The ancient Greeks thought this group of stars looked like a hunter, so they named it Orion after their mythical hunter. The line of three stars at the center is "Orion's Belt." The many different colors of stars reflect the star’s temperature. The bright, red star in the upper left (with an arrow pointing to it), named Betelgeuse (pronounced BET-ul-juice), is not as hot than the blue star in the lower right, named Rigel.
Think about how the color of a piece of metal changes with temperature. A coil of an electric stove will start out black, but with added heat will start to glow a dull red. With more heat, the coil turns a brighter red, then orange. At extremely high temperatures the coil will turn yellow-white, or even blue-white (it’s hard to imagine a stove coil getting that hot). A star’s color is also determined by the temperature of the star’s surface. Relatively cool stars are red, warmer stars are orange or yellow, and extremely hot stars are blue or blue-white (Figure below).
A Hertzsprung-Russell diagram shows the brightness and color of main sequence stars. The brightness is indicated by luminosity and is higher up the y-axis. The temperature is given in degrees Kelvin and is higher on the left side of the x-axis. How does our Sun fare in terms of brightness and color compared with other stars?
Color is the most common way to classify stars. Table below shows the classification system. The class of a star is given by a letter. Each letter corresponds to a color, and also to a range of temperatures. Note that these letters don’t match the color names; they are left over from an older system that is no longer used.
| Class | Color | Temperature Range | Sample Star |
|---|---|---|---|
| O | Blue | 30,000 K or more | Zeta Ophiuchi |
| B | Blue-white | 10,000–30,000 K | Rigel |
| A | White | 7,500–10,000 K | Altair |
| F | Yellowish-white | 6,000–7,500 K | Procyon A |
| G | Yellow | 5,500–6,000 K | Sun |
| K | Orange | 3,500–5,000 K | Epsilon Indi |
| M | Red | 2,000–3,500 K | Betelgeuse, Proxima Centauri |
For most stars, surface temperature is also related to size. Bigger stars produce more energy, so their surfaces are hotter.
| Color | Highlighted Text | Notes | |
|---|---|---|---|
| Please Sign In to create your own Highlights / Notes | |||
| Image | Reference | Attributions |
|---|---|---|
| Credit: Courtesy of Akira Fujii and the Hubble European Space Agency, modified by Henrykus;Courtesy of H. Bond (STScI), and M. Barstow (University of Leicester), NASA/ESA Source: http://commons.wikimedia.org/wiki/File:Betelgeuse_position_in_Orion.png;http://commons.wikimedia.org/wiki/File:Sirius_A_and_B_Hubble_photo.jpg License: Public Domain | ||
| Credit: CK-12 Foundation Source: CK-12 Foundation License: CK-12 Curriculum Materials License |
Your search did not match anything in .