May
2013
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2013Sci...340..587B
Authors
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Borucki, William J.
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Agol, Eric
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Fressin, Francois
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Kaltenegger, Lisa
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Rowe, Jason
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Isaacson, Howard
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Fischer, Debra
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Batalha, Natalie
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Lissauer, Jack J.
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Marcy, Geoffrey W.
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Fabrycky, Daniel
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Désert, Jean-Michel
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Bryson, Stephen T.
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Barclay, Thomas
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Bastien, Fabienne
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Boss, Alan
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Brugamyer, Erik
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Buchhave, Lars A.
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Burke, Chris
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Caldwell, Douglas A.
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Carter, Josh
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Charbonneau, David
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Crepp, Justin R.
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Christensen-Dalsgaard, Jørgen
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Christiansen, Jessie L.
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Ciardi, David
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Cochran, William D.
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DeVore, Edna
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Doyle, Laurance
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Dupree, Andrea K.
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Endl, Michael
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Everett, Mark E.
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Ford, Eric B.
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Fortney, Jonathan
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Gautier, Thomas N.
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Geary, John C.
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Gould, Alan
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Haas, Michael
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Henze, Christopher
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Howard, Andrew W.
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Howell, Steve B.
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Huber, Daniel
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Jenkins, Jon M.
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Kjeldsen, Hans
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Kolbl, Rea
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Kolodziejczak, Jeffery
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Latham, David W.
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Lee, Brian L.
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Lopez, Eric
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Mullally, Fergal
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Orosz, Jerome A.
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Prsa, Andrej
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Quintana, Elisa V.
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Sanchis-Ojeda, Roberto
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Sasselov, Dimitar
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Seader, Shawn
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Shporer, Avi
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Steffen, Jason H.
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Still, Martin
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Tenenbaum, Peter
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Thompson, Susan E.
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Torres, Guillermo
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Twicken, Joseph D.
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Welsh, William F.
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Winn, Joshua N.
Abstract
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We present the detection of five planets—Kepler-62b, c, d, e, and f—of size 1.31, 0.54, 1.95, 1.61 and 1.41 Earth radii (R⊕), orbiting a K2V star at periods of 5.7, 12.4, 18.2, 122.4, and 267.3 days, respectively. The outermost planets, Kepler-62e and -62f, are super-Earth-size (1.25 R⊕ < planet radius ≤ 2.0 R⊕) planets in the habitable zone of their host star, respectively receiving 1.2 ± 0.2 times and 0.41 ± 0.05 times the solar flux at Earth’s orbit. Theoretical models of Kepler-62e and -62f for a stellar age of ~7 billion years suggest that both planets could be solid, either with a rocky composition or composed of mostly solid water in their bulk.
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