Kepler-67
Appearance
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cygnus |
Right ascension | 19h 36m 36.8092s[1] |
Declination | +46° 09′ 59.166″[1] |
Apparent magnitude (V) | 16.4 |
Characteristics | |
Spectral type | G9V |
Astrometry | |
Proper motion (μ) | RA: −3.424±0.093[1] mas/yr Dec.: −8.679±0.077[1] mas/yr |
Parallax (π) | 0.8580 ± 0.0508 mas[1] |
Distance | 3,800 ± 200 ly (1,170 ± 70 pc) |
Details | |
Mass | 0.865 ± 0.034 M☉ |
Radius | 0.778 ± 0.031 R☉ |
Temperature | 5331 ± 63 K K |
Metallicity [Fe/H] | 0.012 ± 0.003 dex |
Rotation | 10.464±0.014 days[2] |
Age | 1 ± 0.17 Gyr |
Other designations | |
KOI-2115[3] | |
Database references | |
SIMBAD | data |
Kepler-67 is a star with slightly less mass than the Sun in the NGC 6811 open cluster in the Cygnus constellation and has one confirmed planet, slightly smaller than Neptune, announced in 2013.
Planetary system
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 0.31 ± 0.06 MJ | 0.1171 ± 0.0015 | 15.7259 ± 0.00011 | — | — | 0.26 ± 0.014 RJ |
References
- ^ a b c d e 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.
- ^ McQuillan, A.; Mazeh, T.; Aigrain, S. (2013). "Stellar Rotation Periods of The Kepler objects of Interest: A Dearth of Close-In Planets Around Fast Rotators". The Astrophysical Journal Letters. 775 (1). L11. arXiv:1308.1845. Bibcode:2013ApJ...775L..11M. doi:10.1088/2041-8205/775/1/L11.
- ^ "Kepler-67". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 15 January 2018.