Kepler-31
Appearance
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | [corvus][1] |
Right ascension | 19h 36m 05.5270s[2] |
Declination | +45° 51′ 11.106″[2] |
Apparent magnitude (V) | [3] |
Characteristics | |
Spectral type | G5[4] |
Astrometry | |
Proper motion (μ) | RA: −1.017±0.043[2] mas/yr Dec.: −7.344±0.044[2] mas/yr |
Parallax (π) | 0.5722 ± 0.0230 mas[2] |
Distance | 5,700 ± 200 ly (1,750 ± 70 pc) |
Details | |
Mass | 1.21 ± 0.17[3] M☉ |
Radius | 1.22 ± 0.24[3] R☉ |
Luminosity | 0.79 ± 0.04[3] L☉ |
Temperature | 6340 ± 200[3] K |
Metallicity [Fe/H] | –0.076 ± 0.400[3] dex |
Other designations | |
Database references | |
SIMBAD | data |
KIC | data |
Kepler-31 is a star in the northern constellation of Cygnus, the swan, that is orbited by a planet found to be unequivocally within the star's habitable zone. It is located at the celestial coordinates: Right Ascension 19h 36m 05.5270s, Declination +45° 51′ 11.106″.[2] With an apparent visual magnitude of 14.0,[3] this star is too faint to be seen with the naked eye.
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 6.8 MJ | 0.16 | 20.8613 | — | — | 4.1 R🜨 |
c | 4.7 MJ | 0.26 | 42.6318 | — | — | 4.1 R🜨 |
References
- ^ "Cygnus – constellation boundary", The Constellations, International Astronomical Union, retrieved 2011-12-15
- ^ a b c d e f 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.
- ^ a b c d e f g Kepler-31b, NASA Ames Research Center, retrieved 2011-12-06
- ^ a b Schneider, Jean, "Star: Kepler-23", Extrasolar Planets Encyclopaedia, Paris Observatory, archived from the original on 2012-05-05, retrieved 2011-12-06