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KEPLER: Search for Earth-Size Planets in the Habitable Zone

Published online by Cambridge University Press:  01 May 2008

William Borucki ,
David Koch ,
Natalie Batalha ,
Douglas Caldwell ,
Jorgen Christensen-Dalsgaard ,
William D. Cochran ,
Edward Dunham ,
Thomas N. Gautier ,
John Geary  and
Ronald Gilliland
...Show all authors
William Borucki
Affiliation:
NASA Ames Research Center, Moffett Field, CA 94035, USA
David Koch
Affiliation:
NASA Ames Research Center, Moffett Field, CA 94035, USA
Natalie Batalha
Affiliation:
San Jose State University, San Jose, CA, 95192, USA
Douglas Caldwell
Affiliation:
SETI Institute, Mountain View, CA, 94043, USA
Jorgen Christensen-Dalsgaard
Affiliation:
University of Aarhus, Denmark
William D. Cochran
Affiliation:
University of Texas at Austin, Austin, TX, 78712, USA
Edward Dunham
Affiliation:
Lowell Observatory, Flagstaff, AZ, 86001, USA
Thomas N. Gautier
Affiliation:
Jet Propulsion Laboratory, Pasadena, CA, 91109, USA
John Geary
Affiliation:
Smithsonian Astrophysical Observatory, Cambridge, MA, 02138, USA
Ronald Gilliland
Affiliation:
Space Telescope Science Institute, Baltimore, MD, 21218, USA
Jon Jenkins
Affiliation:
SETI Institute, Mountain View, CA, 94043, USA
Hans Kjeldsen
Affiliation:
Lowell Observatory, Flagstaff, AZ, 86001, USA
Jack J. Lissauer
Affiliation:
NASA Ames Research Center, Moffett Field, CA 94035, USA
Jason Rowe
Affiliation:
NASA Ames Research Center, Moffett Field, CA 94035, USA
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Abstract

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The Kepler Mission is a space-based mission whose primary goal is to determine the frequency of Earth-size and larger planets in the habitable zone of solar-like stars. The mission will monitor more than 100,000 stars for patterns of transits with a differential photometric precision of 20 ppm at V = 12 for a 6.5 hour transit. It will also provide asteroseismic results on several thousand dwarf stars. It is specifically designed to continuously observe a single field of view of greater than 100 square degrees for 3.5 or more years.

This paper provides a short overview of the mission, a brief history of the mission development, expected results, new investigations by the recently chosen Participating Scientists, and the plans for the Guest Observer and Astrophysical Data Programs.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S253: Transiting Planets , May 2008 , pp. 289 - 299
Copyright
Copyright © International Astronomical Union 2009

References

Borucki, W. J. & Summers, A. L. 1984, Icarus 58, 121CrossRefGoogle Scholar
Borucki, W. J., Allen, L. E., Taylor, S. W., Torbet, E. B., Schaefer, A. R., & Fowler J. 1987, in: Second Workshop on Improvements to PhotometryGoogle Scholar
Borucki, W. J., Torbet, E. B., & Phan P. C. 1988, in: Proceedings of the Fiber Optics in Astronomy ConferenceGoogle Scholar
Borucki, W. J., Caldwell, D., Koch D, Jenkins, J., & Ninkov Z. 1999, In: Backmann, D. (ed.), Proceedings of the NStars WorkshopGoogle Scholar
Borucki, W. J., Caldwell, D., Koch, D. G., Webster, L. D., Jenkins, J. M., Ninkov, Z., & Showen R. 2001, PASP 113, 439CrossRefGoogle Scholar
Borucki, W. J., Koch, D. G., Lissauer, J. J., Basri, G. B., Caldwell, J. J., Cochran, W. D., Dunham, E. W., Geary, J. C., Latham, D. W., Gilliland, R. L., Caldwell, D. A., Jenkins, J. M., & Kondo Y. 2003, in Blades, J. C. & Siegmund, O. H. W. (eds.) Future EUV/UV and Visible Space Astrophysics Missions and Instrumentation Proc. SPIE 4854, p. 129Google Scholar
Borucki, W. J., Koch, D. G., Basri, G. B., Batalha, N., Brown, T. M., Caldwell, D. A., Christensen-Dalsgaard, J., Cochran, W. D., Dunham, E. W., Gautier, T. N., Geary, J. C., Gilliland, R. L., Jenkins J. M. Kondo Y. Latham, D. W., Lissauer, J. J., & Monet D. 2007, in Sun, Y.-S., Mello, S. Ferraz & Zhou, J.-L. (eds.) Exoplanets: Detection, Formation and Dynamics Proc. IAU Symp. 249, p. 17CrossRefGoogle Scholar
Brown, T. M. & Gilliland, R. L. 1994, ARAA, 32, 37CrossRefGoogle Scholar
Charbonneau, D., Brown, T. M., Latham, D. W., & Mayor, M. 2000, ApJ 529, L45CrossRefGoogle Scholar
Christensen-Dalsgaard, J., Arentoft, T., Brown, T. M., Gilliland, R. L., Kjeldsen, H., Borucki, W. J., & Koch, D. 2008, in Gizon, L. & Roth, M. (eds.) Helioseismology, Asteroseismology and the MHD Connections Proc. HELAS II International Conference, (Göttingen, J. Phys. Conf. Ser.), in pressGoogle Scholar
Granados, A. F. & Borucki, W. J., (eds.) 1994 Astrophysical Science with a Spaceborne Photometric Telescope NASA Conf.Publ. 10148 (Mt View)Google Scholar
Kasting, J. F., Whitmire, D. P., & Reynolds, R. T. 1993, Icarus 101, 108CrossRefGoogle Scholar
Koch, D. G., Borucki, W., Dunham, E., Jenkins, J., Webster, L., & Witteborn, F. 2000, in: UV, Optical and IR Space Telescopes and Instruments SPIE Conference 4013 (Munich: SPIE)Google Scholar
Koch, D. G., Borucki, W., Basri, G., Brown, T., Caldwell, D., Christensen-Dalsgaard, J., Cochran, W., Dunham, E., Gautier, T., Geary, J., Gilliland, R., Jenkins, J., Kondo, Y., Latham, D., Lissauer, J., & Monet., D. 2006, ApSS, 304, 389Google Scholar
Marcy, G. 2007, in: Kalas, P. (ed) In the Spirit of Bernard Lyot: The Direct Detection of Planets and Circumstellar Disks in the 21st Century, 21Google Scholar
Marcy, G. W. & Butler, R. P. 1996, ApJ 464, L147CrossRefGoogle Scholar
Mayor, M. & Queloz, D. 1995, Nature, 378, 355CrossRefGoogle Scholar
Rivera, E. J., Lissauer, J. J., Butler, R. P., Marcy, G. W., Vogt, S. S., Fischer, D. A., Brown, T. M., Laughlin, G., & Henry, G. W. 2005, ApJ, 634, 625CrossRefGoogle Scholar
Robinson, L. B., Wei, M. Z., Borucki, W. J., Dunham, E. W., Ford, C. H., & Granados, A. F. 1995, PASP 107, 1094CrossRefGoogle Scholar
Rosenblatt, F. 1971, Icarus 14, 71CrossRefGoogle Scholar
Wolszczan, A., 1994, Science 264, 538CrossRefGoogle Scholar