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Cuando usar Stellar Nucleosynthesis 3D Explorer
Use this cutaway when you want to see where the elements are forged inside a massive star - and skip it when you want a star evolution over time or the Sun energy-transport layers.
- Classroom demos of the onion-shell fusion structure and the iron peak
- Connecting each burning stage to a temperature and a reaction
- Explaining why stars make elements only up to iron
This is an educational cutaway with illustrative shell sizes, not a stellar-interior simulation.
Cifras clave de la nucleosintesis estelar
Cifras clave de la nucleosintesis estelar en un panel: Stellar Nucleosynthesis 3D Explorer compara la cadena pp 26.7 MeV, CNO 25.0 MeV, quema de silicio sobre 3 mil millones K y el endpoint hierro-56.
| Cantidad | Valor |
|---|---|
| Combustion de hidrogeno (cadena pp) | 26.7 MeV por nucleo de helio |
| Combustion de hidrogeno (ciclo CNO) | 25.0 MeV por nucleo de helio |
| Temperatura de combustion de silicio | mas de 3 mil millones de K |
| Punto final de fusion | hierro-56 (energia de enlace maxima) |
Walk the controls in the step-by-step guide, or compare options in vs alternatives. Open the Stellar Nucleosynthesis 3D Explorer.