Stellar Nucleosynthesis
Embed This Widget
Add the script tag and a data attribute to embed this widget.
Embed via iframe for maximum compatibility.
<iframe src="https://starfyi.com/iframe/glossary/stellar-nucleosynthesis/" width="420" height="400" frameborder="0" style="border:0;border-radius:10px;max-width:100%" loading="lazy"></iframe>
Paste this URL in WordPress, Medium, or any oEmbed-compatible platform.
https://starfyi.com/glossary/stellar-nucleosynthesis/
Add a dynamic SVG badge to your README or docs.
[](https://starfyi.com/glossary/stellar-nucleosynthesis/)
Use the native HTML custom element.
Stellar nucleosynthesis is the creation of chemical elements heavier than hydrogen inside stars through successive fusion reactions. Carbon, oxygen, neon, silicon, and iron are progressively built up in the stellar interior, enriching the interstellar medium when the star dies.
Category: Stellar Physics