Lucida Anseris (Alpha Vulpeculae) is a red star that can be located in the constellation of Vulpecula. Alpha Vulpeculae is the Bayer Classification for the star. HIP95771 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD183439. Lucida Anseris has alternative name(s), 6 Vulpeculae , NSV_12069, 6 Vul.
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 Lucida Anseris, the location is 19h 28m 42.41 and +24d39`54.6 .
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 -107.44 ± 0.20 miliarcseconds/year towards the north and -126.13 ± 0.28 miliarcseconds/year east if we saw them in the horizon.
Lucida Anseris has a spectral type of M0 comp. This means the star is a red star. The star has a B-V Colour Index of 1.5 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 4,014 Kelvin.
Lucida Anseris has been calculated as 22.69 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 15,784,707.19.km.
Lucida Anseris has an apparent magnitude of 4.44 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 -0.35 If you used the 2007 Parallax value, you would get an absolute magnitude of -0.36. 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 11.00 which gave the calculated distance to Lucida Anseris as 296.51 light years away from Earth or 90.91 parsecs. It would take a spaceship travelling at the speed of light, 296.51 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 10.97 which put Lucida Anseris at a distance of 297.32 light years or 91.16 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. Lucida Anseris brightness ranges from a magnitude of 5.000 to a magnitude of 5.000 over its variable period. The smaller the magnitude, the brighter the star.
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.
|Traditional/Proper Name||Lucida Anseris|
|Short Name||NSV 12069, 6 Vul|
|Bayer Designation||Alpha Vulpeculae|
|Alternative Name(s)||6 Vulpeculae|
|Hipparcos Library I.D.||95771|
|Bonner Durchmusterung||BD+24 3759|
|Henry Draper Designation||183439|
|Absolute Magnitude||-0.35 / -0.36|
|Right Ascension (R.A.)||19h 28m 42.41|
|1997 Distance from Earth||11.00 Parallax (milliarcseconds)|
|296.51 Light Years|
|2007 Revised Distance from Earth||10.97 Parallax (milliarcseconds)|
|297.32 Light Years|
|Proper Motion Dec.||-107.44 ± 0.20 milliarcseconds/year|
|Proper Motion RA.||-126.13 ± 0.28 milliarcseconds/year|
|Spectral Type||M0 comp|
|Radius (x the Sun)||22.69|
|Calculated Effective Temperature||4,014 Kelvin|
The map was generated using Night Vision, an awesome free application by Brian Simpson.