Tidal Dissipation in Extrasolar Planets
Many known extra-solar giant planets lie close to their host stars. Around 60 have their semi-major axes smaller than 0.05 AU. In contrast to planets further out, the vast majority of these close-in planets have low eccentricity orbits. This suggests that their orbits have been circularized likely d...
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| Language: | en_ca |
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2010
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| Online Access: | http://hdl.handle.net/1807/24849 |