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Star in the constellation Camelopardalis From Wikipedia, the free encyclopedia
Gamma Camelopardalis, Latinized from γ Camelopardalis, is a suspected wide binary star[11] system in the northern circumpolar constellation of Camelopardalis. With a visual magnitude of 4.66,[3] it is faintly visible to the naked eye. Based upon an annual parallax shift of 9.09 mas as seen from Earth,[1] this star is located about 359 light years from the Sun.
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Camelopardalis |
Right ascension | 03h 50m 21.50892s[1] |
Declination | +71° 19′ 56.148″[1][2] |
Apparent magnitude (V) | 4.66[3] + 9.07[4] |
Characteristics | |
Spectral type | A2 IVn[5] |
U−B color index | +0.07[3] |
B−V color index | +0.03[3] |
Astrometry | |
Radial velocity (Rv) | 0.2±2.5[6] km/s |
Proper motion (μ) | RA: +18.17[1] mas/yr Dec.: −42.85[1] mas/yr |
Parallax (π) | 9.09 ± 0.18 mas[1] |
Distance | 359 ± 7 ly (110 ± 2 pc) |
Absolute magnitude (MV) | −0.62[7] |
Details | |
γ Cam A | |
Mass | 2.98±0.04[8] M☉ |
Radius | 2.5[9] R☉ |
Luminosity | 185[8] L☉ |
Temperature | 8,892[8] K |
Rotational velocity (v sin i) | 205[10] km/s |
Other designations | |
Database references | |
SIMBAD | data |
The brighter primary, designated component A, is a white-hued A-type subgiant star with a stellar classification of A2 IVn.[5] It is spinning rapidly with a projected rotational velocity of 205 km/s. This is giving the star an oblate shape with an equatorial bulge that is 17% larger than the polar radius.[10] It has about three[8] times the mass of the Sun and 2.5[9] times the Sun's radius. The star is radiating 185[8] times the Sun's luminosity from its photosphere at an effective temperature of 8,892 K.[8]
The magnitude 9.07 secondary, BD+70 260, designated component C, lies at an angular separation of 106.00 arc seconds along a position angle of 85°, as of 2011. Component B is a magnitude 12.40 visual companion at a separation of 56.30 arc seconds along position angle 247°.[4]
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