WASP-35
WASP-35 is a G-type main-sequence star about 660 light-years away. The star's age cannot be well constrained, but it is probably older than the Sun. WASP-35 is similar in concentration of heavy elements compared to the Sun.
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Eridanus |
| Right ascension | 05h 04m 19.6324s |
| Declination | −06° 13′ 47.3761″ |
| Apparent magnitude (V) | 10.94 |
| Characteristics | |
| Spectral type | G0V |
| Astrometry | |
| Radial velocity (Rv) | 16.96 km/s |
| Proper motion (μ) | RA: 20.664 mas/yr Dec.: 10.822 mas/yr |
| Parallax (π) | 4.9167 ± 0.0409 mas |
| Distance | 663 ± 6 ly (203 ± 2 pc) |
| Details | |
| Mass | 1.06±0.08 M☉ |
| Radius | 1.09±0.02 R☉ |
| Surface gravity (log g) | 4.39±0.02 cgs |
| Temperature | 6072±62 K |
| Metallicity [Fe/H] | 0.01±0.05 dex |
| Rotational velocity (v sin i) | 2.4±0.6 km/s |
| Age | 5.0±1.2 Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
The star has no detectable starspot activity. An imaging survey in 2015 found no detectable stellar companions, although a spectroscopic survey in 2016 yielded a suspected red dwarf companion with a temperature of 3800±1100 K.
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