Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Cygnus[1] |
Right ascension | 19h 41m 55.76712s[2] |
Declination | +48° 31′ 27.9998″[2] |
Apparent magnitude (V) | 14.769±0.206[3] |
Characteristics | |
Evolutionary stage | main sequence star |
Spectral type | G4V[citation needed] |
Apparent magnitude (J) | 13.550±0.023[4] |
Apparent magnitude (H) | 13.204±0.024[4] |
Apparent magnitude (K) | 13.138±0.035[4] |
Variable type | Planetary transit,[3] rotationally variable[4] |
Astrometry | |
Proper motion (μ) | RA: −5.092 mas/yr[2] Dec.: +5.839 mas/yr[2] |
Parallax (π) | 0.6462 ± 0.0165 mas[2] |
Distance | 5,000 ± 100 ly (1,550 ± 40 pc) |
Details[3] | |
Mass | 0.9700+0.0490 −0.0590 M☉ |
Radius | 0.9500+0.1660 −0.0790 R☉ |
Temperature | 5710.0+96.696 −111.431 K |
Metallicity [Fe/H] | −0.0100+0.1410 −0.1880 dex |
Age | 4.37+4.19 −2.59 Gyr |
Other designations | |
KOI-5856, KIC 11037818, 2MASS J19415577+4831280[4] | |
Database references | |
SIMBAD | data |
Kepler-1638 is a G-type main-sequence star located about 5,000 light years away in the constellation of Cygnus.[1] One known exoplanet has been found orbiting the star: Kepler-1638b.[5][6][7][8]As of January 2021, Kepler-1638 is the farthest star with a known exoplanet orbiting in the habitable zone.[9]
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