Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Puppis |
Right ascension | 06h 37m 45.67135s[1] |
Declination | −43° 11′ 45.3602″[1] |
Apparent magnitude (V) | 3.173[2] |
Characteristics | |
Spectral type | B8 III[3] |
U−B color index | −0.397[2] |
B−V color index | −0.113[2] |
Astrometry | |
Radial velocity (Rv) | +30.9[4] km/s |
Proper motion (μ) | RA: −0.44[1] mas/yr Dec.: −3.87[1] mas/yr |
Parallax (π) | 8.78 ± 0.26 mas[1] |
Distance | 370 ± 10 ly (114 ± 3 pc) |
Absolute magnitude (MV) | −2.11[5] |
Details | |
Radius | 4.2[6] R☉ |
Luminosity | 767[7] L☉ |
Luminosity (bolometric) | 1,340[8] L☉ |
Temperature | 12,120[9] K |
Rotational velocity (v sin i) | 225[10] km/s |
Other designations | |
Database references | |
SIMBAD | data |
Nu Puppis (ν Puppis) is a solitary,[12] blue-hued star in the southern constellation of Puppis. It is the fifth-brightest star in Puppis, with an apparent visual magnitude of 3.17.[2] Based upon an annual parallax shift of 8.78 mas as seen from Earth,[1] it is located about 370 light years from the Sun. The system made its closest approach about 3.6 million years ago when it underwent perihelion passage at a distance of roughly 27 light years.[13]
The star has a stellar classification of B8 III,[3] matching a B-type giant. Absorption lines in the spectrum are displaying central quasi-emission peaks, indicating this is a Be shell star with a circumstellar disk of heated gas that is being seen edge-on.[14] ν Puppis is a candidate variable star showing an amplitude of 0.0117 magnitude with a frequency of 0.15292 per day.[15] It is spinning rapidly with a projected rotational velocity of 225 km/s. This rotation is giving the star an oblate shape, with the equator being 31% larger than the poles.[10] It is radiating (after allowance for ultraviolet radiation) 1,340[8] times the Sun's luminosity from its photosphere at an effective temperature of 12,120 K.[9]
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