CONFIRMATION OF A RETROGRADE ORBIT FOR EXOPLANET WASP-17b

被引:24
作者
Bayliss, Daniel D. R. [1 ]
Winn, Joshua N. [2 ,3 ]
Mardling, Rosemary A. [4 ]
Sackett, Penny D. [1 ]
机构
[1] Australian Natl Univ, Mt Stromlo Observ, Res Sch Astron & Astrophys, Weston, ACT 2611, Australia
[2] MIT, Dept Phys, Cambridge, MA 02139 USA
[3] MIT, Kavli Inst Astrophys & Space Res, Cambridge, MA 02139 USA
[4] Monash Univ, Sch Math Sci, Clayton, Vic 3800, Australia
关键词
planets and satellites: dynamical evolution and stability; planets and satellites: individual (WASP-17b); stars: individual (WASP-17); techniques: radial velocities; TRANSITING EXOPLANETS; SPIN; ALIGNMENT; PLANET; ROTATION; VELOCITY; STARS;
D O I
10.1088/2041-8205/722/2/L224
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present high-precision radial velocity observations of WASP-17 throughout the transit of its close-in giant planet, using the MIKE spectrograph on the 6.5 m Magellan Telescope at Las Campanas Observatory. By modeling the Rossiter-McLaughlin effect, we find the sky-projected spin-orbit angle to be lambda = 167.4 +/- 11.2 deg. This independently confirms the previous finding that WASP-17b is on a retrograde orbit, suggesting it underwent migration via a mechanism other than just the gravitational interaction between the planet and the disk. Interestingly, our result for lambda differs by 45 +/- 13 deg from the previously announced value, and we also find that the spectroscopic transit occurs 15 +/- 5 minutes earlier than expected, based on the published ephemeris. The discrepancy in the ephemeris highlights the need for contemporaneous spectroscopic and photometric transit observations whenever possible.
引用
收藏
页码:L224 / L227
页数:4
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