Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Orion |
Right ascension | 05h 36m 54.389s[1] |
Declination | +09° 17′ 26.417″[1] |
Apparent magnitude (V) | 4.081[2] |
Characteristics | |
Evolutionary stage | Yellow giant |
Spectral type | G8 III-IV[3] |
U−B color index | +0.618[2] |
B−V color index | +0.966[2] |
Astrometry | |
Radial velocity (Rv) | 99.03±0.18[1] km/s |
Proper motion (μ) | RA: +98.301 mas/yr[1] Dec.: −305.022 mas/yr[1] |
Parallax (π) | 28.6722 ± 0.1859 mas[1] |
Distance | 113.8 ± 0.7 ly (34.9 ± 0.2 pc)[1] |
Absolute magnitude (MV) | +1.33±0.07[4] |
Details[5] | |
Mass | 1.07±0.04 M☉ |
Radius | 8.22±0.07[6] R☉ |
Luminosity | 29.8±0.04[6] L☉ |
Surface gravity (log g) | 3.00±0.02 cgs |
Temperature | 4,703±11[6] K |
Metallicity [Fe/H] | −0.56±0.02 dex |
Rotational velocity (v sin i) | 1.91±0.53 km/s |
Age | 6.91±1.04 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Phi2 Orionis is a star in the constellation Orion, where it forms a small triangle on the celestial sphere with the nearby Meissa and Phi1 Orionis.[8] This star is visible to the naked eye with an apparent visual magnitude of 4.081.[2] Based upon an annual parallax shift of 28.67 mas,[6] it is located around 114 light-years from the Sun.
This is an evolved G-type star of stellar classification G8 III-IV,[3] which means that it is in an evolutionary stage between a subgiant (IV) and a giant star (III). It is estimated to be 6.9 billion years old, has 1.07 times the mass of the Sun,[5] but has expanded to 8 times the Sun's radius. The star shines with 30 times the solar luminosity from its outer atmosphere at an effective temperature of 4,700 K.[6]
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