Acrux — Double Star in Crux
HIP 60718; Alpha1 Crucis
About Acrux
Description
Acrux is the brightest star in the constellation Crux (the Southern Cross) at a combined magnitude of 0.76. It is a multiple star system located about 320 light-years from Earth. The two brightest components, Alpha1 Crucis (magnitude 1.33, spectral type B0.5IV) and Alpha2 Crucis (magnitude 1.73, spectral type B1V), are separated by about 4 arcseconds. Both are hot, massive blue stars. Alpha1 is itself a spectroscopic binary, making Acrux at least a triple system.
Observing Tips
Acrux marks the foot (southern point) of the Southern Cross and is visible only from latitudes south of about 27°N. A small telescope easily splits the two main components, which present a beautiful pair of nearly matched blue-white stars — one of the finest double stars in the sky. The color contrast with the reddish Gacrux at the top of the Cross adds to the spectacle. Acrux, together with Gacrux, points roughly toward the south celestial pole. Best observed from March through July from southern latitudes.
History
The name Acrux is a modern contraction of 'Alpha Crucis,' coined in the 19th century. The Southern Cross was known to ancient Greeks (it was visible from the Mediterranean due to precession) but gradually sank below their horizon over millennia. European explorers rediscovered it in the Age of Exploration. The Portuguese navigator João Faras made the first known European observation of the Cross in 1500.
Fun Facts
Acrux is the southernmost first-magnitude star and is depicted on the flags of five nations. The two main components of Acrux orbit each other with a period of approximately 75,000 years. Both stars are hot enough and massive enough that they will eventually explode as supernovae — a rare case of a visual double where both components are destined for the same spectacular fate.
Observe
1Physical Properties
2Position & Identifiers
3How easy to split?
| Telescope | Bortle 3 | Bortle 4 | Bortle 5 |
|---|---|---|---|
| 80 mm refractor 80mm refr. | Medium+ | Medium+ | Medium+ |
| 150 mm Newton 150mm Newt. | Easy | Easy | Easy |
| Celestron C8 (203 mm SCT) C8 203mm | Easy | Easy | Easy |
Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs
4Visibility
Set a location in User Settings to see visibility data.
5Multiple Star System Triple B: optical
Separation over time
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
A: 1.3 · B: 1.6 · Sep: 3.5″ · PA: 111° · N up, E right
Resolved · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 2.3″
Explore
7
Size Comparison
8
Compare Stars
9
Spectral Classification
10
Hertzsprung-Russell Diagram
11
Stellar Lifecycle
12
Blackbody Spectrum
13
Stellar Absorption Spectrum
Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.
14
Stellar Fusion
Discover
15Stellar Notes
16
Light Travel Time Machine
17
Relativistic Travel
Nearby in the Sky
Other targets within a few degrees — pan your scope a little and keep exploring.
Visibility scores assume a 150 mm Newton at Bortle 4.
Explore Nightbase
Related knowledge, tools, and stories — no observation planning required.