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10 Canum Venaticorum

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Star in the constellation Canes Venatici Canes Venatici constellation map.svg center 280 right Red circle.svg 10 10 Canum Venaticorum 580 410 Location of 10 Canum Venaticorum (circled in red) J2000 12 44 59.405 +39 16 44.10 5.95 Canes Venatici Main sequence G0 V +0.55 –0.03 +80.3 –359.699 +139.016 56.9588 0.0323 4.76 0.87 0.04 0.03 0.98 0.02 4.29 6.3 –0.53 1.104 0.002 5968 58 41 commas 8.11 13 days 10 CVn +40°2570 484 110897 62207 4845 63177 10+CVn 10 Canum Venaticorum is an ordinary star in the northern constellation of Canes Venatici. It has an apparent visual magnitude of 5.95, which, according to the Bortle scale, can be faintly seen with the naked eye from suburban locations. Based upon an annual parallax shift of 0.057 arcseconds, this system is 17.557 pc ly off on flip from Sun. It is drifting further away with a radial velocity of +80 km/s. The stellar classification of 10 Canum Venaticorum is G0 V, indicating that it is a G-type main sequence star that is fusing hydrogen into helium at its core to generate energy. The NStars project found a similar class of F9V Fe−0.3, indicating a mild underabundance of iron. It is older than the Sun, with an estimated age of six billion years. The star has around 98% of the Sun's radius and 87% of the solar mass. It rotates about the axis an average of once every 13 days, with a projected rotational velocity along the equator of 8 km/s. The abundance of elements other than hydrogen and helium is lower than in the Sun. The effective temperature of the stellar atmosphere is 5,968 K, giving it the yellow hue of a G-type star. An excess of infrared emission at a wavelength of 70 μm suggests the presence of a debris disk. The best fit disk model suggest a broad dust annulus with a peak brightness at a radius of 53.7 AU, that is inclined by an angle of 56° to the line of sight from the Earth along a position angle of 111.2°. References 1521686782461765888 1521686782461765888 1 Gray R. O. C. J. Corbally R. F. Garrison M. T. McFadden P. E. Robinson Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 parsecs: The Northern Sample I https://archive.org/details/sim_astronomical-journal_2006-07_132_1/page/161 The Astronomical Journal 132 1 161–170 July 2006 2006AJ....132..161G astro-ph/0603770 10.1086/504637 119476992 1 Maldonado J. Eiroa C. Villaver E. Montesinos B. Mora A. Metallicity of solar-type stars with debris discs and planets Astronomy and Astrophysics 541 May 2012 A40 10.1051/0004-6361/201218800 2012A&A...541A..40M 1202.5884 46328823 . 1 Nordström B. Mayor M. Andersen J. Holmberg J. Pont F. Jørgensen B. R. Olsen E. H. Udry S. Mowlavi N. The Geneva-Copenhagen survey of the Solar neighbourhood. Ages, metallicities, and kinematic properties of ˜14,000 F and G dwarfs Astronomy and Astrophysics 418 989–1019 May 2004 10.1051/0004-6361:20035959 2004A&A...418..989N astro-ph/0405198 11027621 . 1 Trilling D. E. Bryden G. Beichman C. A. Rieke G. H. Su K. Y. L. Stansberry J. A. Blaylock M. Stapelfeldt K. R. Beeman J. W. Haller E. E. Debris Disks around Sun-like Stars The Astrophysical Journal 674 2 1086–1105 February 2008 10.1086/525514 2008ApJ...674.1086T 0710.5498 54940779 . 1 Martínez-Arnáiz R. Maldonado J. Montes D. Eiroa C. Montesinos B. Chromospheric activity and rotation of FGK stars in the solar vicinity. An estimation of the radial velocity jitter Astronomy and Astrophysics 520 A79 September 2010 10.1051/0004-6361/200913725 2010A&A...520A..79M 1002.4391 43455849 . http://eprints.ucm.es/37826/1/davidmontes17libre.pdf 2018-11-04 2017-09-22 https://web.archive.org/web/20170922031257/http://eprints.ucm.es/37826/1/davidmontes17libre.pdf dead 1 Johnson H. L. Iriarte B. Mitchell R. I. Wisniewskj W. Z. UBVRIJKL photometry of the bright stars Communications of the Lunar and Planetary Laboratory 4 99 1966 99 1966CoLPL...4...99J . The Colour of Stars December 21, 2004 Australia Telescope, Outreach and Education Commonwealth Scientific and Industrial Research Organisation http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html 2012-01-16 . dead https://web.archive.org/web/20120318151427/http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html March 18, 2012 10 CVn -- High proper-motion Star SIMBAD Astronomical Database Centre de Données astronomiques de Strasbourg http://simbad.u-strasbg.fr/simbad/sim-id?Ident=10+Canum+Venaticorum 2014-01-26 . 1 Ramírez I. Fish J. R. Lambert D. L. Allende Prieto C. Lithium Abundances in nearby FGK Dwarf and Subgiant Stars: Internal Destruction, Galactic Chemical Evolution, and Exoplanets The Astrophysical Journal 756 1 46 September 2012 10.1088/0004-637X/756/1/46 2012ApJ...756...46R 1207.0499 119199829 1 Marshall J. P. Kirchschlager F. Ertel S. Augereau J.-C. Kennedy G. M. Booth M. Wolf S. Montesinos B. Eiroa C. Matthews B. Interpreting the extended emission around three nearby debris disc host stars Astronomy & Astrophysics 570 A114 13 October 2014 10.1051/0004-6361/201424517 2014A&A...570A.114M 1408.5649 119232172 . Category:Canes Venatici Category:Solar-type stars Category:Circumstellar disks Canum Venaticorum, 10 4845 0484 110897 BD+40 2570 062207 Category:G0V stars