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Disk Tides and Accretion RunawayIt is suggested that tidal interaction of an accreting planetary embryo with the gaseous pre-planetary disk may provide a mechanism to breach the so-called runaway limit during the formation of the giant planet cores.
Document ID
20210003868
Acquisition Source
Jet Propulsion Laboratory
Document Type
Other
External Source(s)
hdl:2014/28083
Authors
Hahn, J.M.
Ward, W.R.
Date Acquired
January 1, 1995
Publication Date
January 1, 1995
Publication Information
Publisher: UNKNOWN
Distribution Limits
Public
Copyright
Other
Technical Review
Keywords
accretion
accretion
runaway
celestial
mechanics
solar
system
formation

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