Zeta Virginis

Zeta Virginis
Diagram showing star positions and boundaries of the Virgo constellation and its surroundings
Location of ζ Virginis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Virgo
Right ascension 13h 34m 41.591s[1]
Declination –00° 35′ 44.95″[1]
Apparent magnitude (V) +3.376[2]
Characteristics
Spectral type A3 V[3]
U−B color index +0.141[2]
B−V color index +0.114[2]
Astrometry
Radial velocity (Rv)–13.2[2] km/s
Proper motion (μ) RA: –280.48 ± 0.17[1] mas/yr
Dec.: +49.05 ± 0.12[1] mas/yr
Parallax (π)44.03 ± 0.19[1] mas
Distance74.1 ± 0.3 ly
(22.71 ± 0.10 pc)
Absolute magnitude (MV)1.64±0.05[4]
Details
ζ Vir A
Mass2.041±0.024[4] M☉
Radius2.079±0.025[5] R☉
Luminosity17.885±0.252[5] L☉
Surface gravity (log g)4.12 cgs
Temperature8247±52[5] K
Rotational velocity (v sin i)222[6] km/s
Age0.51[7] Gyr
ζ Vir B
Mass0.168+0.012
−0.016[4] M☉
Other designations
Heze (primary), 79 Virginis, BD+00 3076, FK5 501, GJ 3792, HD 118098, HIP 66249, HR 5107, SAO 139420, WDS J13347-0036AB.
Database references
SIMBADdata

Zeta Virginis (ζ Virginis, abbreviated Zeta Vir, ζ Vir) is a binary star in the zodiac constellation of Virgo. It is visible to the naked eye with an apparent visual magnitude of +3.376 and is located about a half degree south of the celestial equator. Based on parallax measurements obtained during the Hipparcos mission, it is about 74 light-years (23 parsecs) distant from the Sun.

The two components are designated Zeta Virginis A (also named Heze[8]) and B.

Nomenclature

ζ Virginis (Latinised to Zeta Virginis) is the system's Bayer designation. The designations of the two components as Zeta Virginis A and B derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU).[9]

Zeta Virginis bore the traditional name Heze, which is of unclear origin,[5] though it appeared in a 1951 publication, Atlas Coeli (Skalnate Pleso Atlas of the Heavens) by Czech astronomer Antonín Bečvář. In 2016, the IAU organized a Working Group on Star Names (WGSN)[10] to catalog and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire multiple systems.[11] It approved the name Heze for the component Zeta Virginis A on 1 June 2018 and it is now so included in the List of IAU-approved Star Names.[8]

In Chinese, 角宿 (Jiǎo Xiù), meaning Horn (asterism), refers to an asterism consisting of ζ Virginis and Spica.[12] Consequently, ζ Virginis are known as 角宿二 (Jiǎo Xiù èr, English: the Second Star of Horn).[13]

Properties

The primary, Z Virginis A, is a main sequence star with a spectral class A3 V,[5] indicating that it is generating energy through the nuclear fusion of hydrogen at its core. This energy is being radiated from its outer envelope at an effective temperature of 8,247 K,[5] giving it the white hue of an A-type star.[14] It has twice the mass of the Sun and double the Sun's radius and is about a half billion years old.[5][7]

In 2010, a low mass stellar companion was discovered - Zeta Virginis B. Though it has not been under observation for a sufficient length of time to determine accurate orbital elements, it is estimated to be orbiting at an average separation of at least 24.9 AU with an orbital eccentricity of 0.16 or more and orbital period of a minimum of 124 years. This companion may be a red dwarf star, which would explain the observed X-ray flux from this system.[4]

References

  1. 1 2 3 4 5 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. Vizier catalog entry
  2. 1 2 3 4 Hipparcos star Zeta Virginis Archived January 2, 2013, at the Wayback Machine.
  3. ↑ The stars of Virgo Alcyone Ephemeris
  4. 1 2 3 4 Hinkley, Sasha (March 2010), "Discovery and Characterization of a Faint Stellar Companion to the A3V Star ζ Virginis", The Astrophysical Journal, 712 (1): 421–428, arXiv:1002.1074, Bibcode:2010ApJ...712..421H, doi:10.1088/0004-637X/712/1/421
  5. 1 2 3 4 5 6 7 Kaler, James B., "HEZE (Zeta Virginis)", Stars, University of Illinois, retrieved 2018-06-24
  6. ↑ Royer, F.; Zorec, J.; Gómez, A. E. (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 Data catalog: Bibcode: 2006yCat..34630671R
  7. 1 2 Su, K. Y. L. (December 2006), "Debris Disk Evolution around A Stars", The Astrophysical Journal, 653 (1): 675–689, arXiv:astro-ph/0608563, Bibcode:2006ApJ...653..675S, doi:10.1086/508649
  8. 1 2 "Naming Stars". IAU.org. Retrieved 18 June 2018.
  9. ↑ Hessman, F. V.; Dhillon, V. S.; Winget, D. E.; Schreiber, M. R.; Horne, K.; Marsh, T. R.; Guenther, E.; Schwope, A.; Heber, U. (2010). "On the naming convention used for multiple star systems and extrasolar planets". arXiv:1012.0707 [astro-ph.SR].
  10. ↑ "IAU Working Group on Star Names (WGSN)". Retrieved 22 May 2016.
  11. ↑ "WG Triennial Report (2015-2018) - Star Names" (PDF). p. 5. Retrieved 2018-07-14.
  12. ↑ (in Chinese) 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 978-986-7332-25-7.
  13. ↑ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 27 日
  14. ↑ "The Colour of Stars", Australia Telescope, Outreach and Education, Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, retrieved 2012-01-16
  • Boyajian, Tabetha S. et al., 2012. Stellar Diameters and Temperatures. I. Main-sequence A, F, and G Stars. The Astrophysical Journal vol 746 (1) p. 101
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