Abstract
We report the discovery of WASP-8b, a transiting planet of 2.25 ± 0.08 MJup on a strongly inclined eccentric 8.15-day orbit, moving in a retrograde direction to the rotation of its late-G host star. Evidence is found that the star is in a multiple stellar system with two other companions. The dynamical complexity of the system indicates that it may have experienced secular interactions such as the Kozai mechanism or a formation that differs from the “classical” disc-migration theory.
Original language | English |
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Pages (from-to) | L1-L4 |
Number of pages | 4 |
Journal | Astronomy and Astrophysics |
Volume | 517 |
Issue number | 5 |
DOIs | |
Publication status | Published - 30 Jul 2010 |
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science