BE Camelopardalis
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Camelopardalis |
| Right ascension | 03h 49m 31.27755s |
| Declination | +65° 31′ 33.5258″ |
| Apparent magnitude (V) | 4.39 (4.35 - 4.48) |
| Characteristics | |
| Evolutionary stage | asymptotic giant branch |
| Spectral type | M2 II |
| B−V color index | 1.870±0.029 |
| Variable type | Lc |
| Astrometry | |
| Radial velocity (Rv) | −1.70±1.47 km/s |
| Proper motion (μ) | RA: +0.319 mas/yr Dec.: −15.593 mas/yr |
| Parallax (π) | 3.3288±0.1874 mas |
| Distance | 958+53 −51 ly (293.7+16.4 −15.5 pc) |
| Absolute magnitude (MV) | −2.51 |
| Details | |
| Mass | 2.93 M☉ |
| Radius | 250 R☉ |
| Luminosity | 10,600 L☉ |
| Temperature | 3,660 K |
| Other designations | |
| BE Cam, BD+65°369, HD 23475, HIP 17884, HR 1155, SAO 12916 | |
| Database references | |
| SIMBAD | data |
BE Camelopardalis is a solitary variable star in the northern circumpolar constellation of Camelopardalis. It is visible to the naked eye as a faint, red-hued point of light with an apparent visual magnitude that fluctuates around 4.39. The star is located roughly 960 light years away.
This object is an M-type bright giant with a stellar classification of M2 II, and is currently on the asymptotic giant branch. In 1928, Joel Stebbins and Charles Morse Huffer announced that the star, then called HR 1155, is a variable star, based on observations made at Washburn Observatory. It was given its variable star designation, BE Camelopardalis, in 1977. It is classified as an irregular variable of subtype Lc and its brightness varies from magnitude +4.35 down to +4.48. Having exhausted the supply of hydrogen at its core, the star has expanded to around 250 times the Sun's radius. It has 2.9 times the Sun's mass and is radiating over 10,000 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 3,660 K.