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75 Ursae Majoris, HD108861, HIP60992, HR4762

75 Ursae Majoris is a white to yellow star that can be located in the constellation of UrsaMajor. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.

The Id of the star in the Yale Bright Star Catalogue is HR4762. HIP60992 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD108861.

Location of 75 Ursae Majoris

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 75 Ursae Majoris, the location is 12h 30m 04.22 and +58d 46` 04.1 .

Proper Motion of 75 Ursae Majoris

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 -14.11 ± 0.21 miliarcseconds/year towards the north and 30.35 ± 0.30 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 -15.10000 km/s with an error of about 0.30 km/s .

Physical Properties (Colour, Temperature, Radius) of 75 Ursae Majoris

75 Ursae Majoris has a spectral type of G8III-IV. This means the star is a white to yellow star. The star is 7440.00000000 Parsecs from the Galactic Centre or terms of Light Years is 24266.5527936000000000s. The star has a B-V Colour Index of 0.98 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 4,888 Kelvin.

75 Ursae Majoris Radius has been calculated as being 10.44 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 7,263,078.25.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 9.52. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

75 Ursae Majoris Apparent and Absolute Magnitudes

75 Ursae Majoris has an apparent magnitude of 6.07 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 0.48 If you used the 2007 Parallax value, you would get an absolute magnitude of 0.68. 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 75 Ursae Majoris

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 7.62 which gave the calculated distance to 75 Ursae Majoris as 428.04 light years away from Earth or 131.23 parsecs. It would take a spaceship travelling at the speed of light, 428.04 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 8.35 which put 75 Ursae Majoris at a distance of 390.61 light years or 119.76 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 7,440.00 Parsecs or 24,266.55 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.

75 Ursae Majoris Facts

Alternative Names

Traditional/Proper Name75 Ursae Majoris
Flamsteed Name75 Ursae Majoris
Flamsteed Short Name75 UMa
Hipparcos Library I.D.60992
Yale Bright Star Catalogue (HR) Id4762
Bonner DurchmusterungBD+59 1446
Henry Draper Designation108861

Visual Facts

Star Type star
ConstellationUrsa Major
Absolute Magnitude0.48 / 0.68
Visual / Apparent Magnitude6.07
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)12h 30m 04.22
Declination (Dec.)+58d 46` 04.1
Galactic Latitude58.14 degrees
Galactic Longitude128.18 degrees
1997 Distance from Earth7.62 Parallax (milliarcseconds)
 428.04 Light Years
 131.23 Parsecs
2007 Revised Distance from Earth8.35 Parallax (milliarcseconds)
 390.61 Light Years
 119.76 Parsecs
Galacto-Centric Distance24,266.55 Light Years / 7,440.00 Parsecs
Proper Motion Dec.-14.11 ± 0.21 milliarcseconds/year
Proper Motion RA.30.35 ± 0.30 milliarcseconds/year
B-V Index0.98
Radial Velocity-15.10 ± 0.30 km/s
Spectral TypeG8III-IV
Colour(G) White to Yellow

Estimated Facts

Calculated Effective Temperature4,888 Kelvin

Sources and Links

SIMBAD SourceLink

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