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HAT-P-10b: A Light and Moderately Hot Jupiter Transiting A K Dwarf

Bakos, G. Á. and Pál, A. and Torres, G. and Sipőcz, B. and Latham, D. W. and Noyes, R. W. and Kovács, Géza and Hartman, J. and Esquerdo, G. A. and Fischer, D. A. and Johnson, J. A. and Marcy, G. W. and Butler, R. P. and Howard, A. W. and Sasselov, D. D. and Kovács, Gábor and Stefanik, R. P. and Lázár, J. and Papp, I. and Sári, P. (2009) HAT-P-10b: A Light and Moderately Hot Jupiter Transiting A K Dwarf. Astrophysical Journal, 696 (2). pp. 1950-1955. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20130111-084302778

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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 T_c = 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.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/696/2/1950DOIArticle
http://iopscience.iop.org/0004-637X/696/2/1950PublisherArticle
ORCID:
AuthorORCID
Bakos, G. Á.0000-0001-7204-6727
Torres, G.0000-0002-5286-0251
Latham, D. W.0000-0001-9911-7388
Esquerdo, G. A.0000-0002-9789-5474
Fischer, D. A.0000-0003-2221-0861
Johnson, J. A.0000-0001-9808-7172
Marcy, G. W.0000-0002-2909-0113
Howard, A. W.0000-0001-8638-0320
Sasselov, D. D.0000-0001-7014-1771
Additional Information:© 2009 American Astronomical Society. Received 2008 September 24; accepted 2009 February 18; published 2009 April 28. Based in part on observations obtained at the W. M. Keck Observatory, which is operated by the University of California and the California Institute of Technology. Keck time has been granted by NOAO (A285Hr) and NASA (N128Hr). HATNet operations have been funded by NASA grants NNG04GN74G, NNX08AF23G, and SAO IR&D grants. The efforts of G.Á.B. and J.A.J. were supported by the Postdoctoral Fellowship of the NSF Astronomy and Astrophysics Program (AST-0702843 and AST-0702821, respectively). We also acknowledge partial support from the Kepler Mission under NASA Cooperative Agreement NCC2-1390 (PI: D.W.L.). G.K. thanks the Hungarian Scientific Research Foundation (OTKA) for support through grant K-60750. This research has made use of Keck telescope time granted through NOAO (program A285Hr) and NASA (N128Hr).
Funders:
Funding AgencyGrant Number
NASANNG04GN74G
NASANNX08AF23G
Smithsonian Astrophysical ObservatoryUNSPECIFIED
NSF Astronomy and Astrophysics FellowshipAST-0702843
NSF Astronomy and Astrophysics FellowshipAST-0702821
NASANCC2-1390
Hungarian Scientific Research Fund (OTKA)K-60750
Subject Keywords:planetary systems; stars: individual (HAT-P-10, GSC 02340-01714); techniques: photometric; techniques: spectroscopic
Issue or Number:2
Record Number:CaltechAUTHORS:20130111-084302778
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20130111-084302778
Official Citation:HAT-P-10b: A Light and Moderately Hot Jupiter Transiting A K Dwarf G. Á. Bakos et al. 2009 ApJ 696 1950
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:36312
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:11 Jan 2013 17:04
Last Modified:09 Mar 2020 13:19

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