17 Canis Majoris

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

17 Canis Majoris is a single[7] star in the southern constellation of Canis Major, located 602 light years away from the Sun.[1] It is visible to the naked eye as a dim, white-hued star with an apparent visual magnitude of 5.80.[2] The object is moving closer to the Earth with a heliocentric radial velocity of −13 km/s.[2]

Right ascension06h 55m 02.73800s[1]
Declination−20° 24′ 17.5578″[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
17 Canis Majoris
Observation data
Epoch J2000      Equinox J2000
Constellation Canis Major
Right ascension 06h 55m 02.73800s[1]
Declination −20° 24′ 17.5578″[1]
Apparent magnitude (V) 5.80[2]
Characteristics
Evolutionary stage Main sequence[3]
Spectral type A2 V[4]
B−V color index 0.048±0.003[2]
Astrometry
Radial velocity (Rv)−12.9±0.5[2] km/s
Proper motion (μ) RA: âˆ’0.242[1] mas/yr
Dec.: âˆ’10.241[1] mas/yr
Parallax (π)5.4157±0.0438 mas
Distance602 ± 5 ly
(185 ± 1 pc)
Absolute magnitude (MV)−0.14[2]
Details
Mass2.84±0.05[3] M☉
Radius5.2[5] R☉
Luminosity126+18
−15
[3] L☉
Surface gravity (log g)3.38[1] cgs
Temperature8,872+164
−162
[3] K
Rotational velocity (v sin i)43[3] km/s
Age340[1] Myr
Other designations
17 CMa, BD−20°1624, GC 9078, HD 51055, HIP 33248, HR 2588, SAO 172569, ADS 5585, CCDM 06550-2025, WDS J06550-2024[6]
Database references
SIMBADdata
Close

This is an A-type main-sequence star with a stellar classification of A2 V,[4] and is near the end of its main sequence lifetime. It has 2.8 times the mass of the Sun and is spinning with a projected rotational velocity of 43 km/s.[3] The star is radiating 126 times the luminosity of the Sun from its photosphere at an effective temperature of 8,872 K.[3] It has a magnitude 8.66 visual companion at an angular separation of 42.90″ along a position angle of 147°, as of 2015.[8]

References

Related Articles

Wikiwand AI