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Kepler-62b __NOTOC__
Kepler-62b is the innermost and the second smallest discovered exoplanet orbiting the star Kepler-62, with a diameter roughly 30% larger than Earth. It was found using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured. it is likely to have a temperature slighly higher than venus (around 500c) which could melt some types of metal. Its stellar flux is 70 ± 9 times Earth's.〔 == References ==
抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)』 ■ウィキペディアで「Kepler-62b」の詳細全文を読む
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