Is tidal heating sufficient to explain bloated exoplanets? Consistent calculations accounting for finite initial eccentricity

Astronomy and Astrophysics

Volumn 516, Issue 19, 2010, Pages

  Leconte, J ^a,b,c   Chabrier, G ^a,b,c   Baraffe, I ^a,b,c,d   Levrard, B ^a,b,c  

^a UNIVERSITÉ DE LYON   (France)

^b UNIVERSITÉ LYON 1   (France)

^c CENTRE DE RECHERCHE ASTROPHYSIQUE DE LYON   (France)

^d UNIVERSITY OF EXETER   (United Kingdom)

Author keywords

brown dwarfs; planet star interactions; planets and satellites: dynamical evolution and stability; planets and satellites: general

Indexed keywords

BROWN DWARFS; CIRCULAR ORBIT; EXO-PLANETS; EXOPLANET; FLUX TRANSPORT; GIANT PLANETS; HEAT BUDGET; INITIAL ECCENTRICITY; JUPITERS; LOW-MASS; ORBIT CIRCULARIZATION; ORBITAL PARAMETERS; PLANETS AND SATELLITES; PLANETS AND SATELLITES: GENERAL; QUALITY FACTORS; STELLAR IRRADIATION; SURFACE WINDS; THREE ORDERS OF MAGNITUDE; TIDAL DISSIPATION; TIDAL ENERGY; TIDAL EVOLUTION; TIDAL HEATING; TIDAL MODELS; TIME-SCALES;

BIOLOGY; ENERGY DISSIPATION; HEATING; ORBITAL LABORATORIES; PLANETS; SEDIMENTATION; STARS; TIDAL POWER;

SATELLITES;

EID: 77957831737     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014337     Document Type: Article

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