Agena
HIP 68702; Beta Cen
Physical Properties
Position & Identifiers
Visibility
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Multiple Star System
Eyepiece View
Sep: 0.2″ · PA: 142° · N up, E left
Unresolved · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 3.1″
Size Comparison
Stellar Lifecycle
Spectral Classification
Hertzsprung-Russell Diagram
Blackbody Spectrum
Stellar Absorption Spectrum
Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.
Stellar Notes
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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.