Red supergiant
From Free net encyclopedia
Red supergiants are supergiant stars of spectral type K-M and a luminosity class of I. They are the largest stars in the universe in terms of physical size, although they are not the most massive.
Stars with more than about 10 solar masses, after burning their hydrogen become red supergiants during their helium-burning phase. These stars have very cool surface temperatures (3500-4500 K), and enormous radii. The three largest known red supergiants in the Galaxy are KW Sagitarii, V354 Cephei, and KY Cygni. All have radii about 1500 times that of the sun, or about 7 astronomical units. Most red supergiants have their radii between 200 and 800 times that of the sun which is still enough to reach from the sun to Earth or Mars.
These massively large stars are little more than "hot vacuums", having no distinct photosphere and simply "tailing off" into interstellar space. They have a slow, dense, stellar wind and if their core's nuclear reactions slow for any reason (such as transitioning between shell fuels) they may shrink into a blue supergiant. A blue supergiant has a fast but sparse stellar wind and causes the material already expelled from the red supergiant phase to compress into an expanding shell. See blue supergiant for further discussion.
The red supergiant phase is relatively short, lasting only a few hundred thousand to a million or so years. The most massive of the red supergiants are thought to evolve to Wolf-Rayet stars, while lower mass red supergiants will likely end their lives as supernovae. Most stars are thought to swing back and forth between red and blue supergiants several times until they finally explode.
Betelgeuse and Antares are the best known examples of red supergiants.