Acrux / Alpha Crucis Star Facts (Type, Distance, Magnitude, Age, Mass, Colour, Location and more)
Facts
Acrux is the southern most star of the constellationCrux, the Southern Cross. Although the picture below probably gives the impression it is the Northern most of the stars, the picture is the wrong way up. Acrux is one of the brightest stars in the night sky, coming in at position thirteen and being one of the most in the Southern hemisphere.
Acrux, also known as Alpha Crucis (Bayer) is a spectroscopic binary star located in the constellation of Crux, The Southern Cross. Acrux is a major star and forms part of the constellation.
Based on the spectral type (B0.5IV), Acrux colour is blue, which means that the star is one of the hottest stars in the Universe, hotter than our star.


Acrux temperature is in the range of 10,000 to 30,000 Kelvin. Based on the spectral type (B0.5IV) as we don't have the exact temperature', we can deduce that the surface temperature of Acrux is in the order of 10,000 and 25,000K based on the notes from Harvard University. To put this in context, the temperature of our Sun is about 5,778 Kelvin as said by Google.
Acrux is the brightest star in Crux and the 13th in the night sky based on the Hipparcos 2007 apparent magnitude. Based on a parallax of 10.13, Acrux distance from Earth can be calculated at being 321.98 light years away or 98.33 parsecs.
Acrux is a naked-eye star, so you don't need a telescope or binoculars when you look up on a clear night. The lower the magnitude, the easier it will be to see it.
Star System
Acrux is a binary or multiple star system. The list below may not include all the stars, only those that are recorded on this site.
- Acrux is the main star in the system and the one that is designated as 'A'. It can also refer to the whole system. Acrux is a blue subgiant star whose temperature is between 10,000 and 25,000 Kelvin.
- Acrux B is a blue main sequence star whose temperature is between 10,000 and 25,000 Kelvin.
Location
The location of the Acrux in the night sky is determined by the right ascension (R.A.) and declination (Dec.). These are equivalent to the Longitude and Latitude on Earth. The Right Ascension (Longitude) is expressed in time (hh:mm:ss) and is how far the star is along Earth's celestial equator. If the R.A. is positive, then it's eastwards and vice versa.
The Declination (Latitude) is how far north or south the object is compared to the celestial equator and is expressed in degrees. If the value is positive, it is north of the celestial equator. For Acrux, the location is 12h 26m 35.94 and -63° 05` 56.6 .
Based on the location of Crux, Acrux can be located in the southern hemisphere of the celestial sky. The celestial hemisphere is equivalent to the hemispheres on Earth. Acrux is south of the Ecliptic. The Ecliptic is the path that the Earth takes as it orbits the Sun. As the Earth is titled, we therefore have Celestial and Ecliptic hemispheres and they can be different for a star.
Physical Properties
Spectral Type
Acrux spectral type of B0.5IV which means its colour and type is blue spectroscopic binary star. There is no relationship between colour and size. For example, a red star can be large or small. Small stars are more energy efficient than larger stars and live longer.
Acrux Luminosity
Luminosity is the amount of energy a star pumps out relative to the amount that our star, the Sun, gives out. Our star, the Sun's value is 1. Acrux luminosity figure of 30,302.96 is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012. The star generates more energy than our star.
Acrux Size (Radius)
Acrux radius has been calculated as being 7.8 times bigger than the Sun. The Sun's radius is 695,800km, therefore, the Acrux radius is an estimated 5,427,240.km. If you need the star's diameter, you just need to multiply the radius by 2.
Acrux Mass
The Acrux mass is 17.8 times that of our star, the Sun. The Sun's Mass is 1,989,100,000,000,000,000,000 billion kg. which to calculate using this website is too large. To give idea of size, the Sun is 99.86% the mass of the solar system.
Acrux Death
We can't be sure when Acrux will die, we can have estimations based on its spectral type and mass. Based on current estimations with Acrux being more than 10 solar masses, it will at the end of its life, most likely die in a Supernova explosion. The explosion will leave behind either a Pulsar or a Black Hole.
Acrux Age
Acrux is believed to be about 11 million years old. To put in context, the Sun is believed to be about five billion years old and the Universe is about 13.8 billion years old. The smaller star is, the more efficient it is with its fuel and so will live longer than a star which is very large. Acrux lifespan can be measured in millions of years based on a typical blue star (B Type). B stars are short lived stars as they are not fuel-efficient.
