Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aquarius |
Right ascension | 22h 04m 48.7262s[1] |
Declination | −12° 01′ 07.999″[1] |
Apparent magnitude (V) | 11.986 |
Characteristics | |
Evolutionary stage | Main sequence |
Spectral type | G9V |
Astrometry | |
Radial velocity (Rv) | −26.56(47)[1] km/s |
Proper motion (μ) | RA: 15.074(20) mas/yr[1] Dec.: −41.467(20) mas/yr[1] |
Parallax (π) | 3.7010 ± 0.0201 mas[1] |
Distance | 881 ± 5 ly (270 ± 1 pc) |
Details | |
Mass | 1.11 (± 0.05) M☉ |
Radius | 1.16 (± 0.26) R☉ |
Luminosity | ~1.16 L☉ |
Surface gravity (log g) | 4.354 (± 0.086) cgs |
Temperature | 5576 (± 68) K |
Metallicity [Fe/H] | +0.36 (± 0.05) dex |
Rotation | 32.5±3.9 d[2] |
Age | 6.5 +2.6 −1.2 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
WASP-47 is a star similar in size and brightness to the Sun about 881 light-years away in the constellation Aquarius. It lies within the Kepler K2 campaign field 3. It was first noticed to have a hot Jupiter exoplanet orbiting every 4 days in 2012 by the Wide Angle Search for Planets (WASP) team.[4] While it was thought to be a typical hot Jupiter system, three more planets were found in 2015:[5][6] an outer gas giant within the habitable zone, a hot Neptune exterior to the hot Jupiter's orbit and a super-Earth interior to the hot Jupiter's orbit. WASP-47 is the only planetary system known to have both planets near the hot Jupiter and another planet much further out.[7]
Gaia DR3
was invoked but never defined (see the help page).Simbad
was invoked but never defined (see the help page).Hellier2012
was invoked but never defined (see the help page).Neveu-VanMalle2016
was invoked but never defined (see the help page).