Rigil Kentaurus (Alpha Centauri) is a white to yellow main sequence dwarf star that can be located in the constellation of Centaurus. It is the 4th brightest star in the night sky. It is calculated at being 4.400 Billion Years old. This information comes from ExoPlanet. Alpha Centauri is the Bayer Classification for the star. The Id of the star in the Yale Bright Star Catalogue is HR5459. HIP71683 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD128620. The Id of the star in the Gould Star Catalogue is 363. Stars in the southern hemisphere are more likely to have a Gould Id than the northern hemisphere. For example, there are no Gould classified stars in Ursa Major. Rigil Kentaurus has alternative name(s), Alpha CenTau , . Rigil Kentaurus is a multiple star system with 2 stars orbiting in its solar system.
Rigil Kentaurus is more famously known as simply Alpha Centauri which is one of the closest stars to our own solar system. The star is a Mutiple Star System where one star orbits the other and both being roughly the same size.
Being the closest star, it features in many science fiction stories and films such as in Avatar where the moon of Pandora is orbiting one of the star`s planets. There has been speculation that there is in fact a few Extrasolar Planets (Exoplanets) in orbit round the planet which if true would make it the closest exoplanet to ours. Before getting too excited, you need to realise it is still far far away to get to. If you could fit the entire Solar System into your room, you would probably be talking situating Rigil some four miles (roughly) away. We just don`t have the technology to get there. Alpha Centauri is roughly about the same size as the The Sun and so will die roughly or before the Sun.
The location of the star in the galaxy is determined by the Right Ascension (R.A.) and Declination (Dec.), these are equivalent to the Longitude and Latitude on the Earth. The Right Ascension is how far expressed in time (hh:mm:ss) the star is along the celestial equator. If the R.A. is positive then its eastwards. The Declination is how far north or south the star is compared to the celestial equator and is expressed in degrees. For Rigil Kentaurus, the location is 14h 39m 40.90 and -60d50`06.5 .
All stars like planets orbit round a central spot, in the case of planets, its the central star such as the Sun. In the case of a star, its the galactic centre. The constellations that 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 are measured in milliarcseconds. The star is moving 473.67 ± 002.46 towards the north and -3,679.25 ± 004.11 east if we saw them in the horizon.
Luminosity is the amount of energy that a star pumps out and its relative to the amount that our star, the Sun gives out. The figure of 1.0000000 that I have given is based on the Spectral Types page that I have found on the Internet. You might find a different figure, one that may have been calculated rather than generalised that I have done. The figure is always the amount times the luminosity of the Sun. It is an imprecise figure because of a number of factors including but not limited to whether the star is a variable star and distance.
Rigil Kentaurus has a spectral type of G2V. This means the star is a white to yellow main sequence dwarf star. The star has a B-V Colour Index of 0.71 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 5,533 Kelvin.
Rigil Kentaurus has been calculated as 1.38 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 958,128.77.km.
The star is believed to be about 4.40 Billion 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 star has companion stars which are in orbit close by, it has at least the following companions in close orbit, Proxima Centauri, Alpha Centauri B.
Rigil Kentaurus has an apparent magnitude of -0.01 which is how bright we see the star from Earth. Apparent Magnitude is also known as Visual Magnitude. If you used the 1997 Parallax value, you would get an absolute magnitude of 4.34 If you used the 2007 Parallax value, you would get an absolute magnitude of 4.39. Magnitude, whether it be apparent/visual or absolute magnitude is measured by a number, the smaller the number, the brighter the Star is. Our own Sun is the brightest star and therefore has the lowest of all magnitudes, -26.74. A faint star will have a high number.
Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 742.12 which gave the calculated distance to Rigil Kentaurus as 4.40 light years away from Earth or 1.35 parsecs. It would take a spaceship travelling at the speed of light, 4.40 years to get there. We don't have the technology or spaceship that can carry people over that distance yet.
In 2007, Hipparcos data was revised with a new parallax of 754.81 which put Rigil Kentaurus at a distance of 4.32 light years or 1.32 parsecs. It should not be taken as though the star is moving closer or further away from us. It is purely that the distance was recalculated.
The Alpha Centaurids Meteor Shower radiants from a point near this star. The meteor shower runs typically between Jan 28 - Feb 21 with a peak date of Feb 07. The speed of a meteor in the shower is 58 Km/s. The amount of meteors predicted to be seen per hour (Zenith Hourly Rate) is 58. p>
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 a E.S.A. satellite operation launched in 1989 for four years. The items in red are values that I've calculated so they could well be wrong. Information regarding Stellar Age, Metallicity or Mass is from the E.U. Exoplanets. The information was obtained as of 12th Feb 2017.
|Traditional Name||Rigil Kentaurus|
|Bayer Designation||Alpha Centauri|
|Alternative Name(s)||Alpha CenTau|
|Hipparcos Library I.D.||71683|
|Yale Bright Star Catalogue (HR) Id||5459|
|Henry Draper Designation||128620|
|Star Type||main sequence dwarf star|
|Age||4.400 Billions of Years|
|Absolute Magnitude||4.34 / 4.39|
|Right Ascension (R.A.)||14h 39m 40.90|
|1997 Distance from Earth||742.12 Parallax (milliarcseconds)|
|4.40 Light Years|
|2007 Revised Distance from Earth||754.81 Parallax (milliarcseconds)|
|4.32 Light Years|
|Proper Motion Dec.||473.67 ± 2.46 milliarcseconds/year|
|Proper Motion RA.||-3679.25 ± 4.11 milliarcseconds/year|
|Brightest in Night Sky||4th|
|Colour||(G) White to Yellow|
|Stars in Solar System||2|
|Companion Stars||Proxima Centauri|
Alpha Centauri B
|Radius (x the Sun)||1.38|
|Luminosity (x the Sun)||1.0000000|
|Calculated Effective Temperature||5,533 Kelvin|