| Catalogue Names | |
| Names | Mizar |
| Type | Double Star |
| Constellation | Ursa Major |
| Season | Summer; April-September |
| Notes | Good introduction to double stars. Naked eye apparent double really isn’t, but the telescope reveals a true double. |
This companion star is called Alcor.
In this image of a 6×30 finder you can see Mizar and Alcor.
This is not a true double star — it is called an apparent double because the two stars seem close together because of our line of sight. In fact, they are quite far apart, and they are not a system — i.e., they are not gravitationally bound to each other.
Alcor will now be well-separated from Mizar. But look at Mizar: it is beginning to “bud”. A small companion is becoming visible at this magnification.
These two stars, Mizar A and Mizar B, are a true double star system — they are orbiting one another at close distance. (About 340 Astronomical Units, or about 8 times the distance from our Sun to Pluto.)
Raising the magnification until the components of a double star are cleanly separated is called “splitting the double”. Some doubles are so close that splitting them requires very high power, very high quality optics, and very steady air.
It goes even further (but not with your telescope). Spectroscopic analysis reveals that Mizar A and Mizar B are each, themselves, double stars. So Mizar is a system of at least 4 stars, possibly more, only two of which we can see with our telescopes.