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<ref name="prialnik00">{{cite book |first=Dina |last=Prialnik |date=2000 |title=An Introduction to the Theory of Stellar Structure and Evolution |publisher=Cambridge University Press |isbn=978-0-521-65937-6}}</ref>
<ref name=mnras386_1>{{cite journal |author1=Schröder, K.-P. |author2=Connon Smith, Robert |title=Distant future of the Sun and Earth revisited |journal=Monthly Notices of the Royal Astronomical Society |date=May 2008 |volume=386 |issue=1 |pages=155–163 |bibcode=2008MNRAS.386..155S |doi=10.1111/j.1365-2966.2008.13022.x |doi-access=free |arxiv=0801.4031 |s2cid=10073988}}</ref>
<ref name=arnett96>{{cite book |first=David |last=Arnett |date=1996 |title=Supernovae and Nucleosynthesis: An Investigation of the History of Matter, from the Big Bang to the Present |publisher=Princeton University Press |isbn=978-0-691-01147-9}}—Hydrogen fusion produces 8×10<sup>14</sup> [[joule|J]]/[[kilogram|kg]] while helium fusion produces 8×10<sup>13</sup> J/kg.</ref>
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