Eta Virginis

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Template:Short description

η Virginis
(incl. Zaniah)
Template:Location mark
Location of η Virginis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Virgo
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 3.890[2]
Characteristics
Spectral type A2 V[3]
U−B Template:Engvar +0.055[2]
B−V Template:Engvar +0.029[2]
Astrometry
Radial velocity (Rv)+2.3[4] km/s
Proper motion (μ) RA: −57.58[1] mas/yr
Dec.: −25.19[1] mas/yr
Parallax (π)13.264±0.161 mas[5]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)−0.66[6]
Orbit[7]
Primaryη Vir Aa
Companionη Vir Ab
Period (P)Template:Val
Semi-major axis (a)Template:Val
Eccentricity (e)Template:Val
Inclination (i)Template:Val°
Orbit[7]
Primaryη Vir A
Companionη Vir B
Period (P)Template:Val
Semi-major axis (a)Template:Val
Eccentricity (e)Template:Val
Inclination (i)Template:Val°
Details
η Vir Aa
MassTemplate:Val[8] Template:Solar mass
Surface gravity (log g)3.0[9] cgs
Temperature9,333[9] K
Metallicity [Fe/H]+0.11[9] dex
Rotational velocity (v sin i)18[10] km/s
η Vir Ab
MassTemplate:Val Template:Solar mass
Metallicity [Fe/H]{{{metal_fe2}}} dex
Details[7]
η Vir B
MassTemplate:Val Template:Solar mass
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Zaniah, 15 Virginis, HR 4689, HD 107259, BD+00°2926, FK5 460, HIP 60129, SAO 138721, CCDM 12199-0040, WDS J12199-0040[11]
Database references
SIMBADdata

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Eta Virginis (η Virginis, abbreviated Eta Vir, η Vir) is a triple star system in the zodiac constellation of Virgo. From parallax measurements, it is about Template:Convert from the Sun.[5] It has a combined apparent visual magnitude of 3.89,[2] bright enough to be seen with the naked eye in dark skies.

The system consists of[12] a binary pair designated Eta Virginis A together with a third companion, Eta Virginis B. A's two components are themselves designated Eta Virginis Aa (officially named Zaniah Template:IPAc-en, the traditional name of the system)[13][14] and Ab.

Nomenclature

η Virginis (Latinised to Eta Virginis) is the system's Bayer designation. The designations of the two constituents as Eta Virginis A and those of A's components - Eta Virginis Aa and Ab - derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU).[15]

It bore the traditional name Zaniah Template:IPAc-en, derived from the Arabic زاوية zāwiyah "corner", the same source as Zavijava (Beta Virginis). In 2016, the IAU organized a Working Group on Star Names (WGSN)[16] to catalogue and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire multiple systems.[17] It approved the name Zaniah for the component Eta Virginis Aa on 12 September 2016 and it is now so included in the List of IAU-approved Star Names.[14]

In the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, this star was designated Thanih al Aoua, which was translated into Latin as Secunda Latratoris, meaning "the second barker".[18] This star, along with Beta Virginis (Zavijava), Gamma Virginis (Porrima), Delta Virginis (Minelauva) and Epsilon Virginis (Vindemiatrix), were Al ʽAwwāʼ, "the Barker".[19]

In Chinese, Script error: No such module "Lang". (Script error: No such module "Lang".), meaning Left Wall of Supreme Palace Enclosure, refers to an asterism consisting of Eta Virginis, Gamma Virginis, Delta Virginis, Epsilon Virginis and Alpha Comae Berenices.[20] Consequently, the Chinese name for Eta Virginis itself is Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx.),[21] representing Script error: No such module "Lang". (Script error: No such module "Lang".), meaning "The Left Law Administrator".[22] 左執法 (Zuǒzhífǎ), spelled Tso Chih Fa by R.H. Allen, means "the Left-hand Maintainer of Law" [23]

Properties

File:Virgo constellation PP3 map PL.svg
Chart of Virgo

Eta Virginis looks single, but lunar occultations have shown it to be a very close triple star system consisting of two stars 0.6 AU apart, assuming a distance of 91 parsecs, with a third slightly more distant star. The inner pair is a spectroscopic binary that completes an orbit in 72 days. The inclination of this orbit was determined through interferometer observations to be 45.5°, allowing the masses of the two stars to be estimated. The primary star, Eta Virginis Aa, has a mass about 2.5 times the Sun's mass, while the secondary, Eta Virginis Ab, has 1.9 solar masses. The faint tertiary star, Eta Virginis B, orbits the inner group in a wider orbit over a period of 13.1 years.[8]

Eta Virginis is 1.97 degrees north of the ecliptic, so it can be occulted by the Moon and (rarely) by planets. On October 12, 272 BC the ancient Greek astronomer Timocharis observed a conjunction of the star with Venus.[24][25] The last occultation by a planet took place on September 27, 1843, also by Venus, which will occult it again on September 30, 2078.Script error: No such module "Unsubst".

Two degrees north-following of Eta Virginis is SS Virginis, a typical cool carbon star and one of the most red-colored stars in the equatorial sky.

References

Template:Reflist

External links

Template:Virgo

Template:Authority control

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  20. Template:In lang 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, Template:ISBN.
  21. Template:In lang 香港太空館 - 研究資源 - 亮星中英對照表 Template:Webarchive, Hong Kong Space Museum. Accessed on line November 23, 2010.
  22. Template:In lang English-Chinese Glossary of Chinese Star Regions, Asterisms and Star Name Template:Webarchive, Hong Kong Space Museum. Accessed on line November 23, 2010.
  23. Richard Hinckley Allen: Star Names — Their Lore and Meaning: Virgo
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  25. Cite error: Invalid <ref> tag; no text was provided for refs named ptolemy