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Stellar nucleosynthesis is the process where stars forge heavier elements from lighter ones via nuclear fusion in their cores, primarily converting hydrogen to helium and subsequently creating carbon, oxygen, and beyond during various stellar life stages.
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The Chandrasekhar Limit defines the maximum mass (approximately 1.44 solar masses) a white dwarf star can have before it collapses under its own gravity, typically triggering a supernova.
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Okay, here's a factual sentence fitting that description: **Nucleosynthesis is the process by which atomic nuclei are built from protons and neutrons, primarily occurring within stars and during the Big Bang to create heavier elements.** (158 characters)
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