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 …

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.

The planetary system Kepler-1652 hosts at least one planet. This list shows all planetary and stellar components in the system. It gives a quick overview of the hierarchical architecture. This table lists all planets in the system Kepler-1652. This planet was discovered by Torres et al. 2017.

2014年7月3日 · Recently, Dressing & Charbonneau 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.

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.

KOI-2626.01. other query modes : Identifier query : Coordinate query : Criteria query : Reference query : Basic query : Script submission : TAP : Output options : Object types: Help: Query : KOI-2626.01 : Basic data : Kepler-1652b -- Extra-solar Planet The astronomical object called Kepler-1652b is a Extra-solar Planet ...

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

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.