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DISCOVERY OF THE TRANSITING PLANET KEPLER-5b

2010/01/06 by David G. Koch, William J. Borucki, Jason F. Rowe +19 · 4 citations
Physics and Astronomy · Social Sciences · #Astronomy and Astrophysical Research #Educational Leadership and Practices #Hot Jupiter #Orbital period #Photometry (optics) #Planet #RADIUS #Radial velocity #Spectrograph #Stellar, planetary, and galactic studies #Transit (satellite) #astro-ph.EP

paper · pdf · doi:10.1088/2041-8205/713/2/l131

13 pages, 3 figures, submitted to the Astrophysical Journal Letters

arxiv created 2010/01/06 · openalex publication_date 2010/03/30 · arxiv updated 2015/05/14 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

We present 44 days of high duty cycle, ultra precise photometry of the 13th magnitude star Kepler-5 (KIC 8191672, T eff = 6300 K, log g = 4.1), which exhibits periodic transits with a depth of 0.7%. Detailed modeling of the transit is consistent with a planetary companion with an orbital period of 3.548460 ± 0.000032 days and a radius of 1.431 +0.041 −0.052 R J . Follow-up radial velocity measurements with the Keck HIRES spectrograph on nine separate nights demonstrate that the planet is more than twice as massive as Jupiter with a mass of 2.114 +0.056 −0.059 M J and a mean density of 0.894 ± 0.079 g cm −3 .

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