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- Publications
- Influence
Kepler Planet-Detection Mission: Introduction and First Results
- W. J. Borucki, D. Koch, +68 authors A. Prša
- Geology, Medicine
- Science
- 19 February 2010
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,… Expand
SDSS-III: MASSIVE SPECTROSCOPIC SURVEYS OF THE DISTANT UNIVERSE, THE MILKY WAY, AND EXTRA-SOLAR PLANETARY SYSTEMS
- D. Eisenstein, D. Weinberg, +237 authors B. Zhao
- Physics
- 1 December 2007
Building on the legacy of the Sloan Digital Sky Survey (SDSS-I and II), SDSS-III is a program of four spectroscopic surveys on three scientific themes: dark energy and cosmological parameters, the… Expand
Architecture and Dynamics of Kepler's Candidate Multiple Transiting Planet Systems
- J. Lissauer, D. Ragozzine, +22 authors D. Sasselov
- Physics
- 2 February 2011
About one-third of the ~1200 transiting planet candidates detected in the first four months of Kepler data are members of multiple candidate systems. There are 115 target stars with two candidate… Expand
Characteristics of planetary candidates observed by Kepler, II: Analysis of the first four months of data
- W. J. Borucki, D. Koch, +63 authors L. Walkowicz
- Physics
- 2 February 2011
On 2011 February 1 the Kepler mission released data for 156,453 stars observed from the beginning of the science observations on 2009 May 2 through September 16. There are 1235 planetary candidates… Expand
A closely packed system of low-mass, low-density planets transiting Kepler-11
- J. Lissauer, D. Fabrycky, +36 authors J. Steffen
- Physics, Medicine
- Nature
- 1 February 2011
When an extrasolar planet passes in front of (transits) its star, its radius can be measured from the decrease in starlight and its orbital period from the time between transits. Multiple planets… Expand
Planet Occurrence within 0.25 AU of Solar-Type Stars from Kepler
We report the distribution of planets as a function of planet radius, orbital period, and stellar effective temperature for orbital periods less than 50 days around solar-type (GK) stars. These… Expand
KEPLER'S FIRST ROCKY PLANET: KEPLER-10b*
- N. Batalha, W. J. Borucki, +74 authors High Altitude Observatory
- Physics
- 3 February 2011
NASA's Kepler Mission uses transit photometry to determine the frequency of Earth-size planets in or near the habitable zone of Sun-like stars. The mission reached a milestone toward meeting that… Expand
Structure and Evolution of Nearby Stars with Planets. II. Physical Properties of ~1000 Cool Stars from the SPOCS Catalog
- G. Takeda, E. Ford, +11 authors S. S. Institute
- Physics
- 11 July 2006
We derive detailed theoretical models for 1074 nearby stars from the SPOCS (Spectroscopic Properties of Cool Stars) Catalog. The California and Carnegie Planet Search has obtained high-quality (R… Expand
Kepler-16: A Transiting Circumbinary Planet
- L. Doyle, J. A. Carter, +46 authors D. Fischer
- Physics, Medicine
- Science
- 15 September 2011
An exoplanet has been observed, comparable in size and mass to Saturn, that orbits a pair of stars. We report the detection of a planet whose orbit surrounds a pair of low-mass stars. Data from the… Expand
An abundance of small exoplanets around stars with a wide range of metallicities
- L. Buchhave, D. Latham, +26 authors S. Quinn
- Physics, Medicine
- Nature
- 21 June 2012
The abundance of heavy elements (metallicity) in the photospheres of stars similar to the Sun provides a ‘fossil’ record of the chemical composition of the initial protoplanetary disk. Metal-rich… Expand