Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Camelopardalis |
Right ascension | 05h 06m 08.45273s[2] |
Declination | +58° 58′ 20.5432″[2] |
Apparent magnitude (V) | 5.08[3] |
Characteristics | |
Spectral type | B3 Ve[4] |
B−V color index | −0.080[5] |
Variable type | Be[6] |
Astrometry | |
Proper motion (μ) | RA: −6.264[2] mas/yr Dec.: −7.118[2] mas/yr |
Parallax (π) | 4.7543 ± 0.1224 mas[2] |
Distance | 690 ± 20 ly (210 ± 5 pc) |
Absolute magnitude (MV) | −1.38[5] |
Details | |
Mass | 6.0±1.2[7] M☉ |
Radius | 7.87[8] R☉ |
Luminosity | 1,766+131 −122[7] L☉ |
Surface gravity (log g) | 4.00±0.35[7] cgs |
Temperature | 17,240±560[7] K |
Rotational velocity (v sin i) | 95±6[7] km/s |
Age | 25±3[9] Myr |
Other designations | |
Database references | |
SIMBAD | data |
11 Camelopardalis is a single[11] star in the northern circumpolar constellation of Camelopardalis, located around 690 light years away from the Sun as determined by parallax. It has the variable star designation BV Camelopardalis; 11 Camelopardalis is the Flamsteed designation. This object is visible to the naked eye as a faint, blue-white hued star with a baseline apparent visual magnitude of +5.22.[5] It forms a double star with 12 Camelopardalis, which is only 3 arcminutes away.
This is a main sequence Be star with a stellar classification of B3 Ve.[4] Samus et al. (2017) classify it as a Be variable, rather than a Gamma Cassiopeiae type, and it ranges from a peak Hipparcos magnitude of 5.10 down to 5.22.[6] The star is spinning with a projected rotational velocity of 95 km/s,[7] but is being viewed from an extreme pole-on position. Hence it is spinning much more rapidly than indicated. Outbursts of hydrogen emission lines have been observed, as well as rapid changes in hydrogen line profiles.[12] It is 25[9] million years old with around six[7] times the mass of the Sun.
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