Kepler-7B: A Transiting Planet With Unusually Low Density

dc.contributor.utaustinauthorCochran, William D.en_US
dc.creatorLatham, David W.en_US
dc.creatorBorucki, William J.en_US
dc.creatorKoch, David G.en_US
dc.creatorBrown, Timothy M.en_US
dc.creatorBuchhave, Lars A.en_US
dc.creatorBasri, Giboren_US
dc.creatorBatalha, Natalie M.en_US
dc.creatorCaldwell, Douglas A.en_US
dc.creatorCochran, William D.en_US
dc.creatorDunham, Edward W.en_US
dc.creatorFuresz, Gaboren_US
dc.creatorGautier, Thomas N., IIIen_US
dc.creatorGeary, John C.en_US
dc.creatorGilliland, Ronald L.en_US
dc.creatorHowell, Steve B.en_US
dc.creatorJenkins, Jon M.en_US
dc.creatorLissauer, Jack J.en_US
dc.creatorMarcy, Geoffrey W.en_US
dc.creatorMonet, David G.en_US
dc.creatorRowe, Jason F.en_US
dc.creatorSasselov, Dimitar D.en_US
dc.date.accessioned2016-10-28T19:34:22Z
dc.date.available2016-10-28T19:34:22Z
dc.date.issued2010-04en_US
dc.description.abstractWe report on the discovery and confirmation of Kepler-7b, a transiting planet with unusually low density. The mass is less than half that of Jupiter, M(P) = 0.43 M(J), but the radius is 50% larger, R(P) = 1.48 R(J). The resulting density, rho(P) = 0.17 g cm(-3), is the second lowest reported so far for an extrasolar planet. The orbital period is fairly long, P = 4.886 days, and the host star is not much hotter than the Sun, T(eff) = 6000 K. However, it is more massive and considerably larger than the Sun, M(star) = 1.35 M(circle dot) and R(star) = 1.84R(circle dot), and must be near the end of its life on the main sequence.en_US
dc.description.departmentAstronomyen_US
dc.description.sponsorshipNASA Cooperative Agreement NCC2-1390en_US
dc.identifierdoi:10.15781/T2TX35870
dc.identifier.citationLatham, David W., William J. Borucki, David G. Koch, Timothy M. Brown, Lars A. Buchhave, Gibor Basri, Natalie M. Batalha et al. "Kepler-7b: a transiting planet with unusually low density." The Astrophysical Journal Letters, Vol. 713, No. 2 (Apr., 2010): L140.en_US
dc.identifier.doi10.1088/2041-8205/713/2/l140en_US
dc.identifier.issn2041-8205en_US
dc.identifier.urihttp://hdl.handle.net/2152/42922
dc.language.isoEnglishen_US
dc.relation.ispartofen_US
dc.relation.ispartofserialAstrophysical Journal Lettersen_US
dc.rightsAdministrative deposit of works to Texas ScholarWorks: This works author(s) is or was a University faculty member, student or staff member; this article is already available through open access or the publisher allows a PDF version of the article to be freely posted online. The library makes the deposit as a matter of fair use (for scholarly, educational, and research purposes), and to preserve the work and further secure public access to the works of the University.en_US
dc.rights.restrictionOpenen_US
dc.subjectplanetary systemsen_US
dc.subjectstars: individual (kepler-7, kic 5780885, 2massen_US
dc.subject19141956+4105233)en_US
dc.subjecttechniques: spectroscopicen_US
dc.subjectstellaren_US
dc.subjectastronomy & astrophysicsen_US
dc.titleKepler-7B: A Transiting Planet With Unusually Low Densityen_US
dc.typeArticleen_US

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