posted on 2012-10-24, 09:08authored byD. Queloz, D. Anderson, A. C. Cameron, M. Gillon, L. Hebb, C. Hellier, P. Maxted, F. Pepe, D. Pollacco, D. Segransan, B. Smalley, A. H. M. J. Triaud, S. Udry, R. West
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.
History
Citation
Astronomy & Astrophysics, 2010, 517
Version
VoR (Version of Record)
Published in
Astronomy & Astrophysics
Publisher
EDP Sciences for European Southern Observatory (ESO)