V744 Centauri is a red pulsating giant star that can be located in the constellation of Centaurus. HIP66666 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD118767. The Id of the star in the Gould Star Catalogue is 246. 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. V744 Centauri has alternative name(s), V744_Cen.
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 V744 Centauri, the location is 13h 39m 59.90 and -49d57`00.0 .
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 018.74 ± 000.24 towards the north and -100.11 ± 000.33 east if we saw them in the horizon.
V744 Centauri has a spectral type of M8III. This means the star is a red giant star. The star has a B-V Colour Index of 1.49 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 4,007 Kelvin.
V744 Centauri has been calculated as 22.98 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 15,986,477.39.km.
V744 Centauri has an apparent magnitude of 5.74 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 -0.37 If you used the 2007 Parallax value, you would get an absolute magnitude of -0.25. 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 6.00 which gave the calculated distance to V744 Centauri as 543.61 light years away from Earth or 166.67 parsecs. It would take a spaceship travelling at the speed of light, 543.61 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 6.35 which put V744 Centauri at a distance of 513.64 light years or 157.48 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 star is a pulsating Semiregular late- (M, C, S or Me, Ce, Se) giants with poorly defined periodicity variable type which means that its size changes over time. The Variable Type is usually named after the first star of that type to be spotted. V744 Centauri brightness ranges from a magnitude of 6.000 to a magnitude of 5.000 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 1.0 days (variability).
|Traditional Name||V744 Centauri|
|Short Name||V744 Cen|
|Hipparcos Library I.D.||66666|
|Henry Draper Designation||118767|
|Star Type||giant star|
|Absolute Magnitude||-0.37 / -0.25|
|Right Ascension (R.A.)||13h 39m 59.90|
|1997 Distance from Earth||6.00 Parallax (milliarcseconds)|
|543.61 Light Years|
|2007 Revised Distance from Earth||6.35 Parallax (milliarcseconds)|
|513.64 Light Years|
|Proper Motion Dec.||18.74 ± 0.24 milliarcseconds/year|
|Proper Motion RA.||-100.11 ± 0.33 milliarcseconds/year|
|Variable Star Class||Pulsating|
|Variable Star Type||Semiregular late- (M, C, S or Me, Ce, Se) giants with poorly defined periodicity|
|Mean Variability Period in Days||1.000|
|Variable Magnitude Range (Brighter - Dimmer)||5.000 - 6.000|
|Radius (x the Sun)||22.98|
|Calculated Effective Temperature||4,007 Kelvin|