Transits and occultations of an earth-sized planet in an 8.5 hr orbit

Roberto Sanchis-Ojeda, Saul Rappaport, Joshua N. Winn, Alan Levine, Michael C. Kotson, David W. Latham, Lars A. Buchhave

Research output: Contribution to journalArticle

81 Scopus citations

Abstract

We report the discovery of an Earth-sized planet (1.16 ± 0.19 R ) in an 8.5 hr orbit around a late G-type star (KIC 8435766, Kepler-xx). The object was identified in a search for short-period planets in the Kepler database and confirmed to be a transiting planet (as opposed to an eclipsing stellar system) through the absence of ellipsoidal light variations or substantial radial-velocity variations. The unusually short orbital period and the relative brightness of the host star (m Kep = 11.5) enable robust detections of the changing illumination of the visible hemisphere of the planet, as well as the occultations of the planet by the star. We interpret these signals as representing a combination of reflected and reprocessed light, with the highest planet dayside temperature in the range of 2300 K-3100 K. Follow-up spectroscopy combined with finer sampling photometric observations will further pin down the system parameters and may even yield the mass of the planet.

Original languageEnglish (US)
Article number54
JournalAstrophysical Journal
Volume774
Issue number1
DOIs
StatePublished - Sep 1 2013
Externally publishedYes

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • planetary systems
  • planets and satellites: atmospheres
  • planets and satellites: detection

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    Sanchis-Ojeda, R., Rappaport, S., Winn, J. N., Levine, A., Kotson, M. C., Latham, D. W., & Buchhave, L. A. (2013). Transits and occultations of an earth-sized planet in an 8.5 hr orbit. Astrophysical Journal, 774(1), [54]. https://doi.org/10.1088/0004-637X/774/1/54