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| a zodiacal constellation between Gemini and Aries, containing the bright star Aldebaran also called the Bull |
| a number of heavenly bodies associated and acting together according to certain natural laws |
| main sequence | |
| —n | |
| astronomy | |
| a. a diagonal band on the Hertzsprung Russell diagram containing about 90% of all known stars; stars evolve onto and then off the band during their lifetime | |
| b. (as modifier): a main-sequence star | |
| main sequence (mān) Pronunciation Key
The continuous, generally diagonal line or band in the Hertzsprung-Russell diagram ranging from the upper left to the lower right and representing stars of average size whose luminosities correspond predictably to their surface temperatures. Stars in this grouping maintain a stable nuclear reaction and experience only small fluctuations in luminosity and temperature. Main-sequence stars are believed to be in the stable, middle phase of their development; they are expected to move off the main sequence once the hydrogen in their core is exhausted. At that point, depending on its size, a main-sequence star will become a giant star, a supergiant star, or a white dwarf. The more massive the star, the faster it burns its nuclear fuel and the shorter it remains in the main sequence. See more at Hertzsprung-Russell diagram, star. |