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65 Ursae Majoris A,B,C, 65 Ursae Majoris, HD103483, HIP58112

65 Ursae Majoris A,B,C is a blue eclipsing binary system main sequence dwarf star that can be located in the constellation of UrsaMajor. The star can not be seen by the naked eye, you need a telescope to see it.

HIP58112 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD103483.

65 Ursae Majoris A,B,C has alternative name(s), DN UMa.

Location of 65 Ursae Majoris A,B,C

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 65 Ursae Majoris A,B,C, the location is 11h 55m 05.74 and +46d28`36.6 .

Proper Motion of 65 Ursae Majoris A,B,C

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 2.38 ± 0.35 miliarcseconds/year towards the north and 10.41 ± 0.58 miliarcseconds/year east if we saw them in the horizon.

65 Ursae Majoris A,B,C Luminosity

Luminosity is the amount of energy that a star pumps out and its relative to the amount that our star, the Sun gives out. The figure of 14.0000000 that I have given is based on the Spectral Types page that I have found on the Internet. You might find a different figure, one that may have been calculated rather than generalised that I have done. The figure is always the amount times the luminosity of the Sun. It is an imprecise figure because of a number of factors including but not limited to whether the star is a variable star and distance.

Physical Properties (Colour, Temperature, Radius) of 65 Ursae Majoris A,B,C

65 Ursae Majoris A,B,C has a spectral type of A3Vn. This means the star is a blue main sequence dwarf star. The star is 7471.00000000 Parsecs from the Galactic Centre or terms of Light Years is 24367.6634302400000000s. The star has a B-V Colour Index of 0.11 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 8,375 Kelvin.

65 Ursae Majoris A,B,C Radius has been calculated as being 5.36 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 3,727,539.24.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 4.62. 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 -0.62 with an error value of 9.99 Fe/H with the Sun has a value of 1 to put it into context.

The star has a companion star which is in orbit close by, it has at least the following companions in close orbit, .

65 Ursae Majoris A,B,C Apparent and Absolute Magnitudes

65 Ursae Majoris A,B,C has an apparent magnitude of 6.54 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 -0.41 If you used the 2007 Parallax value, you would get an absolute magnitude of -0.09. 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 65 Ursae Majoris A,B,C

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 4.07 which gave the calculated distance to 65 Ursae Majoris A,B,C as 801.38 light years away from Earth or 245.70 parsecs. It would take a spaceship travelling at the speed of light, 801.38 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 4.72 which put 65 Ursae Majoris A,B,C at a distance of 691.02 light years or 211.86 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 7,471.00 Parsecs or 24,367.66 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*.

Variable Type of 65 Ursae Majoris A,B,C

The star is a eclipsing binary system Beta Lyrae (Sheliak) 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. 65 Ursae Majoris A,B,C brightness ranges from a magnitude of 6.660 to a magnitude of 6.550 over its variable period. The smaller the magnitude, the brighter the star.

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.

65 Ursae Majoris A,B,C Facts

Alternative Names

Traditional/Proper Name65 Ursae Majoris A,B,C
Flamsteed Name65 Ursae Majoris
Flamsteed Short Name65 UMa
Short NameDN UMa
Hipparcos Library I.D.58112
Bonner DurchmusterungBD+47 1913
Henry Draper Designation103483

Visual Facts

Star Typemain sequence dwarf star
Absolute Magnitude-0.41 / -0.09
Visual / Apparent Magnitude6.54
Naked Eye VisibleRequires a 7x50 Binoculars - Magnitudes
Right Ascension (R.A.)11h 55m 05.74
Declination (Dec.)+46d28`36.6
Galactic Latitude67.68 degrees
Galactic Longitude149.12 degrees
1997 Distance from Earth4.07 Parallax (milliarcseconds)
 801.38 Light Years
 245.70 Parsecs
2007 Revised Distance from Earth4.72 Parallax (milliarcseconds)
 691.02 Light Years
 211.86 Parsecs
Galacto-Centric Distance24,367.66 Light Years / 7,471.00 Parsecs
Proper Motion Dec.2.38 ± 0.35 milliarcseconds/year
Proper Motion RA.10.41 ± 0.58 milliarcseconds/year
B-V Index0.11
Radial Velocity-3.90 ± 4.40 km/s
Iron Abundance-0.62 ± 9.99 Fe/H
Spectral TypeA3Vn
Colour(A) blue

Variable Star Details

Variable Star ClassEclipsing binary system
Variable Star TypeBeta Lyrae (Sheliak)
Variable Magnitude Range (Brighter - Dimmer)6.550 - 6.660

Estimated Facts

Luminosity (x the Sun)14.0000000
Calculated Effective Temperature8,375 Kelvin

Sources and Links

SIMBAD SourceLink

Related Stars

Multi-Star System

The star has been identified as being a multi-star system, one in which there is at least one star in close orbit to another star or two or more stars orbiting a central point. The stars may be of equal mass, unequal mass where one star is stronger than the other or be in groups orbiting a central point which doesn't necessarily have to be a star. More information can be found on my dedicated multiple star systems page. The source of the info is Simbad. The file is dated 2000 so any differences between this and any other source will be down to the actual source from where the information came from.


Proper Motion mas/yr
H.D. IdB.D. IdStar CodeMagnitudeR.A.Dec.SpectrumColourYear
103483+47 1913.0A6.70000-1.000003.00000A0White
B8.500001958
C8.300001832

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