Diffusive redistribution of water vapor in the solar nebula revisited

Details Diffusive redistribution of water vapor in the solar nebula revisited Diffusive redistribution of water vapor in the solar nebula revisited

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993lpi....24.1271s&link_type=abstract

In Lunar and Planetary Inst., Twenty-Fourth Lunar and Planetary Science Conference. Part 3: N-Z p 1271-1272 (SEE N94-20636 05-91

Physics

2

Asteroids, Diffusivity, Jupiter (Planet), Nebulae, Planetary Evolution, Protoplanets, Water Vapor, Drag, Planetary Geology, Solar System, Solar System Evolution

Scientific paper

Stevenson and Lunine presented a model for enhancing the abundance of solid material in the region of the solar nebula at the water condensation point. This was used to provide a means to produce a much more rapid formation of Jupiter than the standard solar nebula models. However, they underestimated the drag induced sun-ward radial drift of the planetesimals of interest. Reanalysis reveals that these particles would spread over the inner solar system and might influence the formation of the asteroids.

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