HAT-P-10b: A LIGHT AND MODERATELY HOT JUPITER TRANSITING A K DWARF
Open Access
- 28 April 2009
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 696 (2) , 1950-1955
- https://doi.org/10.1088/0004-637x/696/2/1950
Abstract
We report on the discovery of HAT-P-10b, one of the lowest mass (0.487 ± 0.018 M J) transiting extrasolar planets (TEPs) discovered to date by transit searches. HAT-P-10b orbits the moderately bright V = 11.89 K dwarf GSC 02340-01714, with a period P = 3.7224747 ± 0.0000065 days, transit epoch Tc = 2454759.68683 ± 0.00016 (BJD), and duration 0.1090 ± 0.0008 days. HAT-P-10b has a radius of 1.005+0.032 –0.027 R J yielding a mean density of 0.594 ± 0.052 g cm–3. Comparing these observations with recent theoretical models we find that HAT-P-10b is consistent with a ~4.5 Gyr, almost pure hydrogen and helium gas giant planet with a 10 M ⊕ core. With an equilibrium temperature of T eq = 1020 ± 17 K, HAT-P-10b is one of the coldest TEPs. Curiously, its Safronov number θ = 0.053 ± 0.002 falls close to the dividing line between the two suggested TEP populations.Keywords
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This publication has 43 references indexed in Scilit:
- HAT-P-5b: A Jupiter-like Hot Jupiter Transiting a Bright StarThe Astrophysical Journal, 2007
- HD 147506b: A Supermassive Planet in an Eccentric Orbit Transiting a Bright StarThe Astrophysical Journal, 2007
- HD 17156b: a transiting planet with a 21.2-day period and an eccentric orbitAstronomy & Astrophysics, 2007
- Possible Solutions to the Radius Anomalies of Transiting Giant PlanetsThe Astrophysical Journal, 2007
- Theory for the Secondary Eclipse Fluxes, Spectra, Atmospheres, and Light Curves of Transiting Extrasolar Giant PlanetsThe Astrophysical Journal, 2006
- A Neptune‐Mass Planet Orbiting the Nearby M Dwarf GJ 436The Astrophysical Journal, 2004
- Wide‐Field Millimagnitude Photometry with the HAT: A Tool for Extrasolar Planet DetectionPublications of the Astronomical Society of the Pacific, 2004
- Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458Astronomy & Astrophysics, 2003
- System Description and First Light Curves of the Hungarian Automated Telescope, an Autonomous Observatory for Variability SearchPublications of the Astronomical Society of the Pacific, 2002
- Attaining Doppler Precision of 3 M s-1Publications of the Astronomical Society of the Pacific, 1996