Magnitude (Apparent / Absolute / Visible)
A number represents a star’s magnitude, whether apparent/visual or absolute. The smaller the number, the brighter the star is. The Sun is the brightest star and therefore has the lowest of all magnitudes, -26.74. A faint star will have a high number.
Acrux apparent magnitude is 0.77, which is a measure of the star's brightness as seen from Earth. Apparent Magnitude is also known as Visual Magnitude.
If you use the 1997 parallax value, Acrux' absolute magnitude is -4.19. If you use the 2007 parallax value, Acrux' absolute magnitude is -4.20. Absolute Magnitude is the star's apparent magnitude from 10 parsecs or 32.6 light years. The magnitude assumes nothing is between the object and the viewer, such as dust clouds. To compare different stars' actual brightness, you would best use Absolute rather than Apparent Magnitude.
Acrux is visible from Earth without needing binoculars or a telescope. The lower the Apparent Magnitude of a star or other object is, the easier it is to see in the night sky. An object with a magnitude greater than 6.5 cannot be seen without a telescope or other device.
Radial Velocity and Proper Motion
In simplistic terms, all non-rogue stars, like planets, orbit around a central object, although that is actually not true. Where is the centre of the Solar System. For simplicity it's the central star, such as the Sun. In the case of a star, it's the galactic centre. The constellations we see today will be different than they were 50,000 years ago or 50,000 years from now.
Proper motion details the movements of these stars and is measured in milliarcseconds. Acrux is moving -14.86 ± 0.36 milliarcseconds/year towards the north and -35.83 ± 0.5 milliarcseconds/year east if we saw them in the horizon.
The radial velocity, the speed at which the Acrux is moving away from the Sun, is 11.90000 km/s with an error of about 2.40 km/s . When the value is negative, the star and the Sun are getting closer to one another; likewise, a positive number means that two stars are moving away. It's nothing to fear as the stars are so far apart they won't collide in our lifetime, if ever.
Source of Information
The source of the information if it has a Hip I.D. is from Simbad, the Hipparcos data library based at the University at Strasbourg, France. Hipparcos was an E.S.A. satellite operation launched in 1989 for four years. The items in red are values that I've calculated, so they could be wrong. Information regarding Metallicity and/or Mass is from the E.U. Exoplanets. The data was obtained as of 12th Feb 2017.
Acrux Fact Table
The table is scrollable if you can't see everything, just swipe the table to see the hidden information.
| Primary Name | Acrux |
|---|---|
| Spectral Type | B0.5IV |
| Binary or Multiple Star | Yes |
| Star Type | Spectroscopic Binary |
| Colour | blue |
| Galaxy | Milky Way |
| Constellation | Crux |
| Main Star | Yes |
| Age | 11 million years |
| Absolute Magnitude | -4.19 / -4.20 |
| Visual / Apparent Magnitude | 0.77 |
| Visible From Earth | Yes |
| Right Ascension (R.A.) | 12h 26m 35.94 |
| Declination (Dec.) | -63° 05` 56.6 |
| Galactic Latitude | -0.36267814 ° |
| Galactic Longitude | 300.12665439 ° |
| 1997 Distance from Earth | 10.17000 Parallax (milliarcseconds) |
| 320.71 Light Years | |
| 98.33 Parsecs | |
| 2007 Distance from Earth | 10.13000 Parallax (milliarcseconds) |
| 321.98 Light Years | |
| 98.72 Parsecs | |
| 20,362,319.786 Astronomical Units | |
| Galacto-Centric Distance | 23,976.267 Light Years / 7,351 Parsecs |
| Proper Motion Dec. | -14.86000 ± 0.36000 milliarcseconds/year |
| Proper Motion RA. | -35.83000 ± 0.50000 milliarcseconds/year |
| B-V Index | -0.24 |
| Radial Velocity | 11.90000 ± 2.4 km/s |
| Eccentricity | 0.05700 |
| Semi-Major Axis | 7057.0000000 |
| Luminosity (Lsun) | 30302.9600000 |
| Mass (Solars) | 17.8000 |
| Radius | 7.8 |
| Brightest in Night Sky | 13th |
Sources and Links
| Modified Date | 13th July 2024 |
| Published Date | Jan 2015 |
| SIMBAD Source | Link |
Crux's Main Stars in Brightness Order
- Acrux (Alpha Crucis)
- Mimosa (Beta Crucis)
- Gacrux (Gamma Crucis)
- Imai (Delta Crucis)
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