Kepler-32
Kepler-32 is an M-type main sequence star located about 1070 light years from Earth, in the constellation of Cygnus. Discovered in January 2012 by the Kepler spacecraft, it shows a 0.58 ± 0.05 solar mass (M☉), a 0.53 ± 0.04 solar radius (R☉), and temperature of 3900.0 K, making it half the mass and radius of the Sun, two-thirds its temperature and 5% its luminosity.
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Cygnus |
| Right ascension | 19h 51m 22.1742s |
| Declination | +46° 34′ 27.390″ |
| Apparent magnitude (V) | 16.0 |
| Characteristics | |
| Spectral type | M1V |
| Astrometry | |
| Proper motion (μ) | RA: −13.618±0.058 mas/yr Dec.: 19.646±0.068 mas/yr |
| Parallax (π) | 3.0595 ± 0.0322 mas |
| Distance | 1,070 ± 10 ly (327 ± 3 pc) |
| Details | |
| Mass | 0.58±0.05 M☉ |
| Radius | 0.53±0.04 R☉ |
| Surface gravity (log g) | 4.64 cgs |
| Temperature | 3900±200 K |
| Metallicity [Fe/H] | 0.00 dex |
| Rotation | 36.220±0.256 days |
| Other designations | |
| Database references | |
| SIMBAD | data |
| KIC | data |
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