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Visual binary in the constellation Camelopardalis From Wikipedia, the free encyclopedia
HD 20104 (HR 967) is a visual binary in the northern circumpolar constellation Camelopardalis. The system has a combined apparent magnitude of 6.41,[9] making it near naked eye visibility. When resolved in a large telescope, HD 20104 appears to be a pair of 7th magnitude A-type main-sequence stars with a separation of about 0.5″.[10] Located approximately 550 light years away,[5] the system is approaching the Sun with a heliocentric radial velocity of −6 km/s.[4]
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Camelopardalis |
A | |
Right ascension | 03h 17m 31.527s[1] |
Declination | +65° 39′ 30.11″[1] |
Apparent magnitude (V) | 7.05±0.01[1] |
B | |
Right ascension | 03h 17m 31.593s[1] |
Declination | +65° 39′ 30.26″[1] |
Apparent magnitude (V) | 7.39±0.01[1] |
Characteristics | |
A | |
Spectral type | A2 V[2] |
U−B color index | +0.06[3] |
B−V color index | +0.08[3] |
B | |
Spectral type | A4V[2] |
Astrometry | |
Radial velocity (Rv) | −6±2[4] km/s |
Proper motion (μ) | RA: −10.54 mas/yr[5] Dec.: +5.84 mas/yr[5] |
Parallax (π) | 5.92 ± 0.65 mas[5] |
Distance | approx. 550 ly (approx. 170 pc) |
Absolute magnitude (MV) | +0.3[6] |
Orbit[7] | |
Primary | HD 20104 A |
Companion | HD 20104 B |
Period (P) | 350 yr |
Semi-major axis (a) | 0.46″ |
Eccentricity (e) | 0.4 |
Inclination (i) | 135° |
Longitude of the node (Ω) | 58° |
Periastron epoch (T) | 2055.0 |
Argument of periastron (ω) (secondary) | 100° |
Details | |
A | |
Mass | 2.46[8] M☉ |
B | |
Mass | 2.27[8] M☉ |
Other designations | |
Database references | |
SIMBAD | The system |
A | |
B |
The system's stars have masses twice that of the Sun[8] and effective temperatures ranging from 8,100 to 8,700 K,[9][11] typical of stars their type. The primary radiates at 71.3 L☉[11] − over luminous for its class − and spins with a projected rotational velocity of 159 km/s.[12] HD 20104 has an age of 313 million years.[11]
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