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Kepler-444 (or KOI-3158, KIC 6278762, 2MASS J19190052+4138043, BD+41°3306) [10] is a triple star system, estimated to be 11.2 billion years old (more than 80% of the age of the universe), [12] approximately 119 light-years (36 pc) away from Earth in the constellation Lyra.
Initially, two stars were discovered that were so close together that their atmospheres touched each other. Both stars take six hours to orbit each other.
Kepler-44, formerly known as KOI-204, is a star in the northern constellation of Cygnus. It is located at the celestial coordinates: Right Ascension 20 h 00 m 24.564 s, Declination +45° 45′ 43.71″. [5] With an apparent visual magnitude of 16, [3] this star is too faint to be seen with the naked eye.
Kepler-442b [1] [4] [5] (also known by its Kepler object of interest designation KOI-4742.01) is a confirmed near-Earth-sized exoplanet, likely rocky, orbiting within the habitable zone of the K-type main-sequence star [6] Kepler-442, about 1,196 light-years (367 pc) from Earth in the constellation of Lyra.
Kepler-445 is a red dwarf star located 401 light-years (123 parsecs) away in the constellation Cygnus. It hosts three known exoplanets , discovered by the transit method using data from the Kepler space telescope and confirmed in 2015. [ 6 ]
Kepler-442 is a K-type main-sequence star approximately 1,196 light years from Earth in the constellation Lyra.It is located within the field of vision of the Kepler spacecraft, the satellite that NASA's Kepler Mission used to detect planets that may be transiting their stars.
Kepler-440b (also known by its Kepler Object of Interest designation KOI-4087.01) is a confirmed super-Earth exoplanet orbiting within the habitable zone of Kepler-440, about 850 light-years (261 pc) from Earth. [1]
KIC 11145123 (sometimes mistakenly called Kepler 11145123 [9]), is a white hued star located in the northern constellation Cygnus, the swan.It has an apparent magnitude of 13.12, [2] making it readily visible in large telescopes, but not to the naked eye.