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| Query : 2005ApJ...628L.159W |
2005ApJ...628L.159W - Astrophys. J., 628, L159-L162 (2005/August-1)
Obliquity tides on hot Jupiters.
WINN J.N. and HOLMAN M.J.
Abstract (from CDS):
Obliquity tides are a potentially important source of heat for extrasolar planets on close-in orbits. Although tidal dissipation will usually reduce the obliquity to zero, a nonzero obliquity can persist if the planet is in a Cassini state, a resonance between spin precession and orbital precession. Obliquity tides might be the cause of the anomalously large size of the transiting planet HD 209458b.
Abstract Copyright: ∼
Journal keyword(s): Celestial Mechanics - Stars: Planetary Systems: Formation - Planets and Satellites: Formation - Stars: Individual: Henry Draper Number: HD 209458
Simbad objects: 2
| Number of rows : 2 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | HD 209458b | Pl | 22 03 10.7727465312 | +18 53 03.549393384 | ~ | 2037 | 1 | |||||
| 2 | HD 209458 | V* | 22 03 10.7727465312 | +18 53 03.549393384 | 8.21 | 7.63 | F9V | 1193 | 1 |
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