7 Comae Berenices

7 Comae Berenices
Observation data; Epoch 2000.0 Equinox 2000.0
Constellation	Coma Berenices
Right ascension	12h 16m 20.53831s[1]
Declination	+23° 56′ 43.4700″[1]
Apparent magnitude (V)	4.93[2]
Characteristics
Evolutionary stage	horizontal branch
Spectral type	G8 III–IIIb[3]
B−V color index	0.957[2]
Astrometry
Radial velocity (Rv)	−27.89±0.13[4] km/s
Proper motion (μ)	RA: −26.55[1] mas/yr ; Dec.: −6.22[1] mas/yr
Parallax (π)	13.08 ± 0.30[1] mas
Distance	249 ± 6 ly ; (76 ± 2 pc)
Absolute magnitude (MV)	+0.51[2]
Details[4]
Mass	2.37±0.16 M☉
Radius	10.07±0.66 R☉
Luminosity	63+14; −12 L☉
Surface gravity (log g)	2.95±0.08 cgs
Temperature	5,023±25 K
Metallicity [Fe/H]	−0.09±0.05 dex
Rotational velocity (v sin i)	2.26±0.45 km/s
Age	730±150 Myr
Other designations
	7 Com, BD+24°2443, FK5 2982, HD 106714, HIP 59847, HR 4667, SAO 82211[5]
Database references
SIMBAD	data

7 Comae Berenices is a single[6] star located 249[1] light years away in the northern constellation of Coma Berenices. It is a dim star but visible to the naked eye near the Coma Star Cluster with an apparent visual magnitude of 4.93.[2] The star is moving closer to the Earth with a heliocentric radial velocity of −28 km/s,[4] and is predicted to come as close as 83 light-years in 2.4 million years.[2]

This is an evolved giant star with a stellar classification of G8 III–IIIb.[3] At the age of 730 million years it is a red clump giant, which indicates it is on the horizontal branch and is generating energy via helium fusion at its core.[7] The star has 2.4 times the mass of the Sun and has expanded to 10 times the Sun's radius. It is radiating about 63 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 5,023 K.[4]

References

van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357.
Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv:1108.4971, Bibcode:2012AstL...38..331A, doi:10.1134/S1063773712050015.
Keenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins catalog of revised MK types for the cooler stars", Astrophysical Journal Supplement Series, 71: 245, Bibcode:1989ApJS...71..245K, doi:10.1086/191373.
Jofré, E.; et al. (2015), "Stellar parameters and chemical abundances of 223 evolved stars with and without planets", Astronomy & Astrophysics, 574: A50, arXiv:1410.6422, Bibcode:2015A&A...574A..50J, doi:10.1051/0004-6361/201424474.
"7 Com". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved December 30, 2018.
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, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x.
Mishenina, T. V.; et al. (September 2006), "Elemental abundances in the atmosphere of clump giants", Astronomy and Astrophysics, 456 (3): 1109–1120, arXiv:astro-ph/0605615, Bibcode:2006A&A...456.1109M, doi:10.1051/0004-6361:20065141.

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.

[vanLeeuwen2007-1] van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357.

[Anderson2012-2] Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv:1108.4971, Bibcode:2012AstL...38..331A, doi:10.1134/S1063773712050015.

[perkins1989-3] Keenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins catalog of revised MK types for the cooler stars", Astrophysical Journal Supplement Series, 71: 245, Bibcode:1989ApJS...71..245K, doi:10.1086/191373.

[jofre2015-4] Jofré, E.; et al. (2015), "Stellar parameters and chemical abundances of 223 evolved stars with and without planets", Astronomy & Astrophysics, 574: A50, arXiv:1410.6422, Bibcode:2015A&A...574A..50J, doi:10.1051/0004-6361/201424474.

[SIMBAD-5] "7 Com". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved December 30, 2018.

[Eggleton2008-6] 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, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x.

[Mishenina2006-7] Mishenina, T. V.; et al. (September 2006), "Elemental abundances in the atmosphere of clump giants", Astronomy and Astrophysics, 456 (3): 1109–1120, arXiv:astro-ph/0605615, Bibcode:2006A&A...456.1109M, doi:10.1051/0004-6361:20065141.