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K2-72 c è il terzo pianeta orbitante attor … K2-72 c è il terzo pianeta orbitante attorno alla stella nana rossa K2-72 ed è stato il secondo ad essere scoperto nel 2016 con l'uso del telescopio spaziale Kepler durante la seconda parte della sua missione. Come il pianeta più esterno del sistema, K2-72 e, sembra trovarsi all'interno della zona abitabile della stella.interno della zona abitabile della stella.
, K2-72c是一顆環繞紅矮星K2-72的小體積太陽系外行星，距離地球約227.7光年。該行星被認為位於母恆星的適居帶內，因此表面可能有液態水存在。K2-72c的軌道週期15.2日，半徑大約是地球的86%。
, K2-72c ist ein kleiner Exoplanet, welcher … K2-72c ist ein kleiner Exoplanet, welcher um den 227,7 Lichtjahre entfernten Roten Zwerg K2-72 kreist. Der Exoplanet befindet sich in der habitablen Zone des Sternes. In dieser Zone kann Wasser auf dem Planeten vorkommen. K2-72c hat eine Umlaufbahn von 15,2 Tagen und eine Masse von 86 % der Erde.,2 Tagen und eine Masse von 86 % der Erde.
, K2-72c is a small exoplanet orbiting around the red dwarf star K2-72 approximately 227.7 light-years away. It is located in the inner edge of the habitable zone. K2-72c completes an orbit in 15.2 days, and it has a radius of only 86% of that of the Earth.
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| rdfs:comment |
K2-72c is a small exoplanet orbiting around the red dwarf star K2-72 approximately 227.7 light-years away. It is located in the inner edge of the habitable zone. K2-72c completes an orbit in 15.2 days, and it has a radius of only 86% of that of the Earth.
, K2-72c是一顆環繞紅矮星K2-72的小體積太陽系外行星，距離地球約227.7光年。該行星被認為位於母恆星的適居帶內，因此表面可能有液態水存在。K2-72c的軌道週期15.2日，半徑大約是地球的86%。
, K2-72c ist ein kleiner Exoplanet, welcher … K2-72c ist ein kleiner Exoplanet, welcher um den 227,7 Lichtjahre entfernten Roten Zwerg K2-72 kreist. Der Exoplanet befindet sich in der habitablen Zone des Sternes. In dieser Zone kann Wasser auf dem Planeten vorkommen. K2-72c hat eine Umlaufbahn von 15,2 Tagen und eine Masse von 86 % der Erde.,2 Tagen und eine Masse von 86 % der Erde.
, K2-72 c è il terzo pianeta orbitante attor … K2-72 c è il terzo pianeta orbitante attorno alla stella nana rossa K2-72 ed è stato il secondo ad essere scoperto nel 2016 con l'uso del telescopio spaziale Kepler durante la seconda parte della sua missione. Come il pianeta più esterno del sistema, K2-72 e, sembra trovarsi all'interno della zona abitabile della stella.interno della zona abitabile della stella.
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K2-72c
, K2-72 c
|
