Sirius (Alpha Canis Majoris) is a blue star that can be located in the constellation of CanisMajor. It is the 2nd brightest star in the night sky. Alpha Canis Majoris is the Bayer Classification for the star. The Id of the star in the Yale Bright Star Catalogue is HR2491. HIP32349 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD48915. Sirius has alternative name(s), 9 Canis Majoris , 9 CMa.
Sirius is also known as the Dog star, after all it is in the Big Dog constellation of Canis Major. It is widely known in part as it is the brightest star in the night sky, it is almost twice as bright as the next brightest star, Canopus. It is also one of our nearest neighbour stars, not as close as Rigil Kentaurus (Alpha Centauri) but still close. The only thing that is brighter excluding the moon is the planet Venus. It is moving closer towards us but won`t for a long time, longer than you and I will be on this planet so nothing to worry. 1. Sirius is a Double Star System with the smaller star being a white dwarf star having used up all its hydrogen.
Being the brightest and one of the most well known, it has become of interest by science fiction writers, for example, the lizard Visitors from V come from a planet orbiting this star. JK Rowling, author of the Harry Potter books has a character Sirius Black who name is inspired from this star. There are also other stars that have been the inspiration for characters such as Regulus Black. Sirius isn`t just limited to being mentioned in these fictions, the star is mentioned elsewhere. Sirius gets mentioned in Star Trek but there`s no real stories based in the Sirius Solar System excluding the cartoon series and extended universe. ref:Memory Alpha.
Sirius is currently moving towards us but don`t fear a solar apocalypse, it will never collide with our Sun. It is moving at a very slow speed of 5.5 km/s and the closest it will ever get to us is 7.8 Light years, down from 8.6 that it is now. It will continue to be the brightest star in the night sky for at least another 90000 year after which point Delta Scuti will then take on that title. ref:StackExchange
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 Sirius, the location is 06h 45m 09.25 and -16d42`47.3 .
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 -1,223.07 ± 001.04 towards the north and -546.01 ± 001.58 east if we saw them in the horizon.
Sirius has a spectral type of A0m.... This means the star is a blue star. The star has a B-V Colour Index of -0.03 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 11,122 Kelvin.
Sirius has been calculated as 1.73 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,203,734.00.km.
The star has a companion star which is in orbit close by, it has at least the following companions in close orbit, Sirius B.
Sirius has an apparent magnitude of -1.44 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 1.45 If you used the 2007 Parallax value, you would get an absolute magnitude of 1.45. 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 379.21 which gave the calculated distance to Sirius as 8.60 light years away from Earth or 2.64 parsecs. It would take a spaceship travelling at the speed of light, 8.60 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 379.21 which put Sirius at a distance of 8.60 light years or 2.64 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 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.
|Short Name||9 CMa|
|Bayer Designation||Alpha Canis Majoris|
|Alternative Name(s)||9 Canis Majoris|
|Hipparcos Library I.D.||32349|
|Yale Bright Star Catalogue (HR) Id||2491|
|Bonner Durchmusterung||BD-16 1591|
|Henry Draper Designation||48915|
|Absolute Magnitude||1.45 / 1.45|
|Right Ascension (R.A.)||06h 45m 09.25|
|1997 Distance from Earth||379.21 Parallax (milliarcseconds)|
|8.60 Light Years|
|2007 Revised Distance from Earth||379.21 Parallax (milliarcseconds)|
|8.60 Light Years|
|Proper Motion Dec.||-1223.07 ± 1.04 milliarcseconds/year|
|Proper Motion RA.||-546.01 ± 1.58 milliarcseconds/year|
|Orbital Period (Days)||18295.40|
|Argument Of Periastron||327.27|
|Brightest in Night Sky||2nd|
|Companion Stars||Sirius B|
|Radius (x the Sun)||1.73|
|Calculated Effective Temperature||11,122 Kelvin|
The star has been identified as being a multi-star system, one in which there is at least one star in close orbit to another star or two or more stars orbiting a central point. The stars may be of equal mass, unequal mass where one star is stronger than the other or be in groups orbiting a central point which doesn't necessarily have to be a star. More information can be found on my dedicated multiple star systems page. The source of the info is Simbad. The file is dated 2000 so any differences between this and any other source will be down to the actual source from where the information came from.
|Proper Motion mas/yr|
|H.D. Id||B.D. Id||Star Code||Magnitude||R.A.||Dec.||Spectrum||Colour||Year|