36 Camelopardalis

Binary star system in the constellation Camelopardalis From Wikipedia, the free encyclopedia

36 Camelopardalis is a single star[11] in the northern circumpolar constellation of Camelopardalis. It is visible to the naked eye as a dim point of light with an apparent visual magnitude of +5.3. Parallax measurements provide a distance estimate of approximately 710 light years away from the Sun, and it is drifting away from the Earth with a radial velocity of −1.15 km/s.

Quick facts Constellation, Right ascension ...
36 Camelopardalis
Observation data
Epoch J2000.0      Equinox ICRS
Constellation Camelopardalis
Right ascension 06h 12m 51.06255s[1]
Declination +65° 43 06.3160[1]
Apparent magnitude (V) 5.344[2]
Characteristics
Spectral type K1 III-IIIb CH-0.5[3]
U−B color index +2.708[4]
B−V color index +0.764[4]
Astrometry
Radial velocity (Rv)+1.15±0.13[5] km/s
Proper motion (μ) RA: +6.240[1] mas/yr
Dec.: −31.308[1] mas/yr
Parallax (π)4.5905±0.0728 mas[1]
Distance710 ± 10 ly
(218 ± 3 pc)
Absolute magnitude (MV)−1.33[6]
Details
Mass1.24[7] M
Radius42[8] R
Luminosity714[8] L
Surface gravity (log g)1.26[7] cgs
Temperature4,589[8] K
Metallicity [Fe/H]−0.11[7] dex
Rotational velocity (v sin i)3.0[9] km/s
Other designations
36 Cam, BD+65°517, FK5 233, GC 7856, HD 41927, HIP 2940, HR 2165, SAO 13756[10]
Database references
SIMBADdata
Close

36 Camelopardalis has a stellar classification of K1 III-IIIb, which indicates that it is a K-type giant star with a mild underabundance of CH molecules in its spectrum. At present it has 1.24 times the mass of the Sun but has expanded to an enlarged diameter of 42 R. It shines at 714 L from its photosphere at an effective temperature of 4,589 K, giving it an orange glow. 36 Cam's metallicity is around solar level and spins slowly with a projected rotational velocity of 3 km/s.

References

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