41 Comae Berenices

41 Comae Berenices is a single, orange-hued star in the northern constellation of Coma Berenices. It is visible to the naked eye, having an apparent visual magnitude of 4.80. Based upon an annual parallax shift of 8.6 mas, it is located around 379 light years away. It is moving closer to the Earth with a heliocentric radial velocity of −16 km/s.

41 Comae Berenices
Observation data
Epoch J2000      Equinox J2000
Constellation Coma Berenices
Right ascension 13h 07m 10.72992s
Declination +27° 37 29.0554
Apparent magnitude (V) 4.80±0.02
Characteristics
Evolutionary stage giant star
Spectral type K5-III
B−V color index 1.482±0.003
Astrometry
Radial velocity (Rv)−15.89±0.13 km/s
Proper motion (μ) RA: +34.155 mas/yr
Dec.: −69.539 mas/yr
Parallax (π)8.5989 ± 0.1327 mas
Distance379 ± 6 ly
(116 ± 2 pc)
Absolute magnitude (MV)−0.04
Details
Mass1.21±0.19 M
Radius33.75±0.77 R
Luminosity323.0±21.7 L
Surface gravity (log g)1.70 cgs
Temperature4,211±54 K
Metallicity [Fe/H]−0.09 dex
Rotational velocity (v sin i)1.8 km/s
Age4.51±1.84 Gyr
Other designations
36 Com, BD+28°2185, FK5 3045, HD 113996, HIP 64022, HR 4954, SAO 82659
Database references
SIMBADdata

At the age of about 4.5 billion years, this is an evolved giant star with a stellar classification of K5-III, currently on the red giant branch. It has 1.2 times the mass of the Sun and, after consuming the hydrogen at its core, has expanded to 34 times the Sun's radius. The star is radiating 323 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,211 K.

In 2017, one planet (HD 113996 b) was found orbiting it via the radial velocity method. The planet has a mass of at least 6.3±1.0 MJ, a semi-major axis of 1.6±0.1 AU, an orbital period of 610.2±3.8 d, and an eccentricity of 0.28±0.12.

The 41 Comae Berenices planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b ≥6.3±1.0 MJ 1.6±0.1 610.2±3.8 0.28±0.12
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