A visual band light curve for BC Canis Minoris, plotted from data presented by Tabur et al. (2009)[1] | |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Canis Minor |
Right ascension | 07h 52m 07.19000s[2] |
Declination | 03° 16′ 38.4465″[2] |
Apparent magnitude (V) | 6.30[3] (6.14 to 6.42)[4] |
Characteristics | |
Evolutionary stage | AGB[5] |
Spectral type | M4/5III[6] |
B−V color index | 1.464±0.015[3] |
Variable type | SRb[4] |
Astrometry | |
Radial velocity (Rv) | −66.91±0.24[3] km/s |
Proper motion (μ) | RA: +49.415[2] mas/yr Dec.: −78.835[2] mas/yr |
Parallax (π) | 6.2916 ± 0.1748 mas[2] |
Distance | 520 ± 10 ly (159 ± 4 pc) |
Absolute magnitude (MV) | 0.36[3] |
Details | |
Radius | 60.4+7.6 −10.3[2] R☉ |
Luminosity | 496.7±15.9[2] L☉ |
Temperature | 3,507+344 −201[2] K |
Other designations | |
Database references | |
SIMBAD | data |
BC Canis Minoris is a variable star in the equatorial constellation of Canis Minor. It has a reddish hue and is just barely visible to the naked eye with an apparent visual magnitude that fluctuates around 6.30.[3] The distance to this object is approximately 520 light years based on parallax,[2] but it is drifting closer with a radial velocity of −67 km/s.[3]
This is an aging red giant star currently on the asymptotic giant branch[5] with a stellar classification of M4/5III.[6] It is a semi-regular variable of subtype SRb[4] with measured pulsation periods of 27.7, 143.3 and 208.3 days, and an average visual magnitude of 6.30.[8] With the supply of hydrogen at its core exhausted, it has cooled and expanded off the main sequence and now has around 60[2] times the girth of the Sun. On average, the star is radiating about 497[2] times the luminosity of the Sun from its swollen photosphere at an effective temperature of 3,507 K.[2]
Tabur
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