Star in the constellation Cygnus
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 20h 00m 24.564s , 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.
Planetary system
The Kepler spacecraft detected a transiting planet candidate around this star that was confirmed by radial velocity measurements taken by the SOPHIE spectrograph mounted on the 1.93 m telescope at the Haute-Provence Observatory .[ 6]
The planet is likely to be tidally locked to the parent star. In 2015, the planetary nightside temperature was estimated to be equal to 2347+149 −280 K .[ 7]
References
^ "Cygnus – constellation boundary", The Constellations , International Astronomical Union , retrieved 2011-12-15
^ a b c d Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties" . Astronomy and Astrophysics . 674 : A1. arXiv :2208.00211 . Bibcode :2023A&A...674A...1G . doi :10.1051/0004-6361/202243940 . S2CID 244398875 .
Gaia DR3 record for this source at VizieR .
^ a b c d e f g h Kepler-44b , NASA Ames Research Center , archived from the original on 2015-09-14, retrieved 2011-12-06
^ a b Schneider, Jean, "Star: Kepler-44" , Extrasolar Planets Encyclopaedia , archived from the original on 2014-03-04, retrieved 2011-12-06
^ "Kepler Discoveries" . 2011-12-05. Archived from the original on 2010-05-27.
^ Bonomo, A. S.; et al. (2012). "SOPHIE velocimetry of Kepler transit candidates. V. The three hot Jupiters KOI-135b, KOI-204b, and KOI-203b (alias Kepler-17b)" . Astronomy and Astrophysics . 538 . A96. arXiv :1110.5462 . Bibcode :2012A&A...538A..96B . doi :10.1051/0004-6361/201118323 . S2CID 118528032 .
^ A Comprehensive Study of Kepler Phase Curves and Secondary Eclipses:Temperatures and Albedos of Confirmed Kepler Giant Planets