Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Canis Major |
Right ascension | 06h 36m 22.85133s[1] |
Declination | −18° 39′ 35.6838″[1] |
Apparent magnitude (V) | 5.704[2] (5.87 + 7.61)[3] |
Characteristics | |
Spectral type | G8 III + F3 IV-V[3] |
B−V color index | +0.815[2] |
Astrometry | |
Radial velocity (Rv) | +26.13[2] km/s |
Proper motion (μ) | RA: −10.09[1] mas/yr Dec.: +13.06[1] mas/yr |
Parallax (π) | 12.3660 ± 0.1985 mas[4] |
Distance | 264 ± 4 ly (81 ± 1 pc) |
Absolute magnitude (MV) | +1.23[5] |
Details | |
ν1 CMa A | |
Mass | 1.41[2] M☉ |
Luminosity | 8[2] L☉ |
Surface gravity (log g) | 3.00[6] cgs |
Temperature | 6,091±822[2] K |
Metallicity [Fe/H] | −0.06[6] dex |
Rotational velocity (v sin i) | 4.8±0.2[5] km/s |
Age | 3.07[2] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Nu1 Canis Majoris (ν1 Canis Majoris) is a binary star in the constellation Canis Major. It is visible to the naked eye with a combined apparent visual magnitude of 5.7.[2] Based on parallax shift of 12.366 mas as seen from our orbit, this system is approximately 264 light years from the Sun.
As of 2011, the pair had an angular separation of 17.29 arc seconds along a position angle of 264.2°.[8] The yellow hued magnitude 5.87[3] primary, component A, is an evolved G-type giant star with a stellar classification of G8 III.[3] Its magnitude 7.61[3] companion, component B, is a yellow-white hued F-type main sequence/subgiant hybrid with a class of F3 IV-V.[3]
vanLeeuwen2007
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was invoked but never defined (see the help page).Mason2012
was invoked but never defined (see the help page).