U Leporis is a blue pulsating very luminous supergiant star that can be located in the constellation of Lepus. HIP22952 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD31599. U Leporis has alternative name(s), U_Lep.
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 U Leporis, the location is 04h 56m 17.96 and -21d13`01.5 .
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 -059.59 ± 001.28 towards the north and 041.45 ± 001.93 east if we saw them in the horizon.
U Leporis has a spectral type of A9/F0Iab:. This means the star is a blue supergiant star.
U Leporis has an apparent magnitude of 10.91 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 3.41 If you used the 2007 Parallax value, you would get an absolute magnitude of 2.07. 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 3.16 which gave the calculated distance to U Leporis as 1032.16 light years away from Earth or 316.46 parsecs. It would take a spaceship travelling at the speed of light, 1032.16 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 1.71 which put U Leporis at a distance of 1907.39 light years or 584.80 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 pulsating RR Lyrae type with asymmetric light curves 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. U Leporis brightness ranges from a magnitude of 11.000 to a magnitude of 10.000 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 1.0 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 Stellar Age, Metallicity or Mass is from the E.U. Exoplanets. The information was obtained as of 12th Feb 2017.
|Traditional Name||U Leporis|
|Short Name||U Lep|
|Hipparcos Library I.D.||22952|
|Bonner Durchmusterung||BD-21 1019|
|Henry Draper Designation||31599|
|Star Type||supergiant star|
|Absolute Magnitude||3.41 / 2.07|
|Right Ascension (R.A.)||04h 56m 17.96|
|1997 Distance from Earth||3.16 Parallax (milliarcseconds)|
|1032.16 Light Years|
|2007 Revised Distance from Earth||1.71 Parallax (milliarcseconds)|
|1907.39 Light Years|
|Proper Motion Dec.||-59.59 ± 1.28 milliarcseconds/year|
|Proper Motion RA.||41.45 ± 1.93 milliarcseconds/year|
|Variable Star Class||Pulsating|
|Variable Star Type||RR Lyrae type with asymmetric light curves|
|Mean Variability Period in Days||1.000|
|Variable Magnitude Range (Brighter - Dimmer)||10.000 - 11.000|