Astronomy:Kepler-31
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Short description: Star in the constellation Cygnus
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | [corvus][1] |
| Right ascension | 19h 36m 05.5270s[2] |
| Declination | +45° 51′ 11.106″[2] |
| Apparent magnitude (V) | 14.0[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[2] mas |
| 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. It is orbited by three known exoplanets. 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.
Planetary system
The three gas giant planets orbiting Kepler-31 were discovered in early 2011, albeit with large false alarm probability, and were confirmed in 2012.[5][6] The planets form a resonant chain, with orbital periods ratio 1:2:4, although 20% probability exists that these period ratios may be coincidental.[7]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | <6.8 MJ | 0.16 | 20.8613 | — | — | 0.38±0.07 RJ |
| c | <4.7 MJ | 0.26 | 42.6318 | — | — | 0.38±0.07 RJ |
| d | — | 0.39 | 87.648901±0.000801 | — | — | 0.407±0.099 RJ |
References
- ↑ "Cygnus – constellation boundary", The Constellations, International Astronomical Union, http://www.iau.org/public/constellations/#cyg, retrieved 2011-12-15
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G. Gaia DR2 record for this source at VizieR.
- ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 Kepler-31b, NASA Ames Research Center, http://kepler.nasa.gov/Mission/discoveries/kepler30b/, retrieved 2011-12-06
- ↑ 4.0 4.1 Schneider, Jean, Star: Kepler-23, http://exoplanet.eu/star.php?st=Kepler-31, retrieved 2011-12-06
- ↑ Lissauer, Jack J.; Ragozzine, Darin; Fabrycky, Daniel C.; Steffen, Jason H.; Ford, Eric B.; Jenkins, Jon M.; Shporer, Avi; Holman, Matthew J. et al. (2011), "Architecture and Dynamics of Kepler 'S Candidate Multiple Transiting Planet Systems", The Astrophysical Journal Supplement Series 197 (1): 8, doi:10.1088/0067-0049/197/1/8, Bibcode: 2011ApJS..197....8L
- ↑ Transit Timing Observations from Kepler: IV. Confirmation of 4 Multiple Planet Systems by Simple Physical Models
- ↑ Pichierri, Gabriele; Batygin, Konstantin; Morbidelli, Alessandro (2019), "The role of dissipative evolution for three-planet, near-resonant extrasolar systems", Astronomy & Astrophysics 625: A7, doi:10.1051/0004-6361/201935259, Bibcode: 2019A&A...625A...7P
- ↑ Planet Kepler-31 d at exoplanets.eu
Coordinates: 
19h 36m 05.523s, +45° 51′ 11.09″
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