PHOTOMETRICALLY DERIVED MASSES AND RADII OF THE PLANET AND STAR IN THE TrES-2 SYSTEM

被引:60
作者
Barclay, Thomas [1 ,2 ]
Huber, Daniel [1 ]
Rowe, Jason F. [1 ,3 ]
Fortney, Jonathan J. [4 ]
Morley, Caroline V. [4 ]
Quintana, Elisa V. [1 ,3 ]
Fabrycky, Daniel C. [4 ]
Barentsen, Geert [5 ]
Bloemen, Steven [6 ]
Christiansen, Jessie L. [1 ,3 ]
Demory, Brice-Olivier [7 ]
Fulton, Benjamin J. [8 ]
Jenkins, Jonm. [1 ,3 ]
Mullally, Fergal [1 ,3 ]
Ragozzine, Darin [9 ]
Seader, Shaun E. [1 ,3 ]
Shporer, Avi [8 ,10 ]
Tenenbaum, Peter [1 ,3 ]
Thompson, Susan E. [1 ,3 ]
机构
[1] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[2] Bay Area Environm Res Inst Inc, Sonoma, CA 95476 USA
[3] SETI Inst, Mountain View, CA 94043 USA
[4] Univ Calif Santa Cruz, Dept Astron & Astrophys, Santa Cruz, CA 95064 USA
[5] Armagh Observ, Armagh BT61 9DG, North Ireland
[6] Katholieke Univ Leuven, Inst Sterrenkunde, B-3001 Louvain, Belgium
[7] MIT, Dept Earth Atmospher & Planetary Sci, Cambridge, MA 02139 USA
[8] Las Cumbres Observ Global Telescope Network, Santa Barbara, CA 93117 USA
[9] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[10] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
基金
欧洲研究理事会;
关键词
planets and satellites: individual (TrES-2b); stars: individual (TrES-2A); techniques: photometric; TRANSIT TIMING OBSERVATIONS; SOLAR-LIKE OSCILLATIONS; HOT JUPITER ATMOSPHERES; SPACE-BASED PHOTOMETRY; LIGHT CURVES; EXTRASOLAR PLANETS; KEPLER-MISSION; RED GIANTS; ELLIPSOIDAL VARIATIONS; HD; 209458B;
D O I
10.1088/0004-637X/761/1/53
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We measure the mass and radius of the star and planet in the TrES-2 system using 2.7 years of observations by the Kepler spacecraft. The light curve shows evidence for ellipsoidal variations and Doppler beaming on a period consistent with the orbital period of the planet with amplitudes of 2.79(-0.62)(+0.44) and 3.44(-0.37)(+0.32) parts per million (ppm), respectively, and a difference between the dayside and the nightside planetary flux of 3.41(-0.82)(+0.55) ppm. We present an asteroseismic analysis of solar-like oscillations on TrES-2A which we use to calculate the stellar mass of 0.94 +/- 0.05 M-circle dot and radius of 0.95 +/- 0.02 R-circle dot. Using these stellar parameters, a transit model fit and the phase-curve variations, we determine the planetary radius of 1.162(-0.024)(+0.020) R-Jup and derive a mass for TrES-2b from the photometry of 1.44 +/- 0.21 M-Jup. The ratio of the ellipsoidal variation to the Doppler beaming amplitudes agrees to better than 2 sigma with theoretical predications, while our measured planet mass and radius agree within 2s of previously published values based on spectroscopic radial velocity measurements. We measure a geometric albedo of 0.0136(-0.0033)(+0.0022) and an occultation (secondary eclipse) depth of 6.5(-1.8)(+1.7) ppm which we combined with the day/night planetary flux ratio to model the atmosphere of TrES-2b. We find that an atmosphere model that contains a temperature inversion is strongly preferred. We hypothesize that the Kepler bandpass probes a significantly greater atmospheric depth on the night side relative to the day side.
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页数:10
相关论文
共 124 条
[1]   VERIFYING ASTEROSEISMICALLY DETERMINED PARAMETERS OF KEPLER STARS USING HIPPARCOS PARALLAXES: SELF-CONSISTENT STELLAR PROPERTIES AND DISTANCES [J].
