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<p>The <b>neon-burning process</b> is a set of <a href="page.php?w=nuclear_fusion">nuclear fusion</a> reactions that take place in <a href="page.php?w=stellar_evolution">evolved</a> massive <a href="page.php?w=star">star</a>s with at least 8 <a href="page.php?w=Solar_mass">Solar mass</a>es. Neon burning requires high temperatures and <a href="page.php?w=density">densities</a> (around 1.2 billion <a href="page.php?w=kelvin">K</a> or 100 <a href="page.php?w=keV">keV</a> and 4 billion kg/m<sup>3</sup>).</p>

<p><big>Process</big></p>
<p><big>Formulae</big></p>
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