The effects of metallicity and grain growth and settling on the early evolution of gaseous protoplanets

The effects of metallicity and grain growth and settling on the early evolution of gaseous protoplanets

Giant protoplanets formed by gravitational instability in the outer regions of circumstellar disks go through an early phase of quasi-static contraction during which radii are large (∼1 AU) and internal temperatures are low (

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Bibliographische Detailangaben
Veröffentlicht in:Icarus (New York, N.Y. 1962) N.Y. 1962), 2011-02, Vol.211 (2), p.939-947
Hauptverfasser: Helled, R., Bodenheimer, P.
Format: Artikel
Sprache:eng
Schlagworte:
Astronomy
Earth, ocean, space
Exact sciences and technology
Extrasolar planets
Jovian planets
Planetary formation
Solar system
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Beschreibung
Zusammenfassung:Giant protoplanets formed by gravitational instability in the outer regions of circumstellar disks go through an early phase of quasi-static contraction during which radii are large (∼1 AU) and internal temperatures are low (
ISSN:0019-1035
1090-2643
DOI:10.1016/j.icarus.2010.09.024