The kepler mission: Astrophysics and eclipsing binaries

D. Koch, W. Borucki, G. Basri, T. Brown, D. Caldwell, J. Christensen-Dalsgaard, W. Cochran, E. Dunham, T. N. Gautier, J. Geary, R. Gilliland, J. Jenkins, Y. Kondo, D. Latham, J. Lissauer, D. Monet

Research output: Contribution to journalArticlepeer-review

6 Scopus citations


The Kepler Mission is a photometric space mission that will continuously observe a single 100 square degree field of view (FOV) of the sky of more than 100,000 stars in the Cygnus-Lyra region for four or more years with a precision of 14 parts per million (ppm) for a 6.5 hour integration including shot noise for a twelfth magnitude star. The primary goal of the mission is to detect Earth-size planets in the habitable zone of solar-like stars. In the process, many eclipsing binaries (EB) will also be detected. Prior to launch, the stellar characteristics will have been determined for all the stars in the FOV with K<14.5. As part of the verification process, stars with transits (about 5%) will need to have follow-up radial velocity observations performed to determine the component masses and thereby separate grazing eclipses caused by stellar companions from transits caused by planets. The result will be a rich database on EBs. The community will have access to the archive for uses such as for EB modeling of the high-precision light curves. A guest observer program is also planned for objects not already on the target list.

Original languageEnglish (US)
Pages (from-to)391-395
Number of pages5
JournalAstrophysics and Space Science
Issue number1-4
StatePublished - Aug 2006

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science


Dive into the research topics of 'The kepler mission: Astrophysics and eclipsing binaries'. Together they form a unique fingerprint.

Cite this