VY Canis Majoris is a red pulsating star that can be located in the constellation of CanisMajor. The star can not be seen by the naked eye, you need a telescope to see it.
HIP35793 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD58061.
VY Canis Majoris has alternative name(s), VY CMa.
VY Canis Majoris is one of the biggest stars in The Milky Way, it is so large that if it was placed at the centre of our Solar System, its radius would reach out past the orbit of Jupiter and we`d be inside its ball of fire. It won`t live much longer as stars that are big live quick, die young. It was once thought to be the biggest star in the observable Universe but that accolade belongs to UY Scuti. Given our limits to what we can see, VY Canis Majoris might be a titchy star compared to a bigger giant out there somewhere
The star is believed to be enveloped in a Nebula which was caused probably by ejections from itself. When it does go out, it will probably turn into a Wolf-Rayet star or go supernova. If it does go bang, Earth will not be affected by the gamma-ray bursts as we`re so far away to be affected by them.
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 VY Canis Majoris, the location is 07h 22m 58.33 and -25d 46` 03.2 .
VY Canis Majoris has a spectral type of M3/M4II:. This means the star is a red star. The star has a B-V Colour Index of 2.05 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 1,500 Kelvin.
VY Canis Majoris has been calculated as 1,573.00 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,094,493,400.00.km.
VY Canis Majoris has an apparent magnitude of 8.08 which is how bright we see the star from Earth. Apparent Magnitude is also known as Visual Magnitude. Using the supplied Parallax value, you would get an absolute magnitude of -0.67 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 1.78 which gave the calculated distance to VY Canis Majoris as 1832.38 light years away from Earth or 561.80 parsecs. It would take a spaceship travelling at the speed of light, 1832.38 years to get there. We don't have the technology or spaceship that can carry people over that distance yet.
The star is a pulsating Slow Irregular 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. VY Canis Majoris brightness ranges from a magnitude of 8.762 to a magnitude of 7.444 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 1.1 days (variability).
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 Metallicity and/or Mass is from the E.U. Exoplanets. The information was obtained as of 12th Feb 2017.
|Traditional/Proper Name||VY Canis Majoris|
|Short Name||VY CMa|
|Hipparcos Library I.D.||35793|
|Henry Draper Designation||58061|
|Visual / Apparent Magnitude||8.08|
|Naked Eye Visible||Requires a 7x50 Binoculars - Magnitudes|
|Right Ascension (R.A.)||07h 22m 58.33|
|Declination (Dec.)||-25d 46` 03.2|
|Galactic Latitude||-5.07 degrees|
|Galactic Longitude||239.35 degrees|
|Distance from Earth||1.78 Parallax (milliarcseconds)|
|1832.38 Light Years|
|Radial Velocity||72.70 ± 3.30 km/s|
|Variable Star Class||Pulsating|
|Variable Star Type||Slow Irregular|
|Mean Variability Period in Days||1.099|
|Variable Magnitude Range (Brighter - Dimmer)||7.444 - 8.762|
|Radius (x the Sun)||1,573.00|
|Calculated Effective Temperature||1,500 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|