Simulations indicate Kepler-62f, Kepler-1126c and Kepler-1544b are fast rotators independent of eccentricity, Kepler-440b is tidally trapped, and Kepler-186f, Kepler-62e, Kepler-442b require unknown eccentricity values to classify.
Revisited mass-radius relations for exoplanets below 120M⊕
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Simulation of the spin evolution of some selected exoplanets and inferences on their climate
Simulations indicate Kepler-62f, Kepler-1126c and Kepler-1544b are fast rotators independent of eccentricity, Kepler-440b is tidally trapped, and Kepler-186f, Kepler-62e, Kepler-442b require unknown eccentricity values to classify.