Planet occurrence within 0.25AU 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 results are based on the 1235 planets (formally "planet candidates") from the Kepler mission tha...
Main Authors: | Seager, Sara, Rogers, Leslie Anne |
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Other Authors: | Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences |
Format: | Article |
Language: | en_US |
Published: |
IOP Publishing
2012
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Online Access: | http://hdl.handle.net/1721.1/74190 https://orcid.org/0000-0003-0638-3455 https://orcid.org/0000-0002-6892-6948 |
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