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Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Virgo[1] |
Right ascension | 13h 35m 01.9538s[2] |
Declination | −17° 30′ 12.528″[2] |
Apparent magnitude (V) | 11.75[3] |
Characteristics | |
Evolutionary stage | Main sequence[4] |
Spectral type | G1[4] |
Astrometry | |
Radial velocity (Rv) | −3.31±0.87[2] km/s |
Proper motion (μ) | RA: +12.037 mas/yr[2] Dec.: −3.747 mas/yr[2] |
Parallax (π) | 3.4194±0.0204 mas[2] |
Distance | 954 ± 6 ly (292 ± 2 pc) |
Details | |
Mass | 1.16±0.03[5] M☉ |
Radius | 1.11±0.01[5] R☉ |
Luminosity | 1.48[6] L☉ |
Surface gravity (log g) | 4.413±0.006[5] cgs |
Temperature | 6,070+51 −46[5] K |
Metallicity [Fe/H] | 0.09±0.05[5] dex |
Rotational velocity (v sin i) | 3.1±1.0[7] km/s |
Age | 1.1+0.8 −0.6[8] Gyr |
Other designations | |
EPIC 212300977, TOI-774, TIC 294301883, WASP-55, TYC 6125-113-1, 2MASS J13350194-1730124[9] | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
WASP-55 is a G-type main-sequence star about 954 light-years away in the constellation Virgo. The star is much younger than the Sun at approximately 1.1+0.8
−0.6 billion years.[8] WASP-55 is similar to the Sun in concentration of heavy elements.[10]
A multiplicity survey in 2016 found one candidate stellar companion to WASP-55 at a projected separation of 4.435″±0.018″.[11] Follow-up observations in 2017 were unable to confirm if the suspected companion red dwarf star, with a temperature of 3,340±90 K, is gravitationally bound to WASP-55 or not.[12] It was confirmed in 2019 using Gaia DR2 data.[13]
In 2012 a transiting hot Jupiter planet, WASP-55b, was detected on a tight, circular orbit.[14] Its equilibrium temperature is 1,305 K.[5]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 0.62±0.04 MJ | 0.0558±0.0006 | 4.4656291(11)[8] | <0.056[7] | 89.0±0.2° | 1.34±0.01 RJ |