Kepler-1229

Kepler-1229 is a red dwarf star located about 870 light-years (270 pc) away from the Earth in the constellation of Cygnus. It is known to host a super-Earth exoplanet within its habitable zone, Kepler-1229b, which was discovered in 2016.

Kepler-1229
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 19h 49m 56.8076s
Declination +46° 59 48.1073
Apparent magnitude (V) 14.474
Characteristics
Evolutionary stage Main sequence
Spectral type M?V
B−V color index 1.48
Astrometry
Proper motion (μ) RA: 21.619±0.092 mas/yr
Dec.: −4.238±0.092 mas/yr
Parallax (π)3.7388 ± 0.0472 mas
Distance870 ± 10 ly
(267 ± 3 pc)
Details
Mass0.43 ± 0.05 M
Radius0.51 ± 0.03 R
Luminosity0.04784 L
Surface gravity (log g)4.75+0.029
−0.023
 cgs
Temperature3784 ± 39 K
Metallicity [Fe/H]–0.06 ± 0.1 dex
Rotation17.98±0.04 d
Age3.72+5.32
−2.07
 Gyr
Other designations
KIC 10027247, KOI-2418
Database references
SIMBADdata
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