36 Camelopardalis
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Camelopardalis |
| Right ascension | 06h 12m 51.06255s |
| Declination | +65° 43′ 06.3160″ |
| Apparent magnitude (V) | 5.344 |
| Characteristics | |
| Spectral type | K1 III-IIIb CH-0.5 |
| U−B color index | +2.708 |
| B−V color index | +0.764 |
| Astrometry | |
| Radial velocity (Rv) | +1.15±0.13 km/s |
| Proper motion (μ) | RA: +6.240 mas/yr Dec.: −31.308 mas/yr |
| Parallax (π) | 4.5905±0.0728 mas |
| Distance | 710 ± 10 ly (218 ± 3 pc) |
| Absolute magnitude (MV) | −1.33 |
| Details | |
| Mass | 1.24 M☉ |
| Radius | 42 R☉ |
| Luminosity | 714 L☉ |
| Surface gravity (log g) | 1.26 cgs |
| Temperature | 4,589 K |
| Metallicity [Fe/H] | −0.11 dex |
| Rotational velocity (v sin i) | 3.0 km/s |
| Other designations | |
| 36 Cam, BD+65°517, FK5 233, GC 7856, HD 41927, HIP 2940, HR 2165, SAO 13756 | |
| Database references | |
| SIMBAD | data |
36 Camelopardalis is a single star in the northern circumpolar constellation of Camelopardalis. It is visible to the naked eye as a dim point of light with an apparent visual magnitude of +5.3. Parallax measurements provide a distance estimate of approximately 710 light years away from the Sun, and it is drifting away from the Earth with a radial velocity of −1.15 km/s.
36 Camelopardalis has a stellar classification of K1 III-IIIb, which indicates that it is a K-type giant star with a mild underabundance of CH molecules in its spectrum. At present it has 1.24 times the mass of the Sun but has expanded to an enlarged diameter of 42 R☉. It shines at 714 L☉ from its photosphere at an effective temperature of 4,589 K, giving it an orange glow. 36 Cam's metallicity is around solar level and spins slowly with a projected rotational velocity of 3 km/s.