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  2. Kepler-22b - Wikipedia

    en.wikipedia.org/wiki/Kepler-22b

    Kepler-22b (also known by its Kepler Object of Interest designation KOI-087.01) is an exoplanet orbiting within the habitable zone of the Sun-like star Kepler-22. It is located about 640 light-years (200 parsecs ) from Earth in the constellation of Cygnus .

  3. Kepler space telescope - Wikipedia

    en.wikipedia.org/wiki/Kepler_space_telescope

    The Kepler Input Catalog is a publicly searchable database of roughly 13.2 million targets used for the Kepler Spectral Classification Program and the Kepler mission. [ 236 ] [ 237 ] The catalog alone is not used for finding Kepler targets, because only a portion of the listed stars (about one-third of the catalog) can be observed by the ...

  4. K2-18b - Wikipedia

    en.wikipedia.org/wiki/K2-18b

    K2-18b, also known as EPIC 201912552 b, is an exoplanet orbiting the red dwarf K2-18, located 124 light-years (38 pc) away from Earth. The planet is a sub-Neptune about 2.6 times the radius of Earth , with a 33-day orbit within the star's habitable zone .

  5. Kepler-22 - Wikipedia

    en.wikipedia.org/wiki/Kepler-22

    Kepler-22 is a Sun-like star in the northern constellation of Cygnus, the swan, that is orbited by at least 1 planet found to be unequivocally within the star's habitable zone. It is located at the celestial coordinates : Right Ascension 19 h 16 m 52.2 s , Declination +47° 53′ 3.9″. [ 2 ]

  6. TrES-2b - Wikipedia

    en.wikipedia.org/wiki/TrES-2b

    The first important result from the Kepler Mission about TrES-2b is an extremely low geometric albedo measured in 2011, making it the darkest known exoplanet. [5] If the entire day–night contrast were due to geometric albedo, it would be 2.53%, but modeling suggests that much of this is dayside emission and the true albedo is much lower. It ...

  7. List of exoplanets discovered by the Kepler space telescope ...

    en.wikipedia.org/wiki/List_of_exoplanets...

    Planet Disc­overy method Mass (M J) Radius (R J) Density (g/cm 3) Orbital period ()Semimajor axis ()Orbital eccentricity Year of con­firm­ation Ref. Earth (for reference): 0.003 15

  8. Transit-timing variation - Wikipedia

    en.wikipedia.org/wiki/Transit-timing_variation

    Transit-timing variation was first convincingly detected for planets Kepler-9b and Kepler-9c [13] and gained popularity by 2012 for confirming exoplanet discoveries. [14] TTV can also be used to indirectly measure the mass of the exoplanets in compact, multiple-planet systems and/or system whose planets are in resonant chains.

  9. GSC 03549-02811 - Wikipedia

    en.wikipedia.org/wiki/GSC_03549-02811

    An image from Kepler with TrES-2b and another point of interest outlined. Celestial north is towards the lower left corner. In March 2009 NASA launched the Kepler spacecraft. This spacecraft was a dedicated mission to discover extrasolar planets by the transit method from solar orbit.