Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Camelopardalis |
Right ascension | 03h 19m 59.27222s[1] |
Declination | +65° 39′ 08.2519″[1] |
Apparent magnitude (V) | 4.74[2] (4.76 - 4.90)[3] |
Characteristics | |
Evolutionary stage | main sequence[4] |
Spectral type | B2.5 Vne[5] |
U−B color index | −0.77[6] |
B−V color index | −0.108±0.002[2] |
R−I color index | −0.13[6] |
Variable type | Be star[3] |
Astrometry | |
Radial velocity (Rv) | −3.4±3.5[2] km/s |
Proper motion (μ) | RA: +10.506[1] mas/yr Dec.: −14.677[1] mas/yr |
Parallax (π) | 6.0704 ± 0.3539 mas[1] |
Distance | 540 ± 30 ly (165 ± 10 pc) |
Absolute magnitude (MV) | −2.07[2] |
Details | |
Mass | 7.5[5] M☉ |
Radius | 4.0[7] R☉ |
Luminosity | 1080.69[2] L☉ |
Surface gravity (log g) | 4.20[4] cgs |
Temperature | 18,720[4] K |
Rotational velocity (v sin i) | 328[4] km/s |
Age | 31.6[5] Myr |
Other designations | |
Database references | |
SIMBAD | data |
BK Camelopardalis is a variable star in the northern circumpolar constellation of Camelopardalis, near the constellation border with Cassiopeia. It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude that fluctuates around 4.74.[2] The star is located approximately 540 light years away from the Sun based on parallax.[1] It is a proposed member of the Cassiopeia–Taurus group of co-moving stars.[9]
GaiaDR2
was invoked but never defined (see the help page).Anderson2012
was invoked but never defined (see the help page).Samus2017
was invoked but never defined (see the help page).zorec
was invoked but never defined (see the help page).tetzlaff2011
was invoked but never defined (see the help page).ducati
was invoked but never defined (see the help page).underhill
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).deZeeuw1999
was invoked but never defined (see the help page).