CQ Camelopardalis

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Template:Short description

CQ Camelopardalis
File:CQCamLightCurve.png
A light curve for CQ Camelopardalis, plotted from Hipparcos data[1]
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Camelopardalis
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 5.19[3]
Characteristics
Evolutionary stage AGB[4]
Spectral type M0 II[5]
B−V Template:Engvar +2.05[3]
R−I Template:Engvar +1.23[3]
Variable type Lc?[6]
Astrometry
Radial velocity (Rv)−22.2±0.5[7] km/s
Proper motion (μ) RA: −3.734 mas/yr[2]
Dec.: −0.171 mas/yr[2]
Parallax (π)1.6385±0.1030 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Details
Mass12.7±0.5[8] Template:Solar mass
Radius333[9] Template:Solar radius
Luminosity13,236[10] Template:Solar luminosity
Surface gravity (log g)0.48±0.08[11] cgs
Temperature3,790±122[9] K
Metallicity [Fe/H]+0.17±0.04[11] dex
Age15.8±0.3[8] Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[12]
Database references
SIMBADdata

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CQ Camelopardalis, abbreviated as CQ Cam, is a solitary[13] variable star in the northern circumpolar constellation Camelopardalis. It has an apparent magnitude of 5.19,[3] making it visible to the naked eye under ideal conditions. The object is relatively far at a distance of about 2,000 light years[2] but is drifting closer with a heliocentric radial velocity of Script error: No such module "val"..[7] It has a peculiar velocity of Script error: No such module "val"., making it a runaway star.[8]

CQ Cam has a stellar classification of M0 II,[5] indicating that it is a red bright giant. CQ Cam is currently on the asymptotic giant branch, fusing hydrogen and helium shells around an inert carbon core. At present it has 12.7 times the mass of the Sun but, at the age of 16 million years,[8] it has expanded to 333 times the radius of the Sun.[9] The object is a luminous star, with a bolometric luminosity over 10,000 times that of the Sun.[10] Despite this brightness, CQ Cam's large diameter yields an effective temperature of Script error: No such module "val".[9] from its photosphere, giving a red hue.

CQ Cam has been classified as a low amplitude slow irregular variable based on Hipparcos photometry.[6] However, there have not been enough observations to confirm this.[14]

References

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Template:Stars of Camelopardalis