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Pi Virginis

From Wikipedia, the free encyclopedia
Binary star in the constellation Virgo
π Virginis
Location of π Virginis (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationVirgo
Right ascension12h 00m 52.39042s[1]
Declination+06° 36′ 51.5571″[1]
Apparent magnitude (V)4.64[2]
Characteristics
Spectral typeA5 V[3]
U−Bcolor index+0.12[2]
B−Vcolor index+0.12[2]
Astrometry
Radial velocity (Rv)−10.4[4] km/s
Proper motion (μ)RA: +0.26[1]mas/yr
Dec.: −30.10[1]mas/yr
Parallax (π)8.49±0.39 mas[1]
Distance380 ± 20 ly
(118 ± 5 pc)
Absolute magnitude (MV)−0.70[5]
Orbit[6]
Primaryπ Virginis A
Companionπ Virginis B
Period (P)282.69 days
Semi-major axis (a)3.55 mas
Eccentricity (e)0.265
Inclination (i)62.71°
Longitude of the node (Ω)149.34°
Periastronepoch (T)2448281.3906
Argument of periastron (ω)
(secondary)
312°
Semi-amplitude (K1)
(primary)
26.20[7] km/s
Details
π Vir A
Mass2.2[7] M
Radius1.5[8] R
Surface gravity (log g)3.51[9] cgs
Temperature8,000[9] K
Rotational velocity (v sin i)71[3] km/s
Other designations
BD+07°2502,FK5 1311,HD 104321,HIP 58590,HR 4589,SAO 119164[10]
Database references
SIMBADdata

Pi Virginis (π Vir, π Virginis) is abinary star in thezodiacconstellation ofVirgo. It is visible to the naked eye with anapparent visual magnitude of 4.64.[2] The distance to this star, based uponparallax measurements,[1] is roughly 380 light years.

This is aspectroscopic binary system with astellar classification of A5V. They have anorbital period of 283 days with aneccentricity of 0.27.[7] The mass ratio of the two stars is about 0.47, with the primary having an estimated mass of around 2.2 times that of the Sun. The primary is a cool metallic-linedAm star.[9]

References

[edit]
  1. ^abcdefvan Leeuwen, F. (November 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.
  2. ^abcdMermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)",Catalogue of Eggen's UBV Data,Bibcode:1986EgUBV........0M.
  3. ^abRoyer, F.; et al. (February 2007), "Rotational velocities of A-type stars. III. Velocity distributions",Astronomy and Astrophysics,463 (2):671–682,arXiv:astro-ph/0610785,Bibcode:2007A&A...463..671R,doi:10.1051/0004-6361:20065224,S2CID 18475298.
  4. ^Evans, D. S. (June 20–24, 1966), Batten, Alan Henry; Heard, John Frederick (eds.), "The Revision of the General Catalogue of Radial Velocities",Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30, vol. 30, University of Toronto:International Astronomical Union, p. 57,Bibcode:1967IAUS...30...57E.
  5. ^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,S2CID 119257644.
  6. ^ESA (1997). "The Hipparcos and Tycho Catalogues".VizieR On-line Data Catalog.Bibcode:1997yCat.1239....0E.
  7. ^abcDucati, J. R.; et al. (January 2011),"The mass ratio and initial mass functions in spectroscopic binaries"(PDF),Astronomy and Astrophysics,525: 9,Bibcode:2011A&A...525A..26D,doi:10.1051/0004-6361/200913895,hdl:10183/99264, A26.
  8. ^Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics",Astronomy and Astrophysics,367 (2):521–524,arXiv:astro-ph/0012289,Bibcode:2001A&A...367..521P,doi:10.1051/0004-6361:20000451,S2CID 425754.
  9. ^abcPaunzen, E.; et al. (February 2013), "A photometric study of chemically peculiar stars with the STEREO satellites - II. Non-magnetic chemically peculiar stars",Monthly Notices of the Royal Astronomical Society,429 (1):119–125,arXiv:1211.1535,Bibcode:2013MNRAS.429..119P,doi:10.1093/mnras/sts318,S2CID 119231581.
  10. ^"pi. Vir -- Spectroscopic binary",SIMBAD Astronomical Database, Centre de Données astronomiques de Strasbourg, retrieved2016-09-16.
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