Astronomy:41 Comae Berenices

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Short description: Star in the constellation Coma Berenices
41 Comae Berenices
Observation data
Equinox J2000.0]] (ICRS)
Constellation Coma Berenices
Right ascension  13h 07m 10.72992s[1]
Declination +27° 37′ 29.0554″[1]
Apparent magnitude (V) 4.80±0.02[2]
Characteristics
Evolutionary stage giant star
Spectral type K5-III[3]
B−V color index 1.482±0.003[4]
Astrometry
Radial velocity (Rv)−15.89±0.13[1] km/s
Proper motion (μ) RA: +34.155[1] mas/yr
Dec.: −69.539[1] mas/yr
Parallax (π)8.5989 ± 0.1327[1] mas
Distance379 ± 6 ly
(116 ± 2 pc)
Absolute magnitude (MV)−0.04[5]
Details[2]
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[6] km/s
Age4.51±1.84 Gyr
Other designations
36 Com, BD+28°2185, FK5 3045, HD 113996, HIP 64022, HR 4954, SAO 82659[7]
Database references
SIMBADdata

41 Comae Berenices is a single,[8] 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.[2] 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.[1]

At the age of about 4.5 billion years, this is an evolved giant star with a stellar classification of K5-III,[3] currently on the red giant branch.[9] 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.[2]

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 Jupiter mass, a semi-major axis of 1.6±0.1 astronomical unit|AU, an orbital period of 610.2±3.8 d, and an eccentricity of 0.28±0.12.[9][10]

The 41 Comae Berenices planetary system[9]
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

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  2. 2.0 2.1 2.2 2.3 Baines, E. et al. (2017), "Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer", The Astronomical Journal 155 (1): 30, doi:10.3847/1538-3881/aa9d8b, Bibcode2018AJ....155...30B. 
  3. 3.0 3.1 Keenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins catalog of revised MK types for the cooler stars", Astrophysical Journal Supplement Series 71: 245, doi:10.1086/191373, Bibcode1989ApJS...71..245K. 
  4. Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode2012AstL...38..331A. 
  5. Cardini, D. (January 2005), "Mg II chromospheric radiative loss rates in cool active and quiet stars", Astronomy and Astrophysics 430: 303–311, doi:10.1051/0004-6361:20041440, Bibcode2005A&A...430..303C. 
  6. De Medeiros, J. R. et al. (November 2000), "Rotation and lithium in single giant stars", Astronomy and Astrophysics 363: 239–243, Bibcode2000A&A...363..239D. 
  7. "41 Com". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=41+Com. 
  8. Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society 389 (2): 869–879, doi:10.1111/j.1365-2966.2008.13596.x, Bibcode2008MNRAS.389..869E. 
  9. 9.0 9.1 9.2 Jeong, G. et al. (February 2018), "Detection of planet candidates around K giants. HD 40956, HD 111591, and HD 113996", Astronomy & Astrophysics 610: 8, doi:10.1051/0004-6361/201629185, A3, Bibcode2018A&A...610A...3J. 
  10. HD 113996 b at the Open Exoplanet Catalogue. Available at https://exoplanet.eu/catalog/hd_113996_b--6676/. Accessed 28 November 2017.