Artist's impression of the Kepler-452 and Kepler-186 systems compared to the inner Solar System, with their respective habitable zones shown. | |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cygnus |
Right ascension | 19h 44m 00.8861s[1] |
Declination | +44° 16′ 39.171″[1] |
Apparent magnitude (V) | 13.426[2] |
Characteristics | |
Evolutionary stage | Main sequence |
Spectral type | G2V[3] |
Astrometry | |
Proper motion (μ) | RA: 9.987(13) mas/yr[1] Dec.: 8.943(14) mas/yr[1] |
Parallax (π) | 1.8053 ± 0.0103 mas[1] |
Distance | 1,810 ± 10 ly (554 ± 3 pc) |
Details | |
Mass | 1.037+0.054 −0.047 M☉ |
Radius | 1.11+0.15 −0.09 R☉ |
Luminosity | 1.2 L☉ |
Surface gravity (log g) | 4.32 ± 0.09 cgs |
Temperature | 5757 ± 85 K |
Metallicity [Fe/H] | 0.21 ± 0.09 dex |
Age | 6 ± 2 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
KIC | data |
Extrasolar Planets Encyclopaedia | data |
Kepler-452 is a G-type main-sequence star located about 1,810 light-years away from Earth[1] in the Cygnus constellation.[5] Although similar in temperature to the Sun, it is 20% brighter, 3.7% more massive and 11% larger.[6][7] Alongside this, the star is approximately six billion years old and possesses a high metallicity.[3]
Gaia DR3
was invoked but never defined (see the help page).Simbad
was invoked but never defined (see the help page).