| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Cygnus |
| Right ascension | 19h 37m 59.2726s[2] |
| Declination | +46° 41′ 22.953″[2] |
| Characteristics | |
| Spectral type | G / G[3] |
| Variable type | Algol[4] |
| Astrometry | |
| Proper motion (μ) | RA: −2.280(30) mas/yr[2] Dec.: −8.305(33) mas/yr[2] |
| Parallax (π) | 0.5248 ± 0.0260 mas[2] |
| Distance | 6,200 ± 300 ly (1,910 ± 90 pc) |
| Orbit[4] | |
| Period (P) | 20.73 d |
| Semi-major axis (a) | 0.176 au |
| Eccentricity (e) | 0.16 |
| Inclination (i) | 89.44° |
| Details[5] | |
| Kepler-35A | |
| Mass | 0.8877 M☉ |
| Radius | 1.0284 R☉ |
| Luminosity | 0.94 L☉ |
| Surface gravity (log g) | 4.3623 cgs |
| Temperature | 5,606 K |
| Metallicity | -0.13 |
| Kepler-35B | |
| Mass | 0.8094 M☉ |
| Radius | 0.7861 R☉ |
| Luminosity | 0.41 L☉ |
| Surface gravity (log g) | 4.5556 cgs |
| Temperature | 5,202 K |
| Metallicity | -0.13 |
| Age | 8-12 Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
| KIC | data |
Kepler-35 is a binary star system in the constellation of Cygnus. These stars, called Kepler-35A and Kepler-35B have masses of 89% and 81% solar masses respectively, and both are assumed to be of spectral class G. They are separated by 0.176 AU, and complete an eccentric orbit around a common center of mass every 20.73 days.[5]
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