Physics
Scientific paper
Nov 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995em%26p...71...73m&link_type=abstract
Earth, Moon, and Planets, Volume 71, Issue 1-2, pp. 73-84
Physics
Scientific paper
The Modern Laplacian Theory of the origin of the solar system (Prentice 1978) assumes a non-dissipative model of supersonic turbulence, and the existence of stable rings left behind during the contraction of the proto-sun. We show by numerical simulation that the turbulence is highly dissipative and the rings unstable. As a result of the instability, the rings spread and interact with the proto-sun. The rings therefore cannot form in the way Prentice proposed.
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