Difference between revisions of "Main sequence star"

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(New page: Main Sequence is the stable phase of a star's lifetime, when outward pressure from internal fusion process using hydrogen for fuel is balanced by the inward force of self-gravitation. This...)
 
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Our [[Sun]] is a main sequence [[star]].
 
Our [[Sun]] is a main sequence [[star]].
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[[category:astronomy]]

Revision as of 16:15, July 18, 2007

Main Sequence is the stable phase of a star's lifetime, when outward pressure from internal fusion process using hydrogen for fuel is balanced by the inward force of self-gravitation. This phase is usually the longest phase of a star's lifetime.

Our Sun is a main sequence star.