24 Ursae Majoris is a white to yellow eclipsing binary system subgiant star that can be located in the constellation of Ursa Major. The description is based on the spectral class. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it. It is calculated at being 4.604 Billion Years old. This information comes from ExoPlanet.
The Id of the star in the Yale Bright Star Catalogue is HR3771. HIP46977 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD82210. The Gliese ID of the star is GL 355.1. The star was part of the original catalogue devised by German Astronomer Wilheim Gliese of stars located within 20 parsecs of Earth. Star Names
24 Ursae Majoris has alternative name(s) :- DK Ursae Majoris, DK UMa.
Flamsteed designations are named after the creator, Sir John Flamsteed. Sir John numbered the stars in the constellation with a number and the latin name, this star's Flamsteed designation is 24 Ursae Majoris with it shortened to 24 UMa.
BD number is the number that the star was filed under in the Durchmusterung or Bonner Durchmusterung, a star catalogue that was put together by the Bonn Observatory between 1859 to 1903. The star's BD Number is BD+70 565.
More details on star alternative names can be found at Star Names .
The location of the star in the night sky 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 24 Ursae Majoris, the location is 09h 34m 28.97 and +69° 49` 48.6 .
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 77.25 ± 0.13 miliarcseconds/year towards the north and -63.84 ± 0.19 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 -27.00000 km/s with an error of about 0.20 km/s .
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 15.77 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012.
24 Ursae Majoris has a spectral type of G4III-IV. This means the star is a white to yellow subgiant star. The star is 7,420.00 Parsecs from the Galactic Centre or terms of Light Years is 24,201.32 s. The star has a B-V Colour Index of 0.78 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 5,337 Kelvin.
24 Ursae Majoris Radius has been calculated as being 4.37 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 3,039,302.22.km. If you need the diameter of the star, you just need to multiple the radius by 2. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 4.31. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures. The star's solar mass is 1.23 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 4.60 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.
24 Ursae Majoris has an apparent magnitude of 4.54 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 1.99 If you used the 2007 Parallax value, you would get an absolute magnitude of 2.02. 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 30.89 which gave the calculated distance to 24 Ursae Majoris as 105.59 light years away from Earth or 32.37 parsecs. It would take a spaceship travelling at the speed of light, 105.59 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 31.32 which put 24 Ursae Majoris at a distance of 104.14 light years or 31.93 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 7,420.00 Parsecs or 24,201.32 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*.
The star is a eclipsing binary system RS Canum Venaticorum 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. 24 Ursae Majoris brightness ranges from a magnitude of 4.717 to a magnitude of 4.672 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 0.0 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 Metallicity and/or Mass is from the E.U. Exoplanets. The information was obtained as of 12th Feb 2017.
|Primary / Proper / Traditional Name||24 Ursae Majoris|
|Alternative Names||D Uma, DK Ursae Majoris, HD 82210, HIP 46977, HR 3771, 24 UMa, BD+70 565, Gliese 355.1, DK UMa|
|Multiple Star System||No / Unknown|
|Star Type||Subgiant Star|
|Colour||white to yellow|
|Age||4.60 Billion Years Old|
|Absolute Magnitude||1.99 / 2.02|
|Visual / Apparent Magnitude||4.54|
|Naked Eye Visible||Yes - Magnitudes|
|Right Ascension (R.A.)||09h 34m 28.97|
|Declination (Dec.)||+69° 49` 48.6|
|Galactic Latitude||38.93 degrees|
|Galactic Longitude||142.55 degrees|
|1997 Distance from Earth||30.89 Parallax (milliarcseconds)|
|105.59 Light Years|
|2007 Distance from Earth||31.32 Parallax (milliarcseconds)|
|104.14 Light Years|
|Galacto-Centric Distance||24,201.32 Light Years / 7,420.00 Parsecs|
|Proper Motion Dec.||77.25 ± 0.13 milliarcseconds/year|
|Proper Motion RA.||-63.84 ± 0.19 milliarcseconds/year|
|Radial Velocity||-27.00 ± 0.20 km/s|
|Iron Abundance||-0.25 ± 9.99 Fe/H|
|Stellar Luminosity (Lsun)||15.77|
|Variable Star Class||Eclipsing binary system|
|Variable Star Type||RS Canum Venaticorum|
|Mean Variability Period in Days||0.034|
|Variable Magnitude Range (Brighter - Dimmer)||4.672 - 4.717|
|Calculated Effective Temperature||5,337 Kelvin|
|Mass Compared to the Sun||1.23|