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Radial pressure in the solar nebula as affecting the motions of planetesimalsGrowing planetesimals and a range of drag laws depending on the Reynolds number and on the ratio of particle size to mean free path are considered. Particles spiral in the direction of positive gradient, thus being concentrated toward toroidal concentrations of gas. The effect increases with decreasing rates of particle growth, i.e., with increasing time scales of planet formation by accretion. In the outer regions, where evidence suggests that comets were formed and Uranus and Neptune were so accumulated, the effect of the pressure gradient is to clear the forming comets from those regions. The large mass of Neptune may have developed because of this effect, perhaps Neptune's solar distance was reduced from Bode's law, and perhaps no comet belt exists beyond Neptune. In the asteroid belt, on a slow time scale, the effect may have spiraled planetesimals toward Mars and Jupiter, thus contributing to the lack of planet formation in this region.
Document ID
19740011359
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Whipple, F. L.
(Harvard Coll. Obs. Cambridge, Mass., United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1973
Publication Information
Publication: NASA, Washington Evolutionary and Phys. Properties of Meteoroids
Subject Category
Space Sciences
Accession Number
74N19472
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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