The Constellation Virgo |
This region of interesting galaxies sweeps right up through Coma Berenices and is often called the "Virgo-Coma Cluster". One of the best is the Black Eye Galaxy, just to the left of that little star right there {point out 35 Comae}. You can spot it with the binoculars, although we need a relatively large telescope (8" or better) to see the black eye at the center. It's actually a lane of dust that is the result of a collision with another galaxy -- literally smacking into this one and leaving it with a black eye.
As the earth goes around the sun, this motion means that every day we look back at the sun in a slightly different direction, with different stars behind it. The sun appears to move through the constellations. Theoretically there are twelve constellations through which the sun moves, one per month, and these are the Zodiac constellations. In reality there is a 13th constellation through which the sun passes (technically at least) and it gets no credit for being in the Zodiac - Ophiuchus.
Astronomers measure star brightness using 'magnitudes' -- Arcturus has a magnitude of 0, Spica has a magnitude of 1, Polaris has a magnitude of 2. As magnitude number goes up, brightness goes down. A magnitude 1 is 2½ times as bright as a magnitude 2, a 2 is 2½ times as bright as a 3, and so on.
This comes from the system set up by ancient Greeks, where the brightest stars were stars of the first magnitude, like 'first class', and the faintest stars you could see were stars of the sixth magnitude. When astronomers got telescopes and instruments that could measure star brightness, they found 1st magnitude stars were almost exactly 100 times the brightness of 6th magnitude stars. That works out to a factor of 2½ from one magnitude to the next.
Magnitudes can go negative for stars brighter than 0 magnitude Arcturus. The brightest star in the sky is Sirius (in the winter sky), which has a magnitude -1.5.
Well, what's really the brightest star in the sky? The sun has a magnitude of -27.
Yup, that's right. Different colors show different temperatures. So which star color is the hottest? Just like a flame, blue is the hottest part, yellow is next, red is the coolest. The sun is a yellow star, about 10,000°F at the surface. A red star is about half the sun's surface temperature, whereas a blue star is three to five times as hot as the sun. White stars are somewhere between the yellow ones and blue ones.
Now, all stars are made of pretty much the same stuff -- about 90% hydrogen and the rest is helium with some traces of other stuff. So, why would one star be burning hotter than another? The answer is in the size of the star. The more massive it is, the more pressure there is at the center and therefore the hotter - and for that matter the brighter - the star burns. So blue stars are the biggest and brightest of stars, and red stars are the smallest and dimmest.
So why is red Antares so bright? Hmmm... yeah... well, like with most rules, there are exceptions to the rule, and this rule is no exception. Antares is a star that is literally running out of gas. As a star burns up all the hydrogen at its center, it starts to burn helium (which is the "ash" from the hydrogen burning), which makes it expand, get brighter, and turn red -- it becomes a red giant. This is the time you can get a bright red star, when the star is near the end of its life.
When our sun starts burning out it will expand so big it will swallow up Mercury and Venus and scorch the surface of the earth to a cinder. If you are hoping to see all that happen you will have to wait about 5 billion years.
So there are two reasons a star could be red -- it is massive (and once was yellow, white or even blue) and is now burning out (a red giant), or it never had enough mass to burn any hotter than red (a red dwarf).
Notice that when we graph out the stars showing their temperature (or color) against their brightness, most of them fall along a line -- this line is called the Main Sequence, and the graph is called the "H-R" (for Hertzsprung-Russell) Diagram. Others are not on the main sequence, mostly stars that are either just being born (called "T-Tauri" stars) or stars that are near the end of life.
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Updated 11 November 2011