Main sequence star
From Conservapedia
This is an old revision of this page, as edited by Barikada (Talk | contribs) at 00:03, January 27, 2008. It may differ significantly from current revision.
- It has been proposed that this page, :Main sequence star, be titled, "Main Sequence Star".
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.
