| Observation data EpochJ2000.0 EquinoxJ2000.0 (ICRS) | |
|---|---|
| Constellation | Canis Minor |
| Right ascension | 07h 24m 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−Vcolor 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 theequatorialconstellation ofCanis Minor, located about 287 light years away from the Sun. It is visible to the naked eye as a faint, white-hued star with anapparent visual magnitude of 5.37.[2] Theradial velocity of this object is poorly constrained at−1.0±4.2 km/s.[2]
Cowley et al. (1969) listed astellar classification of A5 IV[3] for 1 Canis Minoris, matching anA-typesubgiant star that has exhausted the hydrogen at its core and isevolving into agiant. However, Gray and Garrison (1989) catalogued it as anA-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 itsmain sequence lifetime.[7] It has a high rate of spin, showing aprojected 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 theSun's radius. It is radiating 66[7] times theSun's luminosity from itsphotosphere at aneffective temperature of 8,374 K.[5]
