Kepler-385
Kepler-385 (also designated KOI-2433) is an F-type main-sequence star located about 4,900 light-years (1,500 parsecs) away from Earth in the constellation of Cygnus. The star is 10% larger and 5% hotter than the Sun. The star has at least three, and potentially up to seven, exoplanets discovered orbiting it.
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Cygnus |
| Right ascension | 19h 37m 21.23819s |
| Declination | +50° 20′ 11.5477″ |
| Apparent magnitude (V) | 15.76 |
| Astrometry | |
| Proper motion (μ) | RA: 2.738 mas/yr Dec.: -5.398 mas/yr |
| Parallax (π) | 0.6597 ± 0.0183 mas |
| Distance | 4,900 ± 100 ly (1,520 ± 40 pc) |
| Details | |
| Mass | 0.99±0.03 M☉ |
| Radius | 1.09±0.05 R☉ |
| Surface gravity (log g) | 4.19±0.10 cgs |
| Temperature | 5835±64 K |
| Metallicity [Fe/H] | 0.010±0.037 dex |
| Other designations | |
| Database references | |
| SIMBAD | data |
The star has a mass of 1.05 solar masses, a radius of 1.157 solar radii, a temperature of 5829 Kelvin and a luminosity of 1.39 times the solar luminosity.
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