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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...

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]].

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Main sequence star (view source)

Revision as of 00:45, June 2, 2007

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