WASP-56
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Coma Berenices |
| Right ascension | 12h 13m 27.8908s |
| Declination | +23° 03′ 20.428″ |
| Apparent magnitude (V) | 11.48 |
| Characteristics | |
| Evolutionary stage | main sequence |
| Spectral type | G6V |
| Astrometry | |
| Radial velocity (Rv) | 5.97±0.80 km/s |
| Proper motion (μ) | RA: −36.695 mas/yr Dec.: 2.954 mas/yr |
| Parallax (π) | 3.0471±0.0162 mas |
| Distance | 1,070 ± 6 ly (328 ± 2 pc) |
| Details | |
| Mass | 1.107±0.024 M☉ |
| Radius | 1.112+0.026 −0.022 R☉ |
| Surface gravity (log g) | 4.45 ± 0.1 cgs |
| Temperature | 5600 ± 100 K |
| Metallicity [Fe/H] | 0.12±0.06 dex |
| Rotational velocity (v sin i) | 1.5 ± 0.9 km/s |
| Age | 6.2+3.0 −2.1 Gyr |
| Other designations | |
| Melotte 111 AV 561, TOI-1809, TIC 347329162, WASP-56, TYC 1986-1561-1, 2MASS J12132790+2303205 | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
WASP-56 is a sun-like star of spectral type G6 about 1,070 light-years away in the constellation of Coma Berenices. It has an apparent magnitude of 11.48. Observations at the Calar Alto Observatory using the lucky imaging technique detected a candidate companion star located 3.4 arcseconds away, however it was not known if this is an actual binary companion or an optical double. It was confirmed in 2019 using Gaia DR2 data.