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TrES-4: A Transiting Hot Jupiter of Very Low Density

Mandushev, Georgi and O'Donovan, Francis T. and Charbonneau, David and Torres, Guillermo and Latham, David W. and Bakos, Gáspár Á. and Dunham, Edward W. and Sozzetti, Alessandro and Fernández, José M. and Esquerdo, Gilbert A. and Everett, Mark E. and Brown, Timothy M. and Rabus, Markus and Belmonte, Juan A. and Hillenbrand, Lynne A. (2007) TrES-4: A Transiting Hot Jupiter of Very Low Density. Astrophysical Journal Letters, 667 (2). L195-L198. ISSN 2041-8205. https://resolver.caltech.edu/CaltechAUTHORS:20100205-095420946

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Abstract

We report the discovery of TrES-4, a hot Jupiter that transits the star GSC 02620-00648 every 3.55 days. From high-resolution spectroscopy of the star, we estimate a stellar effective temperature of T_(eff) = 6100 ± 150 K, and from high-precision z and B photometry of the transit we constrain the ratio of the semimajor axis a and the stellar radius R_* to be a/R_* = 6.03 ± 0.13. We compare these values to model stellar isochrones to constrain the stellar mass to be M_* = 1.22 ± 0.17 M_⊙. Based on this estimate and the photometric time series, we constrain the stellar radius to be R_* = 1.738 ± 0.092 R_⊙ and the planet radius to be R_p = 1.674 ± 0.094 R_(Jup). We model our radial velocity data assuming a circular orbit and find a planetary mass of 0.84 ± 0.10 M_(Jup). Our radial velocity observations rule out line-bisector variations that would indicate a specious detection resulting from a blend of an eclipsing binary system. TrES-4 has the largest radius and lowest density of any of the known transiting planets. It presents a challenge to current models of the physical structure of hot Jupiters and indicates that the diversity of physical properties among the members of this class of exoplanets has yet to be fully explored.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/522115DOIArticle
http://www.iop.org/EJ/abstract/1538-4357/667/2/L195/PublisherArticle
ORCID:
AuthorORCID
Torres, Guillermo0000-0002-5286-0251
Latham, David W.0000-0001-9911-7388
Additional Information:© 2007 The American Astronomical Society. Received 2007 June 18; accepted 2007 August 6; published 2007 September 14. We thank Travis Barman for useful discussions. This Letter is based on work supported in part by NASA grants NNG04GN74G, NNG04LG89G, NNG05GI57G, NNG05GJ29G, and NNH05AB88I through the Origins of Solar Systems Program, and NASA Planetary Major Equipment grant N4G5-12229.We acknowledge support from the NASA Kepler mission under cooperative agreement NCC2-1390. Work by G. A´. B. was supported by NASA through Hubble Fellowship grant HST-HF-01170.01-A. Observing time on Keck I was awarded by NASA.
Funders:
Funding AgencyGrant Number
NASA NNG04GN74G
NASA NNG04LG89G
NASA NNG05GI57G
NASA NNG05GJ29G
NASA NNH05AB88I
NASA Planetary Major EquipmentN4G5-12229
NASA Kepler missionNCC2-1390
NASA Hubble FellowshipHST-HF-01170.01-A
Subject Keywords:planetary systems; techniques : photometric; techniques : radial velocities; techniques : spectroscopic
Issue or Number:2
Record Number:CaltechAUTHORS:20100205-095420946
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20100205-095420946
Official Citation:TrES-4: A Transiting Hot Jupiter of Very Low Density Georgi Mandushev, Francis T. O'Donovan, David Charbonneau, Guillermo Torres, David W. Latham, Gáspár Á. Bakos, Edward W. Dunham, Alessandro Sozzetti, José M. Fernández, Gilbert A. Esquerdo, Mark E. Everett, Timothy M. Brown, Markus Rabus, Juan A. Belmonte, and Lynne A. Hillenbrand 2007 ApJ 667 L195-L198 doi: 10.1086/522115
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:17395
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:09 Feb 2010 03:14
Last Modified:03 Oct 2019 01:27

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