Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Canis Minor |
Right ascension | 07h24m 58.17971s[1] |
Declination | +11° 40′ 10.2843″[1] |
Apparent magnitude (V) | 5.37[2] |
Characteristics | |
Spectral type | A5 IV[3] or A4 V[4] |
B−V color index | 0.105±0.006[2] |
Astrometry | |
Radial velocity (Rv) | −1.0±4.2[2] km/s |
Proper motion (μ) | RA: −15.263[1] mas/yr Dec.: −15.625[1] mas/yr |
Parallax (π) | 11.3473 ± 0.1958 mas[1] |
Distance | 287 ± 5 ly (88 ± 2 pc) |
Absolute magnitude (MV) | 0.44[2] |
Details | |
Mass | 2.15[5] M☉ |
Radius | 4.6[6] R☉ |
Luminosity | 66.3+3.8 −3.6[7] L☉ |
Surface gravity (log g) | 3.87[5] cgs |
Temperature | 8,374±285[5] K |
Rotational velocity (v sin i) | 159[7] km/s |
Age | 716[5] Myr |
Other designations | |
1 CMi, BD+11°1578, GC 9891, HD 58187, HIP 35987, HR 2820, SAO 96871[8] | |
Database references | |
SIMBAD | data |
1 Canis Minoris is a single[9] star in the equatorial constellationofCanis Minor, located about 287 light years away from the Sun. It is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 5.37.[2] The radial velocity of this object is poorly constrained at −1.0±4.2 km/s.[2]
Cowley et al. (1969) listed a stellar classification of A5 IV[3] for 1 Canis Minoris, matching an A-type subgiant star that has exhausted the hydrogen at its core and is evolving into a giant. However, Gray and Garrison (1989) catalogued it as an A-type main-sequence star with a class of A4 V.[4] The Hipparcos team used a class of A3 Vn,[2] where the 'n' indicates "nebulous" lines due to rapid rotation.
This star is estimated to be 716[5] million years old and is at or near the end of its main sequence lifetime.[7] It has a high rate of spin, showing a projected rotational velocity of 159 km/s.[7] The star has more than double[5] the mass of the Sun with about 4.6[6] times the Sun's radius. It is radiating 66[7] times the Sun's luminosity from its photosphere at an effective temperature of 8,374 K.[5]