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Double star in the constellation Camelopardalis From Wikipedia, the free encyclopedia
29 Camelopardalis (29 Cam) is a double star in the circumpolar constellation Camelopardalis. With an apparent magnitude of 6.59,[2] it's right below the max visibility to the naked eye, and can only be viewed under phenomenal conditions. The star is located 484 light years[1] away based on parallax, but is drifting further away with a radial velocity of 3.9 km/s.[3]
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Camelopardalis |
Right ascension | 05h 50m 33.8729s[1] |
Declination | +56° 55′ 08.1822″[1] |
Apparent magnitude (V) | 6.590±0.009[2] |
Characteristics | |
29 Cam A | |
Spectral type | A4 IV-V |
U−B color index | +0.13[2] |
B−V color index | +0.09[2] |
29 Cam B | |
Spectral type | A3 V |
Astrometry | |
29 Cam A | |
Radial velocity (Rv) | 3.9±2[3] km/s |
Proper motion (μ) | RA: –19.460[1] mas/yr Dec.: –4.249[1] mas/yr |
Parallax (π) | 6.7370 ± 0.0607 mas[1] |
Distance | 484 ± 4 ly (148 ± 1 pc) |
Absolute magnitude (MV) | +0.71[4] |
29 Cam B | |
Proper motion (μ) | RA: +2.585[5] mas/yr Dec.: –0.570[5] mas/yr |
Parallax (π) | 1.6375 ± 0.0483 mas[5] |
Distance | 1,990 ± 60 ly (610 ± 20 pc) |
Details | |
29 Cam A | |
Mass | 2.47 ± 0.08[6] M☉ |
Radius | 3.49+0.14 −0.12[7] R☉ |
Luminosity | 58.9+8.9 −7.6[6] L☉ |
Surface gravity (log g) | 3.77[8] cgs |
Temperature | 8,337 ± 96[6] K |
Rotational velocity (v sin i) | 123[9] km/s |
Age | 380 ± 14[6] Myr |
29 Cam B | |
Mass | 2.12[10] M☉ |
Radius | 2.06[11] R☉ |
Luminosity | 15.043[11] L☉ |
Temperature | 7911[11] K |
Rotational velocity (v sin i) | 110±8[12] km/s |
Other designations | |
Database references | |
SIMBAD | data |
29 Cam A has a classification of A4IV-V, which suggests that this star is beginning to evolve off the main sequence. Zorec et al. models it as a star that has completed 90.6% of the main sequence, which correlates to an age of 380 million years.[6] At present, 29 Cam has 2.47 the mass of the Sun,[6] and 3.49 times its radius. [7] It radiates at 58.9 times the luminosity of the Sun from an effective temperature of 8,337 K,[6] which gives it a white hue of an A-type star. 29 Cam spins rapidly at a projected rotational velocity of 123 km/s despite its evolved state.
29 Cam has a companion designated BD+56 1065B, which is a 10 magnitude star. According to the proper motion, this star is unrelated to the primary, and is 4 times farther than the primary.[13] The companion is relatively cooler and less luminous than the primary.
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