Kepler-62: A Five-Planet System with Planets of 1.4 and 1.6 Earth Radii in the Habitable Zone

@article{Borucki2013Kepler62AF,
  title={Kepler-62: A Five-Planet System with Planets of 1.4 and 1.6 Earth Radii in the Habitable Zone},
  author={W. Borucki and E. Agol and F. Fressin and L. Kaltenegger and J. Rowe and H. Isaacson and D. Fischer and N. Batalha and J. Lissauer and G. Marcy and D. Fabrycky and J. D{\'e}sert and S. Bryson and T. Barclay and F. Bastien and A. Boss and E. Brugamyer and L. Buchhave and C. Burke and D. Caldwell and J. Carter and D. Charbonneau and J. Crepp and J. Christensen-Dalsgaard and J. Christiansen and D. Ciardi and W. Cochran and E. Devore and L. Doyle and A. Dupree and M. Endl and M. Everett and E. Ford and J. Fortney and T. Gautier and J. Geary and A. Gould and M. Haas and C. Henze and A. Howard and S. Howell and D. Huber and J. Jenkins and H. Kjeldsen and R. Kolbl and J. Kolodziejczak and D. Latham and B. Lee and E. Lopez and F. Mullally and J. Orosz and A. Pr{\vs}a and E. Quintana and R. Sanchis-Ojeda and D. Sasselov and S. Seader and A. Shporer and J. Steffen and M. Still and P. Tenenbaum and S. Thompson and G. Torres and J. Twicken and W. Welsh and J. Winn},
  journal={Science},
  year={2013},
  volume={340},
  pages={587 - 590}
}
Two Small Habitable Planets NASA's Kepler space telescope was launched in 2009 with the goal of detecting planets the size of Earth in the habitable zone of Sun-like stars and determining the frequency of these planets. Using data from Kepler, Borucki et al. (p. 587, published online 18 April) report the detection of a five-planet system where all the planets are smaller than twice the size of Earth and where the two outermost planets orbit in the habitable zone of their star, defined as the… Expand
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