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Abstract
We report the discovery of WASP-166b, a super-Neptune planet with a mass of 0.1 MJup (1.9 MNep) and a bloated radius of 0.63 RJup. It transits a V = 9.36, F9V star in a 5.44-d orbit that is aligned with the stellar rotation axis (sky-projected obliquity angle λ = 3 ± 5 degrees). Variations in the radial-velocity measurements are likely the result of magnetic activity over a 12-d stellar rotation period. WASP-166b appears to be a rare object within the “Neptune desert”.
Original language | English |
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Pages (from-to) | 3067-3075 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 488 |
Issue number | 3 |
Early online date | 10 Jul 2019 |
DOIs | |
Publication status | Published - Sept 2019 |
Keywords
- Planetary systems
- Stars: individual (WASP-166)
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Dive into the research topics of 'WASP-166b: a bloated super-Neptune transiting a V = 9 star'. Together they form a unique fingerprint.Projects
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Astronomy at St Andrews 2018-2021: Astronomy at St Andrews 2018-2021
Jardine, M. M. (PI), Bonnell, I. A. (CoI), Cameron, A. C. (CoI), Cyganowski, C. J. (CoI), Dominik, M. (CoI), Helling, C. (CoI), Horne, K. D. (CoI), Scholz, A. (CoI), Tojeiro, R. (CoI), Weijmans, A.-M. (CoI), Wild, V. (CoI), Woitke, P. (CoI), Wood, K. (CoI) & Zhao, H. (CoI)
1/04/18 → 31/03/22
Project: Standard