Eta Ophiuchi

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Template:Short description

Eta Ophiuchi (Sabik)
Template:Location mark
Location of η Ophiuchi (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Ophiuchus
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 2.43[2] (3.05/3.27)[3]
Characteristics
Evolutionary stage main sequence[4]
Spectral type A2V + A2V[4]
U−B Template:Engvar +0.09[2]
B−V Template:Engvar +0.05[2]
Astrometry
Radial velocity (Rv)−0.9[5] km/s
Proper motion (μ) RA: +40.13[1] mas/yr
Dec.: +99.17[1] mas/yr
Parallax (π)36.91±0.80 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Orbit[4]
Period (P)Template:Val yr
Semi-major axis (a)Template:Val
Eccentricity (e)Template:Val
Inclination (i)Template:Val°
Longitude of the node (Ω)Template:Val°
Periastron epoch (T)2024.526
Argument of periastron (ω)
(secondary)
Template:Val°
Details[4]
η Oph A (Sabik)
MassTemplate:Val Template:Solar mass
RadiusTemplate:Val Template:Solar radius
Luminosity35[6] Template:Solar luminosity
Surface gravity (log g)3.74[7] cgs
TemperatureTemplate:Val K
MetallicityTemplate:Val[7] dex
Rotational velocity (v sin i)23[8] km/s
AgeTemplate:Val Myr
η Oph B
MassTemplate:Val Template:Solar mass
RadiusTemplate:Val Template:Solar radius
Luminosity21[6] Template:Solar luminosity
TemperatureTemplate:Val K
Metallicity [Fe/H]{{{metal_fe2}}} dex
AgeTemplate:Val Myr
Other designations
Sabik, 35 Oph, BD−15°4467, GCTP 3895.00, Gl 656.1A/B, HD 155125, HIP 84012, HR 6378, SAO 160332, WDS J17104-1544AB
Database references
SIMBADdata

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Eta Ophiuchi is a binary star in the constellation of Ophiuchus. Its name is a Bayer designation that is Latinized from η Ophiuchi, and abbreviated Eta Oph or η Oph. With a combined apparent magnitude of +2.43, it is the second-brightest of the constellation and one of the brightest stars in the night sky. Based on parallax measurements taken during the Hipparcos mission, it is approximately 88 light-years away.

The components of this system are designated Template:Nobr (also called Sabik Template:IPAc-en[9][10]), and Template:Nobr.

Nomenclature

η Ophiuchi (Latinised to Eta Ophiuchi) is the system's Bayer designation. WDS J17104-1544AB is its designation in the Washington Double Star Catalog. The designations of the two components as WDS J17104-1544 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).[11]

It bore the traditional name Sabik, from the Arabic السابق al-sābiq "the preceding one", of uncertain reference.[9] In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[12] to catalogue and standardize proper names for stars. The WGSN approved the name Sabik for the component WDS J17104-1544 A on 21 August 2016 and it is now so included in the List of IAU-approved Star Names.[10]

In Chinese, this star is considered part of Script error: No such module "Lang". (Script error: No such module "Lang".), meaning Left Wall of Heavenly Market Enclosure, which refers to an asterism representing eleven old states in China that mark the left borderline of the enclosure, consisting of Eta Ophiuchi, Delta Herculis, Lambda Herculis, Mu Herculis, Omicron Herculis, 112 Herculis, Zeta Aquilae, Theta Serpentis, Eta Serpentis, Nu Ophiuchi and Xi Serpentis.[13] Consequently, the Chinese name for Eta Ophiuchi itself is Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx), representing the state Song (宋).[14][15]

Namesake

USS Sabik (AK-121) was a United States Navy Crater class cargo ship named after the star.

Properties

Eta Ophiuchi consists on two A-type main-sequence stars,[4] currently fusing hydrogen into helium at their core. The primary, of apparent magnitude +3.05,[3] has about 2.5 times the Sun's radius and 2.25 times its mass, with an effective temperature around 9,000 K.[4] The secondary, of apparent magnitude +3.27,[3] is 2 times as large and massive than the Sun, with an effective temperature of 8,700 K. The estimated age of the system is 500 million years, albeit with significant uncertainty.[4]

The stars take 87.8 years to complete an orbit, which is highly elliptical: While the semi-major axis is 31 astronomical units, the high orbital eccentricity of 0.931 take them to a distance of 2.15 au during their closest approach (the periastron); the last of such occurring in 2024. Such large eccentricity hindered accurate measurements of the stellar mass with the Kepler's third law, until observations with the Very Large Telescope during the most recent periastron accurately determined orbital elements such as the eccentricity, hence a considerable mass sum for A2V-type stars.[4]

References

Template:Reflist

Template:Stars of Ophiuchus

  1. a b c d e Cite error: Invalid <ref> tag; no text was provided for refs named aaa474_2_653
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  13. 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.
  14. 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.
  15. 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.