Iota Canis Majoris, Latinized from ι Canis Majoris, is a solitary[12] variable supergiant star in the southern constellation of Canis Major. It is visible to the naked eye with an apparent visual magnitude that varies between +4.36 and +4.40.[3] The distance to this star is approximately 2,500 light years based on parallax measurements. It is drifting further away with a radial velocity of +41.2 km/s.[7]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Canis Major |
Right ascension | 06h 56m 08.22413s[1] |
Declination | −17° 03′ 15.2675″[1] |
Apparent magnitude (V) | 4.40[2] (4.36 - 4.40[3]) |
Characteristics | |
Spectral type | B3 Ib[4] or B3 Ib/II[5] |
U−B color index | −0.74[6] |
B−V color index | −0.07[6] |
Variable type | Beta Cephei?[2] |
Astrometry | |
Radial velocity (Rv) | +41.20[7] km/s |
Proper motion (μ) | RA: −3.56 ± 0.17[1] mas/yr Dec.: +2.42 ±0.20[1] mas/yr |
Parallax (π) | 1.30 ± 0.20 mas[1] |
Distance | approx. 2,500 ly (approx. 800 pc) |
Absolute magnitude (MV) | −5.51[8] |
Details | |
Mass | 12.5 ± 1.2[9] M☉ |
Radius | 25.9[8] R☉ |
Luminosity | 47,000[8] L☉ |
Surface gravity (log g) | 2.60[10] cgs |
Temperature | 17,000[10] K |
Metallicity [Fe/H] | −0.17[11] dex |
Rotational velocity (v sin i) | 27±4[10] km/s |
Age | 15.8 ± 0.4[9] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Iota Canis Majoris is a massive blue-white B-type supergiant with a stellar classification of B3 Ib.[4] It has been classified as a Beta Cephei type variable star,[3] but the supergiant spectral type and a period of over a day mean it is no longer considered to be of that type.[2] This star is 15.8[9] million years old and is spinning with a projected rotational velocity of 27 km/s.[10] It has 12.5[9] times the mass and 25.9 times the radius of the Sun.[8] Iota Canis Majoris is radiating 47,000[8] times the luminosity of the Sun from its photosphere at an effective temperature of 17,000 K.[10]
The star displays a bow shock feature from its interaction with the interstellar medium, but this nebulosity is not aligned with the star's motion through the galaxy.[13]