Article (Scientific journals)
The Hot-Jupiter Kepler-17b: Discovery, Obliquity from Stroboscopic Starspots, and Atmospheric Characterization
Désert, Jean*-Michel; Charbonneau, David; Demory, Brice*-Olivier et al.
2011 • In Astrophysical Journal Supplement Series, 197, p. 14
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Keywords :
eclipses; planetary systems; stars: individual: Kepler-17b KIC 10619192 2MASS 19533486+4748540; techniques: photometric
Abstract :
[en] This paper reports the discovery and characterization of the transiting hot giant exoplanet Kepler-17b. The planet has an orbital period of 1.486 days, and radial velocity measurements from the Hobby-Eberly Telescope show a Doppler signal of 419.5[SUP]+13.3[/SUP] [SUB]-15.6[/SUB] m s[SUP]-1[/SUP]. From a transit-based estimate of the host star's mean density, combined with an estimate of the stellar effective temperature T [SUB]eff[/SUB] = 5630 ± 100 from high-resolution spectra, we infer a stellar host mass of 1.06 ± 0.07 M [SUB]&sun;[/SUB] and a stellar radius of 1.02 ± 0.03 R [SUB]&sun;[/SUB]. We estimate the planet mass and radius to be M [SUB]P[/SUB] = 2.45 ± 0.11 M [SUB]J[/SUB] and R [SUB]P[/SUB] = 1.31 ± 0.02 R [SUB]J[/SUB]. The host star is active, with dark spots that are frequently occulted by the planet. The continuous monitoring of the star reveals a stellar rotation period of 11.89 days, eight times the planet's orbital period; this period ratio produces stroboscopic effects on the occulted starspots. The temporal pattern of these spot-crossing events shows that the planet's orbit is prograde and the star's obliquity is smaller than 15°. We detected planetary occultations of Kepler-17b with both the Kepler and Spitzer Space Telescopes. We use these observations to constrain the eccentricity, e, and find that it is consistent with a circular orbit (e < 0.011). The brightness temperatures of the planet's infrared bandpasses are T_{3.6\, {\mu m}} = 1880 ± 100 K and T_{4.5\, {\mu m}} = 1770 ± 150 K. We measure the optical geometric albedo A[SUB]g[/SUB] in the Kepler bandpass and find A[SUB]g[/SUB] = 0.10 ± 0.02. The observations are best described by atmospheric models for which most of the incident energy is re-radiated away from the day side.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Désert, Jean*-Michel;  Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
Charbonneau, David;  Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
Demory, Brice*-Olivier;  Massachusetts Institute of Technology, Cambridge, MA 02159, USA
Ballard, Sarah;  Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
Carter, Joshua A;  Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
Fortney, Jonathan J;  Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064, USA
Cochran, William D;  Department of Astronomy, University of Texas, Austin, USA
Endl, Michael;  Department of Astronomy, University of Texas, Austin, USA
Quinn, Samuel N;  Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
Isaacson, Howard T;  Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA
Fressin, François;  Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
Buchhave, Lars A;  Neils Bohr Institute, University of Copenhagen, DK-2100 Denmark
Latham, David W;  Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
Knutson, Heather A;  Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA
Bryson, Stephen T;  NASA Ames Research Center, Moffett Field, CA 94035, USA
Torres, Guillermo;  Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
Rowe, Jason F;  NASA Ames Research Center, Moffett Field, CA 94035, USA
Batalha, Natalie M;  San Jose State University, San Jose, CA 95192, USA
Borucki, William J;  NASA Ames Research Center, Moffett Field, CA 94035, USA
Brown, Timothy M;  Las Cumbres Observatory Global Telescope, Goleta, CA 93117, USA
Caldwell, Douglas A;  SETI Institute/NASA Ames Research Center, Moffett Field, CA 94035, USA
Christiansen, Jessie L;  NASA Ames Research Center, Moffett Field, CA 94035, USA
Deming, Drake;  Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
Fabrycky, Daniel C;  Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064, USA
Ford, Eric B;  Department of Astronomy, University of Florida, Gainesville, FL 32611, USA
Gilliland, Ronald L;  Space Telescope Science Institute, Baltimore, MD 21218, USA
Gillon, Michaël  ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique et traitement de l'image
Haas, Michaël R;  NASA Ames Research Center, Moffett Field, CA 94035, USA
Jenkins, Jon M;  SETI Institute/NASA Ames Research Center, Moffett Field, CA 94035, USA
Kinemuchi, Karen;  Bay Area Environmental Research Inst./NASA Ames Research Center, Moffett Field, CA 94035, USA
Koch, David;  NASA Ames Research Center, Moffett Field, CA 94035, USA
Lissauer, Jack J;  Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
Lucas, Philip;  Centre for Astrophyiscs Research, University of Hertfordshire, College Lane, Hatfield, AL10 9AB, UK
Mullally, Fergal;  SETI Institute/NASA Ames Research Center, Moffett Field, CA 94035, USA
MacQueen, Phillip J;  Department of Astronomy, University of Texas, Austin, USA
Marcy, Geoffrey W;  Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA
Sasselov, Dimitar D;  Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
Seager, Sara;  Massachusetts Institute of Technology, Cambridge, MA 02159, USA
Still, Martin;  Bay Area Environmental Research Inst./NASA Ames Research Center, Moffett Field, CA 94035, USA
Tenenbaum, Peter;  SETI Institute/NASA Ames Research Center, Moffett Field, CA 94035, USA
Uddin, Kamal;  Orbital Sciences Corporation/NASA Ames Research Center, Moffett Field, CA 94035, USA
Winn, Joshua N;  Massachusetts Institute of Technology, Cambridge, MA 02159, USA
More authors (32 more) Less
Language :
English
Title :
The Hot-Jupiter Kepler-17b: Discovery, Obliquity from Stroboscopic Starspots, and Atmospheric Characterization
Publication date :
01 November 2011
Journal title :
Astrophysical Journal Supplement Series
ISSN :
0067-0049
eISSN :
1538-4365
Publisher :
Univ Chicago Press, Chicago, United States - Illinois
Volume :
197
Pages :
14
Peer reviewed :
Peer Reviewed verified by ORBi
Commentary :
http://de.arxiv.org/abs/1107.5750
Available on ORBi :
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