V424 Aurigae is a eclipsing binary system variable star that can be located in the constellation of Auriga. The description is based on the spectral class.
HIP25252 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD35132.
V424 Aurigae has alternative name(s) :- , V424 Aur.
BD number is the number that the star was filed under in the Durchmusterung or Bonner Durchmusterung, a star catalogue that was put together by the Bonn Observatory between 1859 to 1903. The star's BD Number is BD+32 966.
More details on star alternative names can be found at Star Names .
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 -3.78 ± 0.74 miliarcseconds/year towards the north and 0.25 ± 1.05 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 3.20000 km/s with an error of about 4.90 km/s .
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.
|Primary / Proper / Traditional Name||V424 Aurigae|
|Alternative Names||HD 35132, HIP 25252, BD+32 966, V424 Aur|
|Multiple Star System||Yes|
|Star Type||Variable Star|
|Galactic Latitude||-1.90 degrees|
|Galactic Longitude||174.39 degrees|
|Distance from Earth||1.65 Parallax (milliarcseconds)|
|1976.75 Light Years|
|Proper Motion Dec.||-3.78 ± 0.74 milliarcseconds/year|
|Proper Motion RA.||0.25 ± 1.05 milliarcseconds/year|
|Radial Velocity||3.20 ± 4.90 km/s|
|Variable Star Class||Eclipsing binary system|
|Variable Star Type||Beta Lyrae (Sheliak)|
|Mean Variability Period in Days||1.837|
|Variable Magnitude Range (Brighter - Dimmer)||8.350 - 8.470|
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|