Kepler Planet-Detection Mission: Introduction and First Results

@article{Borucki2010KeplerPM,
  title={Kepler Planet-Detection Mission: Introduction and First Results},
  author={William J. Borucki and David J. Koch and Gibor S. Basri and Natalie M. Batalha and Timothy M. Brown and Douglas A. Caldwell and J. Caldwell and J{\o}rgen Christensen-Dalsgaard and William D. Cochran and E. K. Devore and Edward Wood Dunham and Andrea K. Dupree and Thomas Gautier and John Charles Geary and Ronald L. Gilliland and A. D. Gould and Steve B. Howell and Jon M. Jenkins and Yoji Kondo and David W. Latham and Geoffrey W. Marcy and S{\o}ren Meibom and Hans Kjeldsen and Jack J. Lissauer and David G. Monet and David R. Morrison and Dimitar D. Sasselov and Jill Tarter and Alan P. Boss and Donald Eugene Brownlee and T. C. Owen and Derek L. Buzasi and David Charbonneau and Laurance R. Doyle and Jonathan J. Fortney and Eric B. Ford and Matthew J. Holman and Sara Seager and Jason H. Steffen and William F. Welsh and Jason F. Rowe and Howard Anderson and Lars A. Buchhave and David R. Ciardi and Lucianne M. Walkowicz and William Henry Sherry and Elliott P. Horch and Howard T. Isaacson and Mark E. Everett and Debra A. Fischer and Guillermo Torres and John Asher Johnson and Michael Endl and Phillip J. MacQueen and Stephen T. Bryson and Jessie Dotson and Michael Haas and Jeffrey Kolodziejczak and Jeffrey E. Van Cleve and Hema Chandrasekaran and Joseph D. Twicken and Elisa V. Quintana and Bruce D. Clarke and Christopher D.C. Allen and Jie Li and Haley Wu and Peter Tenenbaum and Ekaterina M. Verner and Frederick C. Bruhweiler and Jason W. Barnes and Andrej Pr{\vs}a},
  journal={Science},
  year={2010},
  volume={327},
  pages={977 - 980}
}
Detecting Distant Planets More than 400 planets have been detected outside the solar system, most of which have masses similar to that of the gas giant planet, Jupiter. Borucki et al. (p. 977, published online 7 January) summarize the planetary findings derived from the first six weeks of observations with the Kepler mission whose objective is to search for and determine the frequency of Earth-like planets in the habitable zones of other stars. The results include the detection of five new… 
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References

SHOWING 1-10 OF 12 REFERENCES
Kepler’s Optical Phase Curve of the Exoplanet HAT-P-7b
TLDR
The Kepler mission is performing at the level required to detect Earth-size planets orbiting solar-type stars, including data for the previously known giant transiting exoplanet HAT-P-7b, which shows a smooth rise and fall of light from the planet as it orbits its star, punctuated by a drop when the planet passes behind its star.
A planetary system around the millisecond pulsar PSR1257 + 12
MILLISECOND radio pulsars, which are old (∼109yr), rapidly rotating neutron stars believed to be spun up by accretion of matter from their stellar companions, are usually found in binary systems with
Exotic Earths: Forming Habitable Worlds with Giant Planet Migration
TLDR
This simulation of terrestrial planet growth during and after giant planet migration is applied to close-in giant planets thought to form far from their host stars and migrate inward, through the terrestrial planet zone, via torques with a massive gaseous disk.
Structure and evolution of super-Earth to super-Jupiter exoplanets - I. Heavy element enrichment in the interior
Aims. We examine the uncertainties in current planetary models and quantify their impact on the planet cooling histories and massradius relationships. Methods. These uncertainties include (i) the
Detection of transits of the nearby hot Neptune GJ 436 b
This Letter reports on the photometric detection of transits of the Neptune-mass planet orbiting the nearby M-dwarf star GJ 436. It is by far the closest, smallest, and least massive transiting
Confirmation of Earth-Mass Planets Orbiting the Millisecond Pulsar PSR B1257 + 12
TLDR
The unambiguous detection of this effect, after 3 years of systematic timing observations of PSR B1257+12 with the 305-meter Arecibo radiotelescope, constitutes irrefutable evidence that the first planetary system around a star other than the sun has been identified.
TrES-2 : The first transiting planet in the kepler field
We announce the discovery of the second transiting hot Jupiter discovered by the Trans-atlantic Exoplanet Survey. The planet, which we dub TrES-2, orbits the nearby star GSC 03549-02811 every 2.47063
HAT-P-7b: An Extremely Hot Massive Planet Transiting a Bright Star in the Kepler Field
We report on the latest discovery of the HATNet project: a very hot giant planet orbiting a bright ( -->V = 10.5) star with a small semimajor axis of -->a = 0.0377 ± 0.0005 AU. Ephemeris for the
Ocean planet or thick atmosphere: On the mass-radius relationship for solid exoplanets with massive atmospheres
The bulk composition of an exoplanet is commonly inferred from its average density. For small planets, however, the average density is not unique within the range of compositions. Variations of a
A Jupiter-mass companion to a solar-type star
The presence of a Jupiter-mass companion to the star 51 Pegasi is inferred from observations of periodic variations in the star's radial velocity. The companion lies only about eight million
...
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