Kepler-18
Appearance
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cygnus |
Right ascension | 19h 52m 19.0688s[1] |
Declination | +44° 44′ 46.808″[1] |
Apparent magnitude (V) | 14.0 |
Characteristics | |
Spectral type | G7 |
Astrometry | |
Proper motion (μ) | RA: −1.432±0.031[1] mas/yr Dec.: −20.313±0.028[1] mas/yr |
Parallax (π) | 2.2804 ± 0.0168 mas[1] |
Distance | 1,430 ± 10 ly (439 ± 3 pc) |
Details[2] | |
Mass | 0.972 ± 0.042 M☉ |
Radius | 1.108 ± 0.051 R☉ |
Luminosity | 0.93 L☉ |
Surface gravity (log g) | 4.32 ± 0.12 cgs |
Temperature | 5383 ± 44 K |
Metallicity [Fe/H] | 0.19 ± 0.06 dex |
Rotational velocity (v sin i) | <4 km/s |
Age | 10.0 ± 2.3 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Kepler-18 is a star with almost the same mass as the Sun in the Cygnus constellation
Planetary system
The star is orbited by 3 confirmed planets, announced in 2011.[2]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 6.9 ± 3.4 M🜨 | 0.0447 ± 0.0006 | 3.504725 ± 0.000028 | — | 84.92 ± 0.26° | 2.00 ± 0.10 R🜨 |
c | 17.3 ± 1.9 M🜨 | 0.0752 ± 0.0011 | 7.6415716 | — | 87.68 ± 0.22° | 5.49 ± 0.26 R🜨 |
d | 16.4 ± 1.4 M🜨 | 0.1172 ± 0.0017 | 14.858941 | — | 88.07 ± 0.1° | 6.98 ± 0.33 R🜨 |
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 Data Release 2 catalog entry
- ^ a b c Cochran, William D.; et al. (2011). "Kepler 18-b, c, and d: A System Of Three Planets Confirmed by Transit Timing Variations, Lightcurve Validation, Spitzer Photometry and Radial Velocity Measurements". The Astrophysical Journal Supplement Series. 197: 7. arXiv:1110.0820. Bibcode:2011ApJS..197....7C. doi:10.1088/0067-0049/197/1/7. S2CID 16505452.
- ^ "Kepler-18". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 25 January 2018.
- ^ Montet, Benjamin T.; Johnson, John Asher (2013), "Model-Independent Stellar and Planetary Masses from Multi-Transiting Exoplanetary Systems", The Astrophysical Journal, 762 (2): 112, arXiv:1211.4028v1, doi:10.1088/0004-637X/762/2/112, S2CID 29261765