astro.wikisort.org - StarKepler-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.
Star in the constellation Cygnus
Kepler-44
Observation data
Epoch J2000 Equinox J2000 |
| Constellation |
Cygnus[1] |
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| Right ascension |
20h 00m 24.5657s[2] |
| Declination |
+45° 45′ 43.763″[2] |
| Apparent magnitude (V) |
15[3] |
| Characteristics |
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| Spectral type |
G0V~G0IV[4] |
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| Astrometry |
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| Proper motion (μ) | RA: −0.943±0.038[2] mas/yr
Dec.: 8.225±0.038[2] mas/yr |
| Parallax (π) | 0.8136 ± 0.0229 mas[2] |
| Distance | 4,000 ± 100 ly
(1,230 ± 30 pc) |
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| Details |
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| Mass | 1.19±0.10[3] M☉ |
| Radius | 1.52±0.09[3] R☉ |
| Temperature | 5757±134[3] K |
| Metallicity [Fe/H] | 0.26±0.10[3] dex |
| Rotational velocity (v sin i) | 5.5±1.5[3] km/s |
| Age | 6.95[3] Gyr |
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| Other designations |
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KOI-204, KIC 9305831, 2MASS J20002456+4545437 |
| Database references |
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| SIMBAD | data |
| KIC | data |
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]
The Kepler-44 planetary system[4]
Companion
(in order from star) |
Mass |
Semimajor axis
(AU) |
Orbital period
(days) |
Eccentricity |
Inclination |
Radius |
| b |
1.02 MJ |
0.0455 |
3.246774 |
— |
— |
13 R🜨 |
References
- "Cygnus – constellation boundary", The Constellations, International Astronomical Union, retrieved 2011-12-15
- Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- Kepler-44b, NASA Ames Research Center, archived from the original on 2015-09-14, retrieved 2011-12-06
- Schneider, Jean, "Star: Kepler-44", Extrasolar Planets Encyclopaedia, Paris Observatory, 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
На других языках
- [en] Kepler-44
[ru] KOI-204
KOI-204 (или Kepler-44) — звезда в созвездии Лебедя. Находится на расстоянии около 7338 световых лет от Солнца. Вокруг звезды обращается, как минимум, одна планета.
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