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Agena — Double Star in Centaurus

HIP 68702; Beta Centauri

Magnitude 0.6m DoubleStar Centaurus (Cen) Visible
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About Agena

Description

Agena (also known as Hadar) is the second brightest star in Centaurus and the 11th brightest in the night sky at magnitude 0.61. It is a giant star of spectral type B1III located about 390 light-years from Earth. Agena is actually a triple star system: the primary is a spectroscopic binary of two blue giant stars orbiting each other every 357 days, with a more distant third companion. The system's combined luminosity is about 41,000 times that of the Sun.

Observing Tips

Agena is a Southern Hemisphere object, visible only from latitudes south of about 30°N. Together with Alpha Centauri, it forms the 'Southern Pointers' — the two bright stars that point toward the Southern Cross (Crux), a vital navigation aid in the southern sky. The two stars are about 4.5 degrees apart and make a striking pair. Best observed from March through September from southern latitudes.

History

The name Hadar comes from the Arabic for 'ground' or 'soil,' possibly referring to its low position as seen from Arabian latitudes. The alternative name Agena is Latin, possibly meaning 'the knee.' Along with Alpha Centauri, it has been used by Polynesian and Aboriginal Australian navigators for centuries. Its spectroscopic binary nature was discovered in the early 20th century.

Fun Facts

Despite being 100 times farther away than Alpha Centauri, Agena appears almost as bright because it is intrinsically far more luminous. The two stars serve as reliable pointers to the Southern Cross — a line drawn through them leads directly to Gacrux (Gamma Crucis) at the top of the Cross.

Observe

1Physical Properties

Magnitude 0.61
Variable Type Beta Cephei (Pulsating)
Spectral Type B1II-III bright giant
Star Color Blue (B-V -0.23)
Temperature 25011 K
Radius 9.1 R☉
Distance 391 ly

2Position & Identifiers

RA 14h 03m 49.4s
Dec -60° 22' 23.0"
Constellation Centaurus (Cen)
HR 5267
HIP 68702
HD 122451
SAO 252582
Bayer Beta
Variable ID Bet Cen

3How easy to spot?

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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Easy Easy Easy
50mm finder Easy Easy Easy
150mm scope 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

Separation 0.2″
Companion Mag 4.0
Position Angle 142°
Star Colors A: Blue B: Blue
Discoverer VOU 31

Separation over time

Period: 133.3 y Eccentricity: 0.802 Now: 0.18", PA 93° + 0.09" in 5 years
0.00" 0.26" 0.52" 0.77" 1.0" 2025 2030 2035 2040 2045 0.18"

Apparent separation over time, computed from ORB6 orbital elements. Steep curves indicate fast-changing pairs — catch them while they're splittable.

Explore

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Size Comparison

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Compare Stars

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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

Beta C? Amp. 0.07V, 0.157d, modulation 352d. Line profiles also vary per. 0.157d.
0.157d and 352d. Interferometer measures indicate multiple star.
Color excess E(B-V) = +0.02. Soft X-ray source.
Sco-Cen assoc.
Lyman alpha observed from COPERNICUS; spectra revealed MgII emission.
AGENA; HADAR.
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Light Travel Time Machine

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Relativistic Travel

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