tucson, AZ, United States)
Hartmann, W. K. (Planetary Science Inst. Tucson, AZ, United States)
Spaute, D. (Planetary Science Inst. Tucson, AZ, United States)
Date Acquired
September 5, 2013
Publication Date
May 1, 1987
Publication Information
Publication: NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1986
Subject Category
Astrophysics
Accession Number
87N23387
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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