Segregation of the non-volatile compounds in turbulent protoplanets

Details Segregation of the non-volatile compounds in turbulent protoplanets Segregation of the non-volatile compounds in turbulent protoplanets

Nov 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978m%26p....19..399s&link_type=abstract

Moon and the Planets, vol. 19, Nov. 1978, p. 399-407.

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4

Interstellar Matter, Planetary Evolution, Turbulence Effects, Volatility, Gravitational Fields, Hydrogen Clouds, Mass Distribution, Nebulae, Physical Properties, Separation, Vapor Pressure

Scientific paper

The effect of turbulence on grain segragation in gaseous protoplanets is studied. It is shown that core formation occurs despite turbulence and that the segregation time is not much larger than in the standard nonmixing case. All the calculated infall times have values close to each other, and it is suggested that similar results would hold for a solar nebula with segregation onto the mid-plane.

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