Epoch J2000.0 Equinox J2000.0
|Right ascension||12h 31m 09.95961s|
|Declination||−57° 06′ 47.5684″|
|Apparent magnitude (V)||+1.64|
|Spectral type||M3.5 III|
|Apparent magnitude (J)||−1.99|
|U−B color index||+1.78|
|B−V color index||+1.59|
|Radial velocity (Rv)||+20.6 km/s|
|Proper motion (μ)|| RA: +28.23 mas/yr |
Dec.: −265.08 mas/yr
|Parallax (π)||36.83 ± 0.18 mas|
|Distance||88.6 ± 0.4 ly |
(27.2 ± 0.1 pc)
|Absolute magnitude (MV)||−0.52|
|Mass||1.5 ± 0.3 M☉|
Gamma Crucis (γ Crucis, abbreviated Gamma Cru, γ Cru), also named Gacrux, is the nearest M-Giant star to the Sun. The distance to Gacrux has been determined using parallax measurements made during the Hipparcos mission, which yielded a value of 88.6 light-years (27.2 parsecs) away from the Sun. With an apparent visual magnitude of +1.63, this is the third-brightest star in the southern circumpolar constellation of Crux, the Southern Cross, and one of the brightest stars in the night sky. A line from the two "Pointers", Alpha Centauri through Beta Centauri, leads to within a few degrees of this star.
Since Gamma Crucis is at roughly −60° declination, it lacks a traditional name. Nonetheless, it was known to the ancient Greeks and Romans, in whose era it was visible north of 40° latitude due to the precession of equinoxes. The astronomer Ptolemy counted it as part of the constellation of Centaurus. The historical name Gacrux is a contraction of the Bayer designation, coined by astronomer Elijah Hinsdale Burritt (1794-1838). In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016 included a table of the first two batches of names approved by the WGSN; which included Gacrux for this star.
In Chinese, 十字架 (Shí Zì Jià), meaning Cross, refers to an asterism consisting of Gamma Crucis, Alpha Crucis, Beta Crucis and Delta Crucis. Consequently, Gamma Crucis itself is known as 十字架一 (Shí Zì Jià yī, English: the First Star of Cross.).
The people of Aranda and Luritja tribe around Hermannsburg, Central Australia named Iritjinga, "The Eagle-hawk", a quadrangular arrangement comprising this star, Delta Crucis (Palida), Gamma Centauri (Muhilfain) and Delta Centauri (Ma Wei).
Among Portuguese-speaking peoples it is also named Rubídea (or Ruby-like), in reference to its color.
Gacrux has a stellar classification M3.5 III. It has evolved off of the main sequence to become a red giant star, but is most likely on the red giant branch rather than the asymptotic giant branch. Although only 30% more massive than the Sun, at this stage the star has expanded to 84 times the Sun's radius. It is radiating roughly 820 times the luminosity of the Sun from its expanded outer envelope. With an effective temperature of 3,626 K, the colour of Gamma Crucis is a prominent reddish-orange, well in keeping with its spectral classification. It is a semi-regular variable with multiple periods. (See table at left.)
The atmosphere of this star is enriched with barium, which is usually explained by the transfer of material from a more evolved companion. Typically this companion will subsequently become a white dwarf. However, no such companion has yet been detected. A +6.4 magnitude companion star lies about 2 arcminutes away at a position angle of 128° from the main star, and can be observed with binoculars. But it is only an optical companion, which is about 400 light years distant from Earth.
Gamma Crucis is represented in the flags of Australia, New Zealand and Papua New Guinea as one of five stars which comprise the Southern Cross. It is also featured in the flag of Brazil, along with 26 other stars, each of which represents a state. Gamma Crucis represents the State of Bahia.
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