Beta Comae Berenices

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Beta Comae Bernices
Observation data
Epoch J2000
Constellation
(pronunciation)
Coma Berenices
Right ascension 13h 11 m 52.4s
Declination +27° 52' 41"
Apparent magnitude (V) 4.26
Characteristics
Spectral type G0V
U-B color index 0.07
B-V color index 0.57
Variable type None
Astrometry
Radial velocity (Rv) +5.2 km/s
Proper motion (μ) RA: -801.94 mas/yr
Dec.: 882.70 mas/yr
Parallax (π) 108.87 ± 0.69 mas
Distance 30 ± 0.2 ly
(9.19 ± 0.06 pc)
Absolute magnitude (MV) 4.45
Details
Mass 1.05 M
Radius 1.19 R
Luminosity 1.42 L
Temperature 6,000 K
Metallicity 146%
Rotation ~6 km/s. (~10 days)
Age 1.7-4.4 ×109 years
Other designations
43 Com, Beta Com, Gl 502, GJ 876, HD 114710, HR 4983, BD +28°2193, GCTP 3015.00, LHS 348, LFT 978, LTT 13815, SAO 82706, FK5 492, HIP 64394.

Beta Coma Berenices (β Comae Berenices / β Com) is a main sequence dwarf star in the constellation of Coma Berenices. The Greek letter beta (β) usually indicates that the star has the second highest visual magnitude in the constellation. In actuality, however, it is slightly brighter than α Comae Berenices.

This star is similar to our own Sun, being only slightly larger and brighter in absolute magnitude. The surface of this star has a measured activity cycle of 16.6 years (compared to 11 years on our Sun.) It may also have a secondary activity cycle of 9.6 years. At one time it was thought that this star may have a spectroscopic companion. However this was ruled out by means of more accurate radial velocity measurements. No planets have yet been detected around this star, and there is no evidence of a dusty disk.

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