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<p>a surface temperature of only about 1000 K at their hottest.Within 50&nbsp;million years, the temperature and pressure at the core of the Sun became so great that its hydrogen began to fuse, creating an internal source of energy that countered gravitational contraction until <a href="page.php?w=hydrostatic_equilibrium">hydrostatic equilibrium</a> was achieved. This marked the Sun's entry into the prime phase of its life, known as the <a href="page.php?w=main_sequence">main sequence</a>. Main-sequence stars derive energy from the fusion of hydrogen</p><p>
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