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I think about and I look at that process in stars, in that our star is fundamentally an early stage star that's burning just hydrogens. But when it burns and does
fusion, those hydrogens combine into heliums, and later stage stars can then burn those heliums and they can fuse those together to form even heavier elements and carbons. And those carbons can fuse
together and form heavier elements. And that whole stellar process is something that inspires us at Helion to think about what are fusion fuels, not just the
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