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<p><sup>32,33,34</sup>S, <sup>35,37</sup>Cl, <sup>36,38</sup>Ar, <sup>39,41</sup>K, and <sup>40,42</sup>Ca. Of these, <sup>28</sup>Si and <sup>32</sup>S constitute 90% of the final composition. The oxygen fuel within the core of the star is exhausted after 0.01-5 years, depending on the star's mass and other parameters. The <a href="page.php?w=silicon-burning_process">silicon-burning process</a>, which follows, creates iron, but this iron cannot react further to create energy to support the star.</p>

<p>During the oxygen-burning process, proceeding</p><p>
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