作者: O. D. Turner , D. R. Anderson , A. Collier Cameron , L. Delrez , D. F. Evans
DOI: 10.1088/1538-3873/128/964/064401
关键词: Astrophysics 、 Stars 、 Orbit 、 Astronomy 、 Transit (astronomy) 、 Planet 、 Variation (astronomy) 、 Physics 、 Atmosphere 、 Planetary system
摘要: We present the discovery by WASP-South survey of three planets transiting moderately bright stars (V ~ 11). WASP-120b is a massive (5.0MJup) planet in 3.6-day orbit that we find likely to be eccentric (e = 0.059+0.025-0.018) around an F5 star. WASP-122b hot-Jupiter (1.37MJup, 1.79RJup) 1.7-day about G4 Our predicted transit depth variation cause atmosphere suggests it well suited characterisation. WASP-123b (0.92MJup, 1.33RJup) 3.0-day old (~ 7 Gyr) G5