The New Transiting Planet OGLE‐TR‐56b: Orbit and Atmosphere
Author(s) -
Dimitar Sasselov
Publication year - 2003
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/378145
Subject(s) - planet , physics , exoplanet , giant planet , astrophysics , atmosphere (unit) , astronomy , orbit (dynamics) , convection , astrobiology , planetary system , mechanics , meteorology , engineering , aerospace engineering
Motivated by the identification of the very close-in extrasolar giant planetOGLE-TR-56b, we explore the implications of its existence on problems of tidaldissipation, planet migration, and atmospheric stability. The small orbit ofOGLE-TR-56b makes the planet an interesting test particle case for tidaldissipation in stellar convection zones. We show that it favors prescriptionsof suppressed convective eddy viscosity. Precise timing of the transits ofOGLE-TR-56b might place interesting constraints on stellar convection theory,if orbital period change is detected in the near future.Comment: 12 pages, 1 figure, submitted to ApJ
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