HD 33564

HD 33564
Observation data
Epoch J2000      Equinox J2000
Constellation Camelopardalis
Right ascension 05h 22m 33.5306s
Declination +79° 13 52.143
Apparent magnitude (V) 5.08
Characteristics
Spectral type F7V
U−B color index −0.13
B−V color index 0.506±0.002
Astrometry
Radial velocity (Rv)−11.09(13) km/s
Proper motion (μ) RA: −78.661(67) mas/yr
Dec.: 162.098(77) mas/yr
Parallax (π)48.1098±0.0727 mas
Distance67.8 ± 0.1 ly
(20.79 ± 0.03 pc)
Absolute magnitude (MV)3.59
Details
Mass1.29 M
Radius1.51+0.02
−0.06
 R
Luminosity3.428±0.017 L
Surface gravity (log g)4.22 cgs
Temperature6,396+135
−36
 K
Metallicity [Fe/H]0.14 dex
Rotational velocity (v sin i)14.3 km/s
Age1.80 Gyr
Other designations
BD+79°169, GC 6455, HD 33564, HIP 25110, HR 1686, SAO 5496, K Cam
Database references
SIMBADdata

HD 33564 (K Camelopardalis) is a single star with an exoplanetary companion in the northern constellation of Camelopardalis. It has an apparent visual magnitude of 5.08, which means it is a 5th magnitude star that is faintly visible to the naked eye. The system is located at a distance of 68 light years from the Sun based on parallax, and it is drifting closer with a radial velocity of −11 km/s. It is a candidate member of the Ursa Major Moving Group.

This is an ordinary F-type main-sequence star with a stellar classification of F7V, indicating that the star is hotter and more massive than the Sun, giving it a yellow-white hue. The star is about two billion years old and is chromospherically quiet, with a projected rotational velocity of 14.3 km/s. It has about 1.5 times the radius and 1.3 times the mass of the Sun. The star is radiating 3.4 times the luminosity of the Sun from its photosphere at an effective temperature of 6,396 K.