
Kepler-61b - Wikipedia
Kepler-61b (also known by its Kepler Object of Interest designation KOI-1361.01) is a super-Earth exoplanet orbiting within parts of the habitable zone of the K-type main-sequence star Kepler …
Kepler-61 b - Science@NASA
2024年10月25日 · Kepler-61 b is a Neptune-like exoplanet that orbits a K-type star. Its mass is 5.27 Earths, it takes 59.9 days to complete one orbit of its star, and is 0.24861 AU from its …
开普勒61b - 维基百科,自由的百科全书
2024年9月29日 · 开普勒61b (Kepler-61b)是一颗于2013年发现的 太阳系外行星,母恒星是 开普勒61。 该行星是以侦测行星通过母恒星前方使母恒星光度下降的凌日法发现 [1]。 开普勒61b …
克卜勒61b - 维基百科,自由的百科全书
克卜勒61b(Kepler-61b)是一顆於2013年發現的太陽系外行星,母恆星是克卜勒61。 該行星是以偵測行星通過母恆星前方使母恆星光度下降的凌日法發現 [ 1 ] 。
Kepler-61 - Wikipedia
Kepler-61b is a super-Earth with a radius 2.15 times that of Earth, and orbits near the inner edge of the habitable zone. It has an eccentric orbit that takes it in and out and thus experiences …
Open Exoplanet Catalogue - Kepler-61 b
Kepler-61 b is a 2.15 Earth-radii transiting exoplanet. It was confirmed using a statistical argument: It is 30,000 times more likely that Kepler-61 b is a planet than a blend scenario. …
[1304.6726] Exoplanet Characterization by Proxy: a Transiting 2.15 …
2013年4月24日 · We present the validation and characterization of Kepler-61b: a 2.15 R_Earth planet orbiting near the inner edge of the habitable zone of a low-mass star. Our …
Exoplanet Characterization by Proxy for Kepler-61b: How a …
We present the validation and characterization of Kepler-61b: a 2.5 R_Earth planet orbiting near the inner edge of the habitable zone of a low-mass star. Our characterization of the host star …
Exoplanet Characterization by Proxy: A Transiting 2.15 R
We present the validation and characterization of Kepler-61b: a 2.15 R ⊕ planet orbiting near the inner edge of the habitable zone of a low-mass star. Our characterization of the host star …
Exoplanet Characterization by Proxy for Kepler-61b: How
2013年1月1日 · We present the validation and characterization of Kepler-61b: a 2.5 R_Earth planet orbiting near the inner edge of the habitable zone of a low-mass star. Our …