Structure and evolution of super-Earth to super-Jupiter exoplanets

2008/02/13 by I. Baraffe, G. Chabrier, Travis Barman +1 · 4 citations
Physics and Astronomy · #Astro and Planetary Science #Astrophysics and Star Formation Studies #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20079321

published as Astron.Astrophys.482:315-332,2008 · 20 pages, 12 figures. Accepted for publication in Astronomy and Astrophysics

arxiv created 2008/02/13 · openalex publication_date 2008/02/18 · arxiv updated 2014/11/18 · openalex created_date 2020/11/23 · openalex updated_date 2026/07/31

Abstract

Aims. We examine the uncertainties in current planetary models and quantify their impact on the planet cooling histories and mass-radius relationships.

Citations

• Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458
• On the Origin of HD 149026b
• Measuring the Oblateness and Rotation of Transiting Extrasolar Giant Planets
• Formation of the Giant Planets
• Detection of transits of the nearby hot Neptune GJ 436 b
• Models of giant planet formation with migration and disc evolution
• THE INTERIORS OF GIANT PLANETS: Models and Outstanding Questions
• Planetary Radii across Five Orders of Magnitude in Mass and Stellar Insolation: Application to Transits
• Irradiated Planets

Cited by

• The multiple planets transiting Kepler-9 I. Inferring stellar properties and planetary compositions
• THREE POSSIBLE ORIGINS FOR THE GAS LAYER ON GJ 1214b
• Atmospheric Dynamics of Hot Giant Planets and Brown Dwarfs
• Exoplanet [wikipedia]