F-type main sequence star in the constellation Virgo
Mu Virginis , Latinized from μ Virginis, is a star in the zodiac constellation of Virgo . It was listed in the Calendarium of Al Achsasi al Mouakket as rijl al-‘awwā’ , Arabic رجل العواء, meaning "The foot of the barking (dog)".[ 10] With an apparent visual magnitude of 3.88,[ 2] it is bright enough to be seen with the naked eye. The position of the star near the celestial equator means it is visible from most of the Earth . Based upon parallax measurements, Mu Virginis is located some 59.6 light-years from the Sun .
Rijl al Awwa is an F-type main-sequence star with a stellar classification of F2 V,[ 4] although it does show some evidence of being a more evolved star .[ 6] It has an effective temperature of 6,751[ 4] K in its outer atmosphere .[ 4] The estimated age of the star is 1.5 billion years, and it has a relatively high 47.0[ 8] km/s projected rotational velocity . A 1990 study of the star gave it a giant star classification, and modeled it with 1.7 times the mass of the Sun, 2.1 times the Sun's radius, and shining with 9.8 times the Sun's luminosity .[ 11]
Past observations of this star show some indications of short-term chromospheric variability as well as radial velocity variations.[ 6] It has a candidate common proper motion companion at a projected separation of 770 AU . This object has a J band magnitude of 10.72.[ 12]
References
^ a b c d e 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 , S2CID 18759600 .
^ a b c d Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data , SIMBAD , Bibcode :1986EgUBV........0M .
^ a b c Holmberg, J.; et al. (July 2009), "The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics", Astronomy and Astrophysics , 501 (3): 941– 947, arXiv :0811.3982 , Bibcode :2009A&A...501..941H , doi :10.1051/0004-6361/200811191 , S2CID 118577511 .
^ a b c d e f g Gray, R. O.; et al. (July 2006), "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample", The Astronomical Journal , 132 (1): 161– 170, arXiv :astro-ph/0603770 , Bibcode :2006AJ....132..161G , doi :10.1086/504637 , S2CID 119476992 .
^ Gontcharov, G. A. (November 2006), "Pulkovo Compilation of Radial Velocities for 35,495 Hipparcos stars in a common system", Astronomy Letters , 32 (11): 759– 771, arXiv :1606.08053 , Bibcode :2006AstL...32..759G , doi :10.1134/S1063773706110065 , S2CID 119231169 .
^ a b c Rachford, Brian L.; Foight, Dillon R. (June 2009), "Chromospheric Variability in Early F-Type Stars", The Astrophysical Journal , 698 (1): 786– 802, arXiv :0904.1620 , Bibcode :2009ApJ...698..786R , doi :10.1088/0004-637X/698/1/786 , S2CID 693296 .
^ Moro-Martín, A.; et al. (2015), "Does the Presence of Planets Affect the Frequency and Properties of Extrasolar Kuiper Belts? Results from the Herschel Debris and Dunes Surveys", The Astrophysical Journal , 801 (2): 143, arXiv :1501.03813 , Bibcode :2015ApJ...801..143M , doi :10.1088/0004-637X/801/2/143 , S2CID 55170390 .
^ a b [permanent dead link ]
^ "* mu. Vir" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2016-09-08 .{{cite web }}
: CS1 maint: postscript (link )
^ Allen, R. H. (1963), Star Names: Their Lore and Meaning (Reprint ed.), New York, NY: Dover Publications Inc., pp. 473 , ISBN 0-486-21079-0
^ Malagnini, M. L.; Morossi, C. (November 1990), "Accurate absolute luminosities, effective temperatures, radii, masses and surface gravities for a selected sample of field stars", Astronomy and Astrophysics Supplement Series , 85 (3): 1015– 1019, Bibcode :1990A&AS...85.1015M .
^ Chini, R.; et al. (January 2014), "New visual companions of solar-type stars within 25 pc", Monthly Notices of the Royal Astronomical Society , 437 (1): 879– 886, arXiv :1310.2684 , Bibcode :2014MNRAS.437..879C , doi :10.1093/mnras/stt1953 , S2CID 118717758 .
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