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main sequence
(redirected from Main-sequence)

   Also found in: Wikipedia, Hutchinson 0.10 sec.
main sequence [′mān ′sē·kwəns]
(astronomy)
The band in the spectrum luminosity diagram which has the great majority of stars; their energy derives from core burning of hydrogen into helium.


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This would make Beta Pictoris far too young to qualify as a main-sequence star, burning hydrogen at its core.
Over billions of years, enough of this material could accumulate in a main-sequence star to leave a core of strange matter when the star dies.
For nearly a decade, Beta Pictoris has reigned as the only mature, main-sequence star with an encircling disk of dust - perhaps much like the disk from which our solar system evolved 4.
 
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