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Zuben Elgenubi — Double Star in Libra

HIP 72622; Alpha2 Librae; 9 Librae

Observable Double Star Good (43/100)

Sep: 230.8", Companion: mag 5.2

Magnitude 2.8m DoubleStar Libra (Lib) Visible
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About Zuben Elgenubi

Description

Zuben Elgenubi is a wide double star system at magnitude 2.75 in Libra, the second brightest star in the constellation. A white subgiant of spectral type A3IV, located about 77 light-years from Earth. A telescope reveals a fainter companion (magnitude 5.2) about 231 arcseconds away, making it one of the widest bright double stars in the sky.

Observing Tips

Zuben Elgenubi is the more southerly of Libra's two main stars, forming the southern pan of the Scales with Zuben Elschemali to the north. The wide companion is visible in binoculars. The pair lies between Virgo and Scorpius on the ecliptic. Best observed May through July.

History

The name Zuben Elgenubi comes from the Arabic 'al-zuban al-janubi,' meaning 'the southern claw,' from when Libra's stars were considered part of Scorpius. The Romans separated them into Libra, the only zodiacal constellation representing an inanimate object.

Fun Facts

The ecliptic passes very close to Zuben Elgenubi, making it one of the most frequently occulted bright stars. The Moon and planets regularly pass over it, and it has been used to study the lunar limb profile during occultations.

Observe

1Physical Properties

Magnitude 2.75
Spectral Type A3 III/V giant
Star Color White (B-V 0.15)
Distance 76 ly

2Position & Identifiers

RA 14h 50m 52.7s
Dec -16° 02' 30.0"
Constellation Libra (Lib)
HR 5531
HIP 72622
HD 130841
SAO 158840
Bayer Alpha2
Flamsteed 9 Lib

3How easy to split?

Primary 2.8 mag Companion 5.2 mag Separation 230.8″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Easy Easy Easy
150mm Newt. Easy Easy Easy
C8 203mm Easy Easy Easy
Easy Medium Hard Very hard Impossible

Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs

4Visibility

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Best season Mar – May (peak: Apr)

5Multiple Star System Triple C,E: optical

Components 3 (triple)
Component IDs O
Separation 230.8″
Companion Mag 5.2
Companion Sp F4IV
Position Angle 314°
Star Colors A: White B: Yellow-white
Discoverer SHJ 186
CPM with HR 5530. Suspected occultation double.

Separation over time

Measured 1836 → 2016 (180 y)
Separation drift 229.0" → 230.8" (+1.80")
Rate +0.0100" / y
PA drift 314° → 314° (+0°, +0.000°/y)

Slow change over generations — observable in lifetime comparisons.

Measured from the WDS observational archive. No orbital solution has been derived — most likely the period is too long to fit an orbit to the available measurement arc.

Eyepiece View

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32x Dawes: 1.9″ TFOV: 1.6°
Realistic = true angular size
N E 314°

A: 2.8 · B: 5.2 · Sep: 230.8″ · PA: 314° · N up, E right

Resolved · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 2.3″

Explore

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Size Comparison

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Spectral Classification

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Hertzsprung-Russell Diagram

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Stellar Lifecycle

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Blackbody Spectrum

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Stellar Absorption Spectrum

Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.

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Stellar Fusion

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15Stellar Notes

Zuben Elgenubi; Zubenelgenubi; Kiffa Australis; Elkhiffa Australis.
About 2 solar radii.
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Light Travel Time Machine

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Relativistic Travel

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