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    • The distribution of transit durations for Kepler planet candidates and implications for their orbital eccentricities 

      Moorhead, A.V.; Ford, E.B.; Morehead, R.C.; Rowe, J.; Caldwell, D.A.; Jenkins, J.M.; Li, J.; Quintana, E.; Borucki, W.J.; Bryson, S.T.; Koch, D.G.; Jenkins, J.M.; Li, J.; Lissauer, J.J.; Quintana, E.; Batalha, N.M.; Fabrycky, D.C.; Gautier, T.N.; Holman, M.J.; Quinn, S.N.; Ragozzine, D.; Torres, G.; Lucas, P.W.; Marcy, G.W.; Shporer, A.; Still, M.; Shporer, A. (2011-11-01)
      Doppler planet searches have discovered that giant planets follow orbits with a wide range of orbital eccentricities, revolutionizing theories of planet formation. The discovery of hundreds of exoplanet candidates by NASA's ...