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14 Leonis Minoris - HD84453 - HIP47973

14 Leonis Minoris is a orange to red subgiant star that can be located in the constellation of UrsaMajor. It is calculated at being 5.000 Billion Years old. This information comes from ExoPlanet. HIP47973 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD84453. 14 Leonis Minoris has alternative name(s), 14 Ursae Majoris , 14 UMa.

Location of 14 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 14 Leonis Minoris, the location is 09h 46m 42.44 and +45d06`53.0 .

Proper Motion of 14 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 -131.37 ± 000.33 towards the north and 055.04 ± 000.56 east if we saw them in the horizon.

Physical Properties (Colour, Temperature, Age, Mass, Radius) of 14 Leonis Minoris

14 Leonis Minoris has a spectral type of K0IV. This means the star is a orange to red subgiant star. The star has a B-V Colour Index of 0.94 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 4,968 Kelvin.

14 Leonis Minoris has been calculated as 4.53 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 3,155,025.41.km. The star's solar mass is 1.00 times that of the Sun's. The Sun's Mass is 1,989,100,000,000,000,000,000 billion kg. which to calculate using this website is too large. To give idea of size, the Sun is 99.86% the mass of the solar system.

The star's metallicity is -0.250000, this value is the fractional amount of the star that is not Hydrogen (X) or Helium (Y). An older star would have a high metallicity whereas a new star would have a lower one.

The star is believed to be about 5.00 Billion years old. To put in context, the Sun is believed to be about five billion years old and the Universe is about 13.8 billion years old.

14 Leonis Minoris Apparent and Absolute Magnitudes

14 Leonis Minoris has an apparent magnitude of 6.81 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 2.22 If you used the 2007 Parallax value, you would get an absolute magnitude of 2.27. 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 14 Leonis Minoris

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 12.06 which gave the calculated distance to 14 Leonis Minoris as 270.45 light years away from Earth or 82.92 parsecs. It would take a spaceship travelling at the speed of light, 270.45 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 12.35 which put 14 Leonis Minoris at a distance of 264.10 light years or 80.97 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.

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 Stellar Age, Metallicity or Mass is from the E.U. Exoplanets. The information was obtained as of 12th Feb 2017.

14 Leonis Minoris Facts

Alternative Names

Traditional Name14 Leonis Minoris
Short Name14 UMa
Alternative Name(s)14 Ursae Majoris
Hipparcos Library I.D.47973
Bonner DurchmusterungBD+45 1762
Henry Draper Designation84453

Visual Facts

Star Typesubgiant star
Age5.000 Billions of Years
Absolute Magnitude2.22 / 2.27
Apparent Magnitude6.81
Right Ascension (R.A.)09h 46m 42.44
Declination (Dec.)+45d06`53.0
1997 Distance from Earth12.06 Parallax (milliarcseconds)
 270.45 Light Years
 82.92 Parsecs
2007 Revised Distance from Earth12.35 Parallax (milliarcseconds)
 264.10 Light Years
 80.97 Parsecs
Proper Motion Dec.-131.37 ± 0.33 milliarcseconds/year
Proper Motion RA.55.04 ± 0.56 milliarcseconds/year
B-V Index0.94
Spectral TypeK0IV
Colour(K) Orange to Red

Estimated Facts

Radius (x the Sun)4.53
Calculated Effective Temperature4,968 Kelvin
Mass Compared to the Sun1.00

Sources and Links

SIMBAD SourceLink

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