Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cygnus |
Right ascension | 19h 48m 06.77346s [1] |
Declination | +48° 12′ 30.9642″ [1] |
Apparent magnitude (V) | 12.70 |
Characteristics | |
Spectral type | G2V [2] |
Apparent magnitude (B) | 13.34 [2] |
Apparent magnitude (V) | 12.70 [2] |
Apparent magnitude (J) | 11.39 [2] |
Apparent magnitude (K) | 11.06 [2] |
Astrometry | |
Radial velocity (Rv) | 5.64423 ± 4.5 × 10–4 [2] km/s |
Proper motion (μ) |
RA: −9.393
mas/
yr
[1] Dec.: 0.158 mas/ yr [1] |
Parallax (π) | 1.9259 ± 0.0092 mas [1] |
Distance | 1,694 ± 8
ly (519 ± 2 pc) |
Details | |
Mass | 1.238±0.029 [2] M☉ |
Radius | 1.447±0.014 [2] R☉ |
Surface gravity (log g) | (Spectroscopic) 4.28 ± 0.10 cgs (Asteroseismic) 4.210 ± 0.013 [2] cgs |
Temperature | 5854±61 [2] K |
Metallicity [Fe/H] | 0.321±0.065 [2] dex |
Rotational velocity (v sin i) | 3.6±0.5 [2] km/s |
Age | 4.29+0.70 −0.56 [2] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Kepler-107 is a star about 1,694 light-years (519 parsecs) away in the constellation Cygnus. It is a spectral type G2 star. An imaging survey in 2016 failed to find any stellar companions to it. [4]
Kepler-107 has four known planets discovered in 2014. [5] [6] [7] [8] A giant impact is the likely origin of two planets in the system. [2] Kepler-107 c is more than twice as dense (about 12.6 g cm−3) as the innermost exoplanet Kepler-107 b (about 5.3 g cm−3). [2]
Companion (in order from star) |
Mass |
Semimajor axis ( AU) |
Orbital period ( days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 3.8+1.8 −1.7 M🜨 |
0.04544±0.00036 | 3.1800218±0.0000029 | <0.10 | 89.05±0.67 ° | 1.536±0.025 R🜨 |
c | 10.0±2.0 M🜨 | 0.06064±0.00048 | 4.901452±0.0 | <0.080 | 89.49+0.34 −0.44 ° |
1.597±0.026 R🜨 |
d | <7.7 M🜨 | 0.08377±0.00065 | 7.95839±0.00012 | <0.11 | 87.55+0.64 −0.48 ° |
0.860±0.060 R🜨 |
e | 14.1±3.3 M🜨 | 0.12638±0.00099 | 14.749143±0.000019 | <0.10 | 89.67±0.22 ° | 2.903±0.035 R🜨 |