Problem of the formation of the distant planets

Details Problem of the formation of the distant planets Problem of the formation of the distant planets

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992prir....9....3p&link_type=abstract

Priroda (ISSN 0032-874X), no. 9, p. 3-9.

Other

Cosmology, Mathematical Models, Planetary Evolution, Stellar Mass Accretion, Stellar Mass Ejection, Accretion Disks, Interplanetary Dust, Interstellar Matter, Neptune (Planet), Pluto (Planet), Uranus (Planet)

Scientific paper

Two models for the formation of the distant planets in the solar system (i.e., Uranus, Neptune, and Pluto) are presented: solid-body accumulation and the evolution of condensations. In the first model, consideration of the ejection of bodies from the feed zone of the growing planet did not lead to a solution of the time-of-growth problem for the distant planets. On the other hand, the second model provides a solution not only to the time-of-growth problem but also to the sufficient-matter problem.

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