Kepler-1652b (also known by its Kepler Objects of Interest designation KOI-2626.01) is a super-Earth exoplanet, orbiting within the habitable zone of the red dwarf Kepler-1652 about 822 light-years away in the Cygnus constellation.

2014年7月3日 · We use our high-resolution imaging to spatially resolve the stellar multiplicity of Kepler-296, KOI-2626, and KOI-3049, and develop a conversion to the Kepler photometry (Kp) from the F555W and F775W filters on WFC3/UVIS.

2013年2月6日 · The three planetary candidates highlighted in this study are Kepler Object of Interest (KOI) 1422.02, which is 90 percent the size of Earth in a 20-day orbit; KOI-2626.01, 1.4 times the size of Earth in a 38-day orbit; and KOI-854.01, 1.7 times the size of …

2013年2月6日 · The three habitable-zone planetary candidates identified in this study are Kepler Object of Interest (KOI) 1422.02, which is 90 percent the size of Earth in a 20-day orbit; KOI 2626.01, 1.4 times the size of Earth in a 38-day orbit; and KOI 854.01, 1.7 times the size of Earth in a 56-day orbit.

We found KOI-2626 to be a triple star system with a projected separation of 0.201’’ 110 AU) between the primary and secondary components and 0.161’’ 90 AU) between the primary and tertiary components.

Kepler-1652 b is an exoplanet orbiting the star Kepler-1652, located about 821.9 light-years (252.0 pc) away from Solar System. Its discovery was publicly announced on 2017. The host star Kepler-1652 has apparent magnitude of 10.2, with absolute magnitude of 3.2. It is 0.4 times more massive and 0.4 times bigger compared with our Sun.

Identifiers (2) : An access of full data is available using the icon Vizier near the identifier of the catalogue Kepler -1652b KOI -2626.01

2017年11月18日 · The exoplanet KOI-2626.01, which has been a rather well-known candidate for YEARS now, has been confirmed at Kepler-1652b. It's about 1.6 times the radius of Earth with a density of 9.9 g/cm^3, suggesting a mass of around 7.356 Me.

Kepler-1652b (also known by its Kepler Objects of Interest designation KOI-2626.01) is a super-Earth exoplanet, orbiting within the habitable zone of the red dwarf Kepler-1652 about 822 light-years away in the Cygnus constellation.

2014年7月3日 · Recently, Dressing & Charbonneau (2013) identified three candidate Earth-like planets inside the HZ of M-dwarf stars: (1) Kepler Object of Interest (KOI) 2626.01; (2) KOI 1422.02; and (3) KOI 854.01.