THE LOW DENSITY TRANSITING EXOPLANET WASP-15b
Journal Article
·
· Astronomical Journal (New York, N.Y. Online)
- Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH (United Kingdom)
- Astrophysics Group, Keele University, Staffordshire ST5 5BG (United Kingdom)
- Observatoire de Geneve, Universite de Geneve, 51 Chemin des Maillettes, 1290 Sauverny (Switzerland)
- School of Physics and Astronomy, University of St. Andrews, North Haugh, Fife KY16 9SS (United Kingdom)
- Department of Astronomy, Harvard University, 60 Garden Street, MS 10, Cambridge, MA 02138 (United States)
- Las Cumbres Observatory, 6740 Cortona Dr. Suite 102, Santa Barbara, CA 93117 (United States)
- Astrophysics Research Centre, School of Mathematics and Physics, Queen's University, University Road, Belfast BT7 1NN (United Kingdom)
We report the discovery of a low-density exoplanet transiting an 11th magnitude star in the Southern hemisphere. WASP-15b, which orbits its host star with a period P = 3.7520656 {+-} 0.0000028 d, has a mass M {sub p} = 0.542 {+-} 0.050 M {sub J} and radius R {sub p} = 1.428 {+-} 0.077 R {sub J}, and is therefore one of the least dense transiting exoplanets so far discovered ({rho}{sub p} = 0.247 {+-} 0.035 g cm{sup -3}). An analysis of the spectrum of the host star shows it to be of spectral type around F5, with an effective temperature T {sub eff} = 6300 {+-} 100 K and [Fe/H] = -0.17 {+-} 0.11.
- OSTI ID:
- 21255735
- Journal Information:
- Astronomical Journal (New York, N.Y. Online), Vol. 137, Issue 6; Other Information: DOI: 10.1088/0004-6256/137/6/4834; Country of input: International Atomic Energy Agency (IAEA); ISSN 1538-3881
- Country of Publication:
- United States
- Language:
- English
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