On the rapid formation of giant planet cores

Details On the rapid formation of giant planet cores On the rapid formation of giant planet cores

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...345l..99w&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 345, Oct. 15, 1989, p. L99-L102.

Astronomy and Astrophysics

Astrophysics

27

Gas Giant Planets, Planetary Cores, Planetary Evolution, Planetary Mass, Jupiter (Planet), Protoplanets, Saturn (Planet), Solar Corona, Planets, Giant Planets, Core, Formation, Origin, Accretion, Models, Timescale, Jupiter, Saturn, Theoretical Studies, Solar Nebula, Calculations, Parameters, Hypotheses

Scientific paper

The formation of the ice-rock cores of the giant planets by density wave-assisted accretion is outlined. The process could be rapid (100,000-1,000,000 yr) and completed within the probable lifetime of the solar nebula. The mechanism works for both Jupiter and Saturn and does not require a large excess of mass over that believed present in their cores.

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