publication . Article . Other literature type . Preprint . 2012


Spiegel, David S.; Burrows, Adam;
Open Access
  • Published: 16 Jan 2012 Journal: The Astrophysical Journal, volume 745, page 174 (issn: 0004-637X, eissn: 1538-4357, Copyright policy)
  • Publisher: IOP Publishing
Gas-giant planets that form via core accretion might have very different characteristics from those that form via disk-instability. Disk-instability objects are typically thought to have higher entropies, larger radii, and (generally) higher effective temperatures than core-accretion objects. We provide a large set of models exploring the observational consequences of high-entropy (hot) and low-entropy (cold) initial conditions, in the hope that this will ultimately help to distinguish between different physical mechanisms of planet formation. However, the exact entropies and radii of newly-formed planets due to these two modes of formation cannot, at present, b...
arXiv: Astrophysics::Earth and Planetary AstrophysicsAstrophysics::Galaxy AstrophysicsAstrophysics::Solar and Stellar Astrophysics
free text keywords: Space and Planetary Science, Astronomy and Astrophysics, Jupiter mass, Astrophysics, Astronomy, Physics, Planetary mass, Giant planet, Planet, Planetary migration, Jupiter, Primary atmosphere, Hot Jupiter, Astrophysics - Earth and Planetary Astrophysics
Related Organizations
Funded by
NSF| Postdoctoral program in theoretical and observational astrophysics
  • Funder: National Science Foundation (NSF)
  • Project Code: 0807444
  • Funding stream: Directorate for Mathematical & Physical Sciences | Division of Astronomical Sciences
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