期刊
ASTROPHYSICAL JOURNAL
卷 696, 期 2, 页码 1950-1955出版社
IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/696/2/1950
关键词
planetary systems; stars: individual (HAT-P-10, GSC 02340-01714); techniques: photometric; techniques: spectroscopic
资金
- NASA [NNG04GN74G, NNX08AF23G, NCC2-1390, N128Hr]
- SAO IR D
- NSF [AST-0702843, AST-0702821]
- Hungarian Scientific Research Foundation (OTKA) [K-60750]
- NOAO [A285Hr]
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 T-c = 2454759.68683 +/- 0.00016 (BJD), and duration 0.1090 +/- 0.0008 days. HAT-P-10b has a radius of 1.005(-0.027)(+0.032) 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-P10b is consistent with a similar to 4.5Gyr, almost pure hydrogen and helium gas giant planet with a 10 M-circle plus core. With an equilibrium temperature of T-eq = 1020 +/- 17 K, HAT-P-10b is one of the coldest TEPs. Curiously, its Safronov number theta = 0.053 +/- 0.002 falls close to the dividing line between the two suggested TEP populations.
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