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51 Leonis Minoris, HD96094, HIP54196

51 Leonis Minoris is a white to yellow star that can be located in the constellation of LeoMinor. The star can not be seen by the naked eye, you need a telescope to see it. The star has an estimated age of 8.60 Billion of Years but could be as young as 7.80 to 9.40 according to Hipparcos.

HIP54196 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD96094.

Location of 51 Leonis Minoris

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 51 Leonis Minoris, the location is 11h 05m 15.73 and +25d 12` 07.4 .

Proper Motion of 51 Leonis Minoris

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 -61.78 ± 0.39 miliarcseconds/year towards the north and -399.99 ± 0.60 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 0.62000 km/s with an error of about 0.14 km/s .

Physical Properties (Colour, Temperature, Age, Radius) of 51 Leonis Minoris

51 Leonis Minoris has a spectral type of G0. This means the star is a white to yellow star. The star is 7419.00000000 Parsecs from the Galactic Centre or terms of Light Years is 24198.0584913600000000s. The star has a B-V Colour Index of 0.59 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 5,898 Kelvin.

51 Leonis Minoris Radius has been calculated as being 1.62 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,127,046.59.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 1.50. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures. The star's Iron Abundance is -0.37 with an error value of 0.02 Fe/H with the Sun has a value of 1 to put it into context.

The stars age according to Hipparcos data files put the star at an age of about 8.60 Billion years old but could be between 7.80 and 9.40 Billion years old. In comparison, the Sun's age is about 4.6 Billion Years Old.

51 Leonis Minoris Apparent and Absolute Magnitudes

51 Leonis Minoris has an apparent magnitude of 7.60 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 3.71 If you used the 2007 Parallax value, you would get an absolute magnitude of 3.88. 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.

Distance to 51 Leonis Minoris

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 16.68 which gave the calculated distance to 51 Leonis Minoris as 195.54 light years away from Earth or 59.95 parsecs. It would take a spaceship travelling at the speed of light, 195.54 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 18.03 which put 51 Leonis Minoris at a distance of 180.90 light years or 55.46 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's Galacto-Centric Distance is 7,419.00 Parsecs or 24,198.06 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*.

Source of Information

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.

51 Leonis Minoris Facts

Alternative Names

Traditional/Proper Name51 Leonis Minoris
Flamsteed Name51 Leonis Minoris
Flamsteed Short Name51 LMi
Hipparcos Library I.D.54196
Bonner DurchmusterungBD+25 2335
Henry Draper Designation96094

Visual Facts

Star Type star
ConstellationLeo Minor
Age8.60 Billion Years Old
Age Range7.80 - 9.40 Billion Years Old
Absolute Magnitude3.71 / 3.88
Visual / Apparent Magnitude7.60
Naked Eye VisibleRequires a 7x50 Binoculars - Magnitudes
Right Ascension (R.A.)11h 05m 15.73
Declination (Dec.)+25d 12` 07.4
Galactic Latitude66.14 degrees
Galactic Longitude211.53 degrees
1997 Distance from Earth16.68 Parallax (milliarcseconds)
 195.54 Light Years
 59.95 Parsecs
2007 Revised Distance from Earth18.03 Parallax (milliarcseconds)
 180.90 Light Years
 55.46 Parsecs
Galacto-Centric Distance24,198.06 Light Years / 7,419.00 Parsecs
Proper Motion Dec.-61.78 ± 0.39 milliarcseconds/year
Proper Motion RA.-399.99 ± 0.60 milliarcseconds/year
B-V Index0.59
Radial Velocity0.62 ± 0.14 km/s
Iron Abundance-0.37 ± 0.02 Fe/H
Spectral TypeG0
Colour(G) White to Yellow

Estimated Facts

Calculated Effective Temperature5,898 Kelvin

Sources and Links

SIMBAD SourceLink

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