Double & Multiple Stars · Constellation Crux

Acrux (Alpha Crucis / α¹ & α² Crucis)

Coordinates, Hipparcos distance (321 ly), magnitude 0.76, 4.0″ B-star visual binary + α Cru C triple, and observing guide for Acrux.

Right Ascension (J2000.0)12h 26m 35.92s
Declination (J2000.0)-63° 05′ 56.7″
Primary ClassificationMassive B-type multiple star system (brightest star in Crux)
Best Observing SeasonSouthern Autumn to Winter (March–July; circumpolar south of −27°S)

Provenance-Backed Scientific Measurements

Every measurement below preserves its unit, uncertainty interval, observational method, reference epoch, quality status, and primary catalog source. See Uncertainty & Provenance for how competing measurements are handled.

Astrometric, Photometric, and Physical Parameters for Acrux (Alpha Crucis / α¹ & α² Crucis)
ParameterValueUncertaintyMethod & EpochQuality StatusSource Archive
Combined apparent visual magnitude (V)0.76 mag± 0.01 magJohnson UBV photometry (α¹ Cru = 1.33 mag, α² Cru = 1.73 mag)definitiveHipparcos New Reduction Catalog
Trigonometric parallax10.13 mas± 0.5 masHipparcos New Reduction astrometric solution (98.7 ± 4.9 pc) (J2000.0)definitiveHipparcos New Reduction Catalog
Distance in light-years321.9 ly± 15.8 lyDerived from Hipparcos parallax 10.13 ± 0.50 mashigh-confidenceHipparcos New Reduction Catalog
Visual α¹–α² angular separation0.067 arcmin± 0.002 arcminWashington Double Star Catalog astrometry (4.0 arcseconds at PA 112°)definitiveSIMBAD Astronomical Database (CDS)
Combined bolometric luminosity45000 L☉± 5000 L☉UV/optical B0.5 IV + B1 V spectrophotometry (~25,000 + 20,000 L☉)high-confidenceSIMBAD Astronomical Database (CDS)
Measurement Uncertainties & Competing Solutions: While α¹ and α² Crucis clearly form a physically bound pair separated by ≥430 AU (orbital period ≥1,500 years), whether the 4.86-magnitude B4 V star HD 108250 (α Cru C, 90″ away) is gravitationally bound or merely a co-moving Sco-Cen member remains debated.

J2000 Equatorial Sky Chart & Culmination Altitude

The chart below plots Acrux (Alpha Crucis Southern Cross Multiple) at RA 12h 26m 35.92s, Dec -63° 05′ 56.7″ within Crux, alongside peak meridian transit altitudes for 40°N and 30°S observers. Use the RA/Dec Coordinate Converter to compute exact culmination altitude for your latitude.

J2000 Equatorial Sky Position (Crux) +90° 0° −90° 24h 12h RA 0h Peak Meridian Altitude 0° 40°N Lat 57° 30°S Lat RA: 12h 26m 35.92s Dec: -63° 05′ 56.7″ Epoch: J2000.0 · V = 0.76 mag First-party vector diagram derived from IAU / CDS SIMBAD / Gaia DR3 astrometry.

Astrophysical Context & Structure

Acrux (Alpha Crucis) anchors the southern foot of the Southern Cross (Crux) and is the thirteenth-brightest star in Earth's night sky at combined apparent magnitude 0.76—making it the southernmost first-magnitude star in the heavens (declination −63° 06′). Featured on the national flags of Australia, New Zealand, Brazil, Papua New Guinea, and Samoa, Acrux was first resolved into a telescopic double star by Jesuit missionary astronomers Fontenay and Richaud in 1685–1689.

Located 98.7 ± 4.9 parsecs (322 light-years) away in the Lower Centaurus–Crux subgroup of the Scorpius–Centaurus OB association, Acrux resolves in any small telescope into two scorching blue-white diamonds separated by 4.0 arcseconds along position angle 112°: α¹ Crucis (magnitude 1.33, spectral class B0.5 IV, ~28,000 K) and α² Crucis (magnitude 1.73, spectral class B1 V, ~26,000 K, 13 solar masses). Separated by at least 430 AU in space, the pair takes upwards of 1,500 years to complete one orbit.

Furthermore, α¹ Crucis is itself a double-lined spectroscopic binary composed of two massive stars (~14 and ~10 solar masses) whipping around each other every 75.77 days at a separation of barely 1 AU. Ninety arcseconds south-southwest sits a third visual component, magnitude 4.86 HD 108250 (sometimes called α Crucis C), which is itself a 1.22-day spectroscopic binary—bringing the total count in the eyepiece field to five hot stars!

Practical Visual Observing Guide

Minimum InstrumentNaked eye; 60 mm telescope at 100×+ splits the 4.0″ α¹–α² pair
Recommended Magnification100×–180×
Best Evening SeasonSouthern Autumn to Winter (March–July; circumpolar south of −27°S)
  • In any 60–80 mm telescope at 100×–150×, Acrux is one of the most dazzling double stars in the entire sky: two almost equally brilliant icy-white headlights (magnitudes 1.3 and 1.7) separated by 4.0 arcseconds, joined 90 arcseconds away in the same field by 4.9-magnitude HD 108250.
  • Extend the long axis of the Southern Cross from Gacrux (γ Cru) through Acrux 4.5 times southward to locate the unmarked South Celestial Pole.

Catalog Cross-Identifications & Aliases

Common Aliases: α Crucis · α¹ & α² Crucis · HD 108248 / HD 108249 · HIP 60718

Cross-Catalog Identifiers for Acrux (Alpha Crucis / α¹ & α² Crucis)
Catalog AuthorityIdentifier
HIPHIP 60718
HDHD 108248
SIMBAD* alf Cru
WIKIDATAQ13020
Related Object · Centaurus

Proxima Centauri (Nearest Star to Sun)

Coordinates, Gaia DR3 parallax (768.07 mas, 4.2465 ly), magnitude 11.13, flare activity, and planetary system guide for Proxima Centauri.

Reference Guide

Angular Size, Separation & Field of View

How angular diameter (degrees, arcminutes, arcseconds), spherical angular separation, and small-angle physical diameter relate to telescope field of view.

Reference Guide

Stellar Spectral Classification (OBAFGKM)

Reference guide to Morgan-Keenan (MK) stellar classification (O B A F G K M), luminosity classes (I–V, WD), color index (B-V), and the H-R diagram.

Scientific Sources & Dataset Provenance