Aguirre, V. Silva ;
Casagrande, L. ;
Basu, S. ;
Campante, T. L. ;
Chaplin, W. J. ;
Huber, D. ;
Miglio, A. ;
Serenelli, A. M. ;
Ballot, J. ;
Bedding, T. R. ;
Christensen-Dalsgaard, J. ;
Creevey, O. L. ;
Elsworth, Y. ;
Garcia, R. A. ;
Gilliland, R. L. ;
Hekker, S. ;
Kjeldsen, H. ;
Mathur, S. ;
Metcalfe, T. S. ;
Monteiro, M. J. P. F. G. ;
Mosser, B. ;
Pinsonneault, M. H. ;
Stello, D. ;
Weiss, A. ;
Tenenbaum, P. ;
Twicken, J. D. ;
Uddin, K. .
ASTROPHYSICAL JOURNAL, 2012, 757 (01)
[2]   TrES-1: The transiting planet of a bright K0V star [J].
Alonso, R ;
Brown, TM ;
Torres, G ;
Latham, DW ;
Sozzetti, A ;
Mandushev, G ;
Belmonte, JA ;
Charbonneau, D ;
Deeg, HJ ;
Dunham, EW ;
O'Donovan, FT ;
Stefanik, RP .
ASTROPHYSICAL JOURNAL, 2004, 613 (02) :L153-L156
[3]   A homogeneous spectroscopic analysis of host stars of transiting planets [J].
Ammler-von Eiff, M. ;
Santos, N. C. ;
Sousa, S. G. ;
Fernandes, J. ;
Guillot, T. ;
Israelian, G. ;
Mayor, M. ;
Melo, C. .
ASTRONOMY & ASTROPHYSICS, 2009, 507 (01) :523-530
[4]   THERMAL TIDES IN FLUID EXTRASOLAR PLANETS [J].
Arras, Phil ;
Socrates, Aristotle .
ASTROPHYSICAL JOURNAL, 2010, 714 (01) :1-12
[5]   System description and first light curves of the Hungarian Automated Telescope, an autonomous observatory for variability search [J].
Bakos, GA ;
Lázár, J ;
Papp, I ;
Sári, P ;
Green, EM .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2002, 114 (799) :974-987
[6]   A SEARCH FOR ADDITIONAL PLANETS IN THE NASA EPOXI OBSERVATIONS OF THE EXOPLANET SYSTEM GJ 436 [J].
Ballard, Sarah ;
Christiansen, Jessie L. ;
Charbonneau, David ;
Deming, Drake ;
Holman, Matthew J. ;
Fabrycky, Daniel ;
A'Hearn, Michael F. ;
Wellnitz, Dennis D. ;
Barry, Richard K. ;
Kuchner, Marc J. ;
Livengood, Timothy A. ;
Hewagama, Tilak ;
Sunshine, Jessica M. ;
Hampton, Don L. ;
Lisse, Carey M. ;
Seager, Sara ;
Veverka, Joseph F. .
ASTROPHYSICAL JOURNAL, 2010, 716 (02) :1047-1059
[7]   Serendipitous Kepler observations of a background dwarf nova of SU UMa type [J].
Barclay, Thomas ;
Still, Martin ;
Jenkins, Jon M. ;
Howell, Steve B. ;
Roettenbacher, Rachael M. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2012, 422 (02) :1219-1230
[8]  
Barnes R., 2010, Formation and evolution of exoplanets
[9]   EFFECT OF UNCERTAINTIES IN STELLAR MODEL PARAMETERS ON ESTIMATED MASSES AND RADII OF SINGLE STARS [J].
Basu, Sarbani ;
Verner, Graham A. ;
Chaplin, William J. ;
Elsworth, Yvonne .
ASTROPHYSICAL JOURNAL, 2012, 746 (01)
[10]   DETERMINATION OF STELLAR RADII FROM ASTEROSEISMIC DATA [J].
Basu, Sarbani ;
Chaplin, William J. ;
Elsworth, Yvonne .
ASTROPHYSICAL JOURNAL, 2010, 710 (02) :1596-1609