Coel Hellier c.hellier@keele.ac.uk
WASP-20b and WASP-28b: a hot Saturn and a hot Jupiter in near-aligned orbits around solar-type stars
Hellier; Smalley; Maxted
Authors
Barry Smalley b.smalley@keele.ac.uk
Pierre Maxted p.maxted@keele.ac.uk
Abstract
We report the discovery of the planets WASP-20b and WASP-28b along with measurements of their sky-projected orbital obliquities. WASP-20b is an inflated, Saturn-mass planet (0.31?MJup; 1.46?RJup) in a 4.9-day, near-aligned (? = 12.7 ± 4.2°) orbit around CD-24 102 (V = 10.7; F9). Due to the low density of the planet and the apparent brightness of the host star, WASP-20 is a good target for atmospheric characterisation via transmission spectroscopy. WASP-28b is an inflated, Jupiter-mass planet (0.91?MJup; 1.21?RJup) in a 3.4-day, near-aligned (? = 8 ± 18°) orbit around a V = 12, F8 star. As intermediate-mass planets in short orbits around aged, cool stars (7+ 2-1 Gyr and 6000 ± 100 K for WASP-20; 5+ 3-2 Gyr and 6100 ± 150 K for WASP-28), their orbital alignment is consistent with the hypothesis that close-in giant planets are scattered into eccentric orbits with random alignments, which are then circularised and aligned with their stars’ spins via tidal dissipation.
Citation
Hellier, Smalley, & Maxted. (2015). WASP-20b and WASP-28b: a hot Saturn and a hot Jupiter in near-aligned orbits around solar-type stars. Astronomy & Astrophysics, https://doi.org/10.1051/0004-6361/201423591
Acceptance Date | Dec 5, 2014 |
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Publication Date | Feb 24, 2015 |
Journal | Astronomy & Astrophysics |
Print ISSN | 0004-6361 |
Publisher | EDP Sciences |
DOI | https://doi.org/10.1051/0004-6361/201423591 |
Keywords | planetary systems, stars, WASP-20b, WASP-28b |
Publisher URL | https://doi.org/10.1051/0004-6361/201423591 |
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Publisher Licence URL
https://creativecommons.org/licenses/by/4.0/
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