Megrez / Delta Ursae Majoris Star Facts (Type, Distance, Magnitude, Age, Colour, Location and more)
Megrez, also known as Delta Ursae Majoris (Bayer) is a main sequence star located in the constellation of Ursa Major, The Big Bear. Megrez is a major star and forms part of the constellation.
Based on the spectral type (A3Vvar), Megrez colour is blue - white, although not the hottest stars, they are considerably hotter than our own star which is white.


Megrez temperature is in the range of between 7,500 and 10,000 Kelvin. Megrez effective temperature is 6,907 Kelvin which is hotter than the Sun's effective temperature, which is 5,777 Kelvin. Based on a parallax of 40.51, Megrez distance from Earth can be calculated at being 80.51 light years away or 24.97 parsecs.
Megrez is a naked-eye star, so you don't need a telescope or binoculars when you look up on a clear night. The lower the magnitude, the easier it will be to see it.
Location
The location of the Megrez in the night sky is determined by the right ascension (R.A.) and declination (Dec.). These are equivalent to the Longitude and Latitude on Earth. The Right Ascension (Longitude) is expressed in time (hh:mm:ss) and is how far the star is along Earth's celestial equator. If the R.A. is positive, then it's eastwards and vice versa.
The Declination (Latitude) is how far north or south the object is compared to the celestial equator and is expressed in degrees. If the value is positive, it is north of the celestial equator. For Megrez, the location is 12h 15m 25.45 and +57° 01` 57.4 .
Based on the location of Ursa Major, Megrez can be located in the northern hemisphere of the celestial sky. The celestial hemisphere is equivalent to the hemispheres on Earth. Megrez is north of the Ecliptic. The Ecliptic is the path that the Earth takes as it orbits the Sun. As the Earth is titled, we therefore have Celestial and Ecliptic hemispheres and they can be different for a star.
Physical Properties
Spectral Type
Megrez spectral type of A3Vvar which means its colour and type is blue - white main sequence star. There is no relationship between colour and size. For example, a red star can be large or small. Small stars are more energy efficient than larger stars and live longer.
Megrez Luminosity
Luminosity is the amount of energy a star pumps out relative to the amount that our star, the Sun, gives out. Our star, the Sun's value is 1. Megrez Luminosity figure of 23.243 comes from the Vizier online catalogue. The star generates more energy than our star.
Megrez Size (Radius)
Megrez radius has been calculated as being 3.37 times bigger than the Sun. The Sun's radius is 695,800km, therefore, the Megrez radius is an estimated 2,344,846.km. If you need the star's diameter, you just need to multiply the radius by 2.
Iron Abundance
Megrez Iron Abundance is -0.443 with an error value of 9.99 Fe/H, with the Sun having a value of 1 to put it into context. The value comes from the Hipparcos Extended Catalog.
Megrez Surface Gravity
The Surface Gravity of Megrez as measured in CGS (Centimeter-Gram-Second) is 3.943. The gravity has a relationship to its mass and radius. The larger the mass, the larger the gravity. Megrez surface gravity has an uncertainty range of between - and +.
Magnitude (Apparent / Absolute / Visible)
A number represents a star’s magnitude, whether apparent/visual or absolute. The smaller the number, the brighter the star is. The Sun is the brightest star and therefore has the lowest of all magnitudes, -26.74. A faint star will have a high number.
Megrez apparent magnitude is 3.32, which is a measure of the star's brightness as seen from Earth. Apparent Magnitude is also known as Visual Magnitude.
If you use the 1997 parallax value, Megrez' absolute magnitude is 1.33. If you use the 2007 parallax value, Megrez' absolute magnitude is 1.36. Absolute Magnitude is the star's apparent magnitude from 10 parsecs or 32.6 light years. The magnitude assumes nothing is between the object and the viewer, such as dust clouds. To compare different stars' actual brightness, you would best use Absolute rather than Apparent Magnitude.
