11 Canis Majoris

Star in the constellation Canis Major From Wikipedia, the free encyclopedia

11 Canis Majoris is a single[10] star in the southern constellation of Canis Major, the eleventh entry in John Flamsteed's catalogue of stars in that constellation. It has a blue-white hue and is visible to the naked eye with an apparent visual magnitude of 5.28.[2] The distance to this star is approximately 1,010 light years from the Sun based on parallax,[1] and it is drifting further away with a radial velocity of around +15 km/s.[4] It has an absolute magnitude of −1.63.[2]

Right ascension06h 46m 51.09272s[1]
Declination−14° 25′ 33.5042″[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
11 Canis Majoris
Observation data
Epoch J2000      Equinox J2000
Constellation Canis Major
Right ascension 06h 46m 51.09272s[1]
Declination −14° 25′ 33.5042″[1]
Apparent magnitude (V) 5.28[2]
Characteristics
Spectral type B8/9III[3]
B−V color index −0.024±0.004[2]
Astrometry
Radial velocity (Rv)+15.0±4.2[4] km/s
Proper motion (μ) RA: âˆ’2.853±0.344[1] mas/yr
Dec.: +8.514±0.363[1] mas/yr
Parallax (π)3.2263±0.1847 mas[1]
Distance1,010 ± 60 ly
(310 ± 20 pc)
Absolute magnitude (MV)−1.63[2]
Details
Mass3.9[5] M☉
Radius8.8[6] R☉
Luminosity465[5] L☉
Surface gravity (log g)3.85[7] cgs
Temperature13,274[7] K
Metallicity [Fe/H]+0.39[7] dex
Rotational velocity (v sin i)130[8] km/s
Other designations
11 CMa, BD−14°1584, GC 8879, HD 49229, HIP 32492, HR 2504, SAO 151919[9]
Database references
SIMBADdata
Close

This star has a stellar classification of B8/9III,[3] matching a B-type star that is in the giant stage. It has a high rate of spin with a projected rotational velocity of 130 km/s.[8] The star is radiating 465 times the luminosity of the Sun[5] from its photosphere at an effective temperature of 13,274 K.[7]

References

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