| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Canis Major |
| Right ascension | 06h37m 53.42144s[1] |
| Declination | −18° 14′ 14.9218″[1] |
| Apparent magnitude (V) | 4.41[2] (4.63 + 8.56)[3] |
| Characteristics | |
| Spectral type | K0 II-III[4] |
| U−B color index | +1.04[2] |
| B−V color index | +1.16[2] |
| Astrometry | |
| Radial velocity (Rv) | −1.50±0.70[5] km/s |
| Proper motion (μ) | RA: −7.32[1] mas/yr Dec.: −8.72[1] mas/yr |
| Parallax (π) | 7.74 ± 0.43 mas[1] |
| Distance | 420 ± 20 ly (129 ± 7 pc) |
| Absolute magnitude (MV) | −1.13[6] |
| Details[4] | |
| ν3 CMa A | |
| Mass | 3.38±0.37[7] M☉ |
| Radius | 32.7 R☉ |
| Luminosity | 398 L☉ |
| Surface gravity (log g) | 2.34 cgs |
| Temperature | 4,510 K |
| Metallicity [Fe/H] | −0.24 dex |
| Rotation | 183 d |
| Rotational velocity (v sin i) | 8[8] km/s |
| Age | 380±20[7] Myr |
| Other designations | |
ν3 CMa, 8 Canis Majoris, BD−18°1492, GC 8660, HD 47442, HIP 31700, HR 2443, SAO 151730, CCDM 06379-1814[9] | |
| Database references | |
| SIMBAD | data |
Nu3 Canis Majoris, Latinized from ν3 Canis Majoris, is a binary star[3] system in the southern constellationofCanis Major.
The star system, appearing as one star, is deemed visible to the naked eye with its combined apparent visual magnitude of 4.41.[2] Based upon an annual parallax shift of 7.74 mas as seen from Earth,[1] this system is about 420 light years from the Sun, much further than Nu1 and Nu2 which appear nearby when seen from one point in the Solar System.
The primary member, component A, is an evolved, orange-hued giant/bright giant hybrid with an apparent magnitude of +4.63[3] and a stellar classification of K0 II-III.[4] It is most likely (96% chance) on the horizontal branch.[7] The star has a moderate level of surface activity with a magnetic field strength of 2.2±0.4 G and is a source of X-ray emission with a luminosity of 624×1027 erg s−1.[4]
This giant has an estimated 3.4[7] times the mass of the Sun and has expanded to 33[4] times the Sun's radius. It is radiating 398 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,510 K.[4] The star is spinning with the leisurely period of 183 days.[4] Its companion, component B has been observed at 1.040 arcseconds distant and has an apparent magnitude of +8.56.[3]
{{cite web}}: CS1 maint: postscript (link)
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