Megrez is visible from Earth without needing binoculars or a telescope. The lower the Apparent Magnitude of a star or other object is, the easier it is to see in the night sky. An object with a magnitude greater than 6.5 cannot be seen without a telescope or other device.
Radial Velocity and Proper Motion
In simplistic terms, all non-rogue stars, like planets, orbit around a central object, although that is actually not true. Where is the centre of the Solar System. For simplicity it's the central star, such as the Sun. In the case of a star, it's the galactic centre. The constellations 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 is measured in milliarcseconds. Megrez is moving 7.3 ± 0.11 milliarcseconds/year towards the north and 104.11 ± 0.15 milliarcseconds/year east if we saw them in the horizon.
The radial velocity, the speed at which the Megrez is towards the Sun, is -15.30000 km/s with an error of about 0.50 km/s . When the value is negative, the star and the Sun are getting closer to one another; likewise, a positive number means that two stars are moving away. It's nothing to fear as the stars are so far apart they won't collide in our lifetime, if ever.
Megrez Fact Table
The table is scrollable if you can't see everything, just swipe the table to see the hidden information.
| Primary Name | Megrez |
|---|---|
| Spectral Type | A3Vvar |
| Star Type | High proper-motion Star |
| Colour | blue - white |
| Galaxy | Milky Way |
| Constellation | Ursa Major |
| Main Star | Yes |
| Absolute Magnitude | 1.33 / 1.36 |
| Visual / Apparent Magnitude | 3.32 |
| Visible From Earth | Yes |
| Right Ascension (R.A.) | 12h 15m 25.45 |
| Declination (Dec.) | +57° 01` 57.4 |
| Galactic Latitude | 59.41686902 ° |
| Galactic Longitude | 132.56710106 ° |
| 1997 Distance from Earth | 40.05000 Parallax (milliarcseconds) |
| 81.44 Light Years | |
| 24.97 Parsecs | |
| 2007 Distance from Earth | 40.51000 Parallax (milliarcseconds) |
| 80.51 Light Years | |
| 24.69 Parsecs | |
| 5,092,642.58 Astronomical Units | |
| Galacto-Centric Distance | 24,165.442 Light Years / 7,409 Parsecs |
| Proper Motion Dec. | 7.30000 ± 0.11000 milliarcseconds/year |
| Proper Motion RA. | 104.11000 ± 0.15000 milliarcseconds/year |
| B-V Index | 0.07 |
| Radial Velocity | -15.30000 ± 0.5 km/s |
| Iron Abundance (Fe/H) | -0.4433 ± 9.99 |
| Eccentricity | 0.21410 |
| Semi-Major Axis | 8751.0000000 |
| Luminosity (Lsun) | 23.2430000 |
| Effective Temp. (Kelvin) | 6,907 |
| Surface Gravity (cgs) | 3.943 |
| Radius | 3.37 |
Sources and Links
| Modified Date | 24th July 2024 |
| Published Date | Jan 2015 |
| SIMBAD Source | Link |
| Source | Vizier, Vizier, |
Ursa Major's Main Stars in Brightness Order
- Dubhe (Alpha Ursae Majoris)
- Merak (Beta Ursae Majoris)
- Phecda (Gamma Ursae Majoris)
- Megrez (Delta Ursae Majoris)
- Alioth (Epsilon Ursae Majoris)
- Alcor
- Alkaid (Eta Ursae Majoris)
- Sarir (Theta Ursae Majoris)
- Talitha (Iota Ursae Majoris)
- Alkaphrah (Kappa Ursae Majoris)
- Tania Borealis (Lambda Ursae Majoris)
- Tania Australis (Mu Ursae Majoris)
- Alula Borealis (Nu Ursae Majoris)
- Muscida (Omicron Ursae Majoris)
- Upsilon Ursae Majoris
- Phi Ursae Majoris
- Taiyangshou (Chi Ursae Majoris)
- Psi Ursae Majoris
- 23 Ursae Majoris
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Comments and Questions
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William Creed
When I was a kid in around 1955 to 1969 that star was very visible in the night. Why has it seemed to fade over the 20 some years.