Kepler-167

Kepler-167 is a K-type main-sequence star located about 1,119 light-years (343 pc) away from the Solar System in the constellation of Cygnus. The star has about 78% the mass and 75% the radius of the Sun, and a temperature of 4,884 K (4,611 °C; 8,332 °F). It hosts a system of four known exoplanets. There is also a companion red dwarf star at a separation of about 700 AU, with an estimated orbital period of over 15,000 years.

Kepler-167
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 19h 30m 38.02619s
Declination +38° 20 43.4372
Apparent magnitude (V) 14.284±0.126
Characteristics
Evolutionary stage Main sequence
Spectral type K3-K4 + M4V
Apparent magnitude (V) 14.284±0.126
Apparent magnitude (G) 13.988±0.003
Apparent magnitude (J) 12.446±0.022
Apparent magnitude (H) 11.974±0.023
Apparent magnitude (K) 11.832±0.022
Astrometry
Radial velocity (Rv)−26.79±2.21 km/s
Proper motion (μ) RA: 15.097 mas/yr
Dec.: 36.352 mas/yr
Parallax (π)2.9157 ± 0.0131 mas
Distance1,119 ± 5 ly
(343 ± 2 pc)
Absolute magnitude (MV)6.53±0.12
Details
Mass0.777+0.034
−0.031
 M
Radius0.749±0.020 R
Luminosity (bolometric)0.289+0.017
−0.020
 L
Surface gravity (log g)4.579+0.027
−0.025
 cgs
Temperature4884+69
−75
 K
Metallicity [Fe/H]0.020±0.067 dex
Rotational velocity (v sin i)<2 km/s
Age7.1+4.4
−4.6
 Gyr
Other designations
Kepler-167, KOI-490, KIC 3239945, TIC 137686948, 2MASS J19303802+3820434
Database references
SIMBADdata
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