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 (Ό) |
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]
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 (Ό) |
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]