Acrux

Acrux

The position of Acrux
Observation data
Epoch J2000      Equinox J2000
Constellation Crux
Pronunciation /ˈkrʌks/
Right ascension 12h 26m 35.89522s
Declination −63° 05′ 56.7343″
Apparent magnitude (V) 0.76 (1.33 + 1.75)
Characteristics
Spectral type B0.5IV + B1V
B−V color index −0.26
Variable type β Cep
Astrometry
Radial velocity (Rv)+19.2±0.8 km/s
Proper motion (μ) RA: −35.83 mas/yr
Dec.: −14.86 mas/yr
Parallax (π)10.13±0.50 mas
Distance320 ± 20 ly
(99 ± 5 pc)
Absolute magnitude (MV)−3.77 (−2.2 + −2.7)
Orbit
Primaryα Crucis Aa
Nameα Crucis Ab
Period (P)75.7469±0.0017 d
Semi-major axis (a)(9.48±0.30)×10−3"
(1.01±0.04 au)
Eccentricity (e)0.369±0.015
Inclination (i)66.2±1.4°
Longitude of the node (Ω)225.0±2.0°
Periastron epoch (T)2,458,183.1±0.4 JD
Argument of periastron (ω)
(secondary)
229.5±2.2°
Semi-amplitude (K1)
(primary)
40.6±0.9 km/s
Orbit
Primaryα Crucis Ba
Nameα Crucis Bb
Period (P)405.4+0.4
−0.3
 d
Semi-major axis (a)(28.2±0.8)×10−3"
(3.0 au)
Eccentricity (e)0.36+0.45
−0.07
Inclination (i)94.4+2.6
−0.3
°
Longitude of the node (Ω)86.0+3.4
−6.1
°
Periastron epoch (T)2,458,099+258
−145
 JD
Argument of periastron (ω)
(secondary)
105.2+32.1
−55.3
°
Details
α Crucis Aa
Mass17.2±1.2 M
Radius6.8 R
Luminosity31,110+3,190
−2,910
 L
Temperature28,950 K
Rotational velocity (v sin i)84 km/s
Age7.1 Myr
α Crucis Ab
Mass6.8±0.3 M
Radius3.2 R
Luminosity1,400 L
Temperature19,750 K
Age7.1 Myr
α Crucis Ba
Mass12.4 M
Radius5.4 R
Luminosity14,000 L
Surface gravity (log g)4.00 cgs
Temperature26,950 K
Rotational velocity (v sin i)200 km/s
Age7.1 Myr
α Crucis Bb
Mass9.8 M
Radius4.4 R
Luminosity6,100 L
Temperature24,350 K
Other designations
α Crucis, CPD−62°2745, HIP 60718, CCDM J12266-6306, WDS J12266-6306
α Cru A: Acrux, α1 Crucis, 26 G. Crucis, FK5 462, GC 16952, HD 108248, HR 4730
α Cru B: α2 Crucis, 27 G. Crucis, GC 16953, HD 108249, HR 4731, 2MASS J12263615-6305571
Database references
SIMBADα Cru
α1 Cru
α2 Cru

Acrux is the brightest star system in the southern constellation of Crux. It has the Bayer designation α Crucis, which is Latinised to Alpha Crucis and abbreviated Alpha Cru or α Cru. With a combined visual magnitude of +0.76, it is the 13th-brightest star in the night sky. It is the most southerly star of the asterism known as the Southern Cross and is the southernmost first-magnitude star, 2.3 degrees more southerly than Alpha Centauri. This system is located at a distance of 321 light-years from the Sun.

To the naked eye Acrux appears as a single star, but it is actually a multiple star system containing seven components. Through optical telescopes, Acrux appears as a triple star, whose two brightest components are visually separated by about 4 arcseconds and are known as α Cru A and α Cru B, α1 Crucis and α2 Crucis, or α Crucis A and α Crucis B. Both components are B-type stars, and are many times more massive and luminous than the Sun. This system was the second ever to be recognized as a binary, in 1685 by a Jesuit priest. α1 and α2 Crucis are close binaries themselves, with components designated α Crucis Aa (officially named Acrux, historically the name of the entire system) α Crucis Ab, α Crucis Ba, and α Crucis Bb.

HR 4729, also known as α Cru C, is a more distant companion, forming a triple star through small telescopes. C has a faint companion and is also a spectroscopic binary, which brings the total number of stars in the system to seven.