Campbell's Star is a eclipsing binary system Wolf-Rayet star that can be located in the constellation of Cygnus. The star can not be seen by the naked eye, you need a telescope to see it.
HIP96295 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD184738.
Campbell's Star has alternative name(s), V1966 Cyg.
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 Campbell's Star, the location is 19h 34m 45.24 and +30d 30` 59.0 .
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 -9.21 ± 1.62 miliarcseconds/year towards the north and -4.08 ± 2.32 miliarcseconds/year east if we saw them in the horizon. The Radial Velocity, that is the speed at which the star is moving away/towards us is -30.40000 km/s with an error of about 3.30 km/s .
Campbell's Star has a spectral type of WC.... This means the star is a Wolf-Rayet star. The star has a B-V Colour Index of -0.01 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 10,551 Kelvin. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.
Campbell's Star has an apparent magnitude of 10.00 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 If you used the 2007 Parallax value, you would get an absolute magnitude of -3.49. 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 -1.63 which gave the calculated distance to Campbell's Star as -2001.00 light years away from Earth or -613.50 parsecs. It would take a spaceship travelling at the speed of light, -2001.00 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 0.20 which put Campbell's Star at a distance of 16308.17 light years or 5000 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 eclipsing binary system Eclipsing 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. Campbell's Star brightness ranges from a magnitude of 9.534 to a magnitude of 9.423 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 0.1 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||Campbell's Star|
|Short Name||V1966 Cyg|
|Hipparcos Library I.D.||96295|
|Bonner Durchmusterung||BD+30 3639|
|Henry Draper Designation||184738|
|Star Type||Wolf-Rayet star|
|Visual / Apparent Magnitude||10.00|
|Naked Eye Visible||Requires a 7x50 Binoculars - Magnitudes|
|Right Ascension (R.A.)||19h 34m 45.24|
|Declination (Dec.)||+30d 30` 59.0|
|Galactic Latitude||5.02 degrees|
|Galactic Longitude||64.79 degrees|
|1997 Distance from Earth||-1.63 Parallax (milliarcseconds)|
|-2001.00 Light Years|
|2007 Revised Distance from Earth||0.20 Parallax (milliarcseconds)|
|16308.17 Light Years|
|Proper Motion Dec.||-9.21 ± 1.62 milliarcseconds/year|
|Proper Motion RA.||-4.08 ± 2.32 milliarcseconds/year|
|Radial Velocity||-30.40 ± 3.30 km/s|
|Variable Star Class||Eclipsing binary system|
|Variable Star Type||Eclipsing|
|Mean Variability Period in Days||0.059|
|Variable Magnitude Range (Brighter - Dimmer)||9.423 - 9.534|
|Calculated Effective Temperature||10,551 Kelvin|
The map was generated using Night Vision, an awesome free application by Brian Simpson.