| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Cygnus |
| Right ascension | 19h 41m 40.2991s[1] |
| Declination | +51° 11′ 05.168″[1] |
| Apparent magnitude (V) | 13.036±0.006[2] |
| Characteristics | |
| Evolutionary stage | Main sequence |
| Spectral type | F?V[3] |
| Apparent magnitude (B) | 13.498±0.011[2] |
| Astrometry | |
| Proper motion (μ) | RA: −0.068(16) mas/yr[1] Dec.: −1.423(16) mas/yr[1] |
| Parallax (π) | 0.9932 ± 0.0126 mas[1] |
| Distance | 3,280 ± 40 ly (1,010 ± 10 pc) |
| Details | |
| Mass | 1.40+0.06 −0.08[3] M☉ |
| Radius | 1.57+0.20 −0.18[3] R☉ |
| Luminosity | 2.7+1.6 −0.8[4] L☉ |
| Surface gravity (log g) | 4.19±0.09[3] cgs |
| Temperature | 6421+76 −80[3] K |
| Metallicity [Fe/H] | 0.16+0.08 −0.04[3] dex |
| Rotation | 4.492±0.012 days[5] |
| Rotational velocity (v sin i) | 14.41±1.3[3] km/s |
| Age | 2.8+1.3 −1.2[4] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
Kepler-419 is an F-type main-sequence star located about 3,280 light years from Earth in the constellation Cygnus. It is located within the field of vision of the Kepler spacecraft, the satellite that NASA's Kepler Mission used to detect planets that may be transiting their stars. In 2012, a potential planetary companion in a very eccentric orbit was detected around this star,[4] but its planetary nature was not confirmed until 12 June 2014, when it was named Kepler-419b. A second planet was announced orbiting further out from the star in the same paper, named Kepler-419c.[3]
Gaia DR3 was invoked but never defined (see the help page).APASS DR9 was invoked but never defined (see the help page).Dawson2014 was invoked but never defined (see the help page).Dawson2012 was invoked but never defined (see the help page).McQuillan2013 was invoked but never defined (see the help page).Simbad was invoked but never defined (see the help page).