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Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cygnus[1] |
Right ascension | 20h 00m 24.5657s[2] |
Declination | +45° 45′ 43.763″[2] |
Apparent magnitude (V) | 15[3] |
Characteristics | |
Spectral type | G0V~G0IV[4] |
Astrometry | |
Proper motion (μ) | RA: −0.956(18) mas/yr[2] Dec.: 8.241(19) mas/yr[2] |
Parallax (π) | 0.8719 ± 0.0163 mas[2] |
Distance | 3,740 ± 70 ly (1,150 ± 20 pc) |
Details | |
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 |
Other designations | |
Database references | |
SIMBAD | data |
KIC | data |
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.
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]
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🜨 |