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Star in the constellation Pavo From Wikipedia, the free encyclopedia
Epsilon Pavonis, Latinized from ε Pavonis, is a single,[9] white-hued star in the constellation Pavo. It can be viewed with the naked eye, having an apparent visual magnitude of 3.97.[2] The annual parallax shift of 31.04[1] mas provides a distance estimate of 105 light years from the Sun. This star is a member of the proposed Argus Association, a young moving group of more than 60 stars associated with the IC 2391 cluster.[10] Epsilon Pavonis is moving closer to the Sun with a radial velocity of −6.7 km/s.[4]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Pavo |
Right ascension | 20h 00m 35.55558s[1] |
Declination | −72° 54′ 37.8198″[1] |
Apparent magnitude (V) | 3.97[2] |
Characteristics | |
Spectral type | A0 Va[2] |
U−B color index | −0.05[3] |
B−V color index | −0.03[2] |
Astrometry | |
Radial velocity (Rv) | −6.7±0.7[4] km/s |
Proper motion (μ) | RA: +81.78[1] mas/yr Dec.: −132.16[1] mas/yr |
Parallax (π) | 31.04 ± 0.17 mas[1] |
Distance | 105.1 ± 0.6 ly (32.2 ± 0.2 pc) |
Absolute magnitude (MV) | 1.43[2] |
Details | |
Mass | 2.2[5] M☉ |
Radius | 1.74[6] R☉ |
Luminosity | 32[7] L☉ |
Surface gravity (log g) | 4.32±0.02[6] cgs |
Temperature | 10,440[8] K |
Rotational velocity (v sin i) | 85[7] km/s |
Age | 27[6] Myr |
Other designations | |
Database references | |
SIMBAD | data |
With a stellar classification of A0 Va,[2] Epsilon Pavonis is an ordinary A-type main-sequence star that is generating energy through hydrogen fusion at its core. It is just 27[6] million years old with a projected rotational velocity of 85[7] km/s. The star has 2.2[5] times the mass of the Sun and 1.74[6] the Sun's radius. It is radiating 32[7] times the Sun's luminosity from its photosphere at an effective temperature of 10,440 K.[8]
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