CQ Camelopardalis
Appearance
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Camelopardalis |
Right ascension | 03h 24m 40.555745s[1] |
Declination | +64° 35′ 09.5771″[1] |
Apparent magnitude (V) | 5.15-5.27[2] |
Characteristics | |
Spectral type | M0II[2] |
U−B color index | 2.06 |
B−V color index | 2.08 |
R−I color index | 1.23 |
Variable type | Lc[2] |
Astrometry | |
Radial velocity (Rv) | -22.20 km/s |
Proper motion (μ) | RA: -2.86 mas/yr Dec.: 0.87 mas/yr |
Parallax (π) | 1.59 ± 0.34 mas |
Distance | approx. 2,100 ly (approx. 600 pc) |
Details | |
Luminosity | 17153[3] L☉ |
Temperature | 3598[3] K |
Other designations | |
Database references | |
SIMBAD | data |
Data sources: | |
Hipparcos Catalogue, CCDM (2002), Bright Star Catalogue (5th rev. ed.) |
CQ Camelopardalis is a variable star in the constellation Camelopardalis. A red giant of spectral type M0II, it varies irregularly from magnitude 5.15 to 5.27.[2] Located around 628 parsecs distant, it shines with a luminosity approximately 17153 times that of the Sun and has a surface temperature of 3598 K.[3]
References
- ^ a b Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.
- ^ a b c d Otero, Sebastian Alberto (15 August 2011). "CQ Camelopardalis". The International Variable Star Index. American Association of Variable Star Observers. Retrieved 20 July 2014.
- ^ a b c McDonald, I.; Zijlstra, A. A.; Boyer, M. L. (2012). "Fundamental Parameters and Infrared Excesses of Hipparcos Stars". Monthly Notices of the Royal Astronomical Society. 427 (1): 343–57. arXiv:1208.2037. Bibcode:2012MNRAS.427..343M. doi:10.1111/j.1365-2966.2012.21873.x.
{{cite journal}}
: CS1 maint: unflagged free DOI (link)