Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Pavo |
Right ascension | 20h 01m 44.74682s[2] |
Declination | â59° 22′ 33.1864″[2] |
Apparent magnitude (V) | 4.95[3] |
Characteristics | |
Spectral type | M6 III[4] |
BâV color index | 1.356±0.011[3] |
Variable type | SRb[5] |
Astrometry | |
Radial velocity (Rv) | â10.3±2.8[6] km/s |
Proper motion (ÎŒ) | RA: +20.385[2] mas/yr Dec.: â26.769[2] mas/yr |
Parallax (Ï) | 7.0208 ± 0.4464 mas[2] |
Distance | 460 ± 30 ly (142 ± 9 pc) |
Absolute magnitude (MV) | â0.86[3] |
Details | |
Radius | 204±29[7] R☉ |
Luminosity | 7,412[3] L☉ |
Surface gravity (log g) | 0.87[8] cgs |
Temperature | 3,516±275[7] K |
Other designations | |
Database references | |
SIMBAD | data |
NU Pavonis (N-U, not "nu") is a variable star in the southern constellation of Pavo. With a nominal apparent visual magnitude of 4.95,[3] it is a faint star but visible to the naked eye. The distance to NU Pav, as determined from its annual parallax shift of 7.0 mas[2] as seen from Earth's orbit, is around 460 light years. It is moving closer with a heliocentric radial velocity of â10 km/s.[6]
This is an aging red giant with a stellar classification of M6 III,[4] currently on the asymptotic giant branch. It is a semiregular variable star of sub-type SRb that ranges in magnitude from 4.91 down to 5.26 with a period of 60 days.[7] The star has expanded to 204[7] times the Sun's radius and is radiating 7,412[3] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 3,516 K.[7] Far-ultraviolet emission has been detected from these coordinates, which may be coming from a companion star.[8]
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