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Quando 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.


Numeros principais da nucleossintese estelar

Numeros principais da nucleossintese estelar em um painel: Stellar Nucleosynthesis 3D Explorer compara a cadeia pp 26.7 MeV, CNO 25.0 MeV, queima de silicio acima de 3 bilhoes K e o endpoint ferro-56.

Compare os numeros principais da nucleossintese estelar: a cadeia pp, o ciclo CNO, a combustao de silicio e o ponto final de ferro.
Nucleossintese: cadeia pp, ciclo CNO, combustao de silicio e ponto final de ferro.
QuantidadeValor
Combustao de hidrogenio (cadeia pp)26,7 MeV por nucleo de helio
Combustao de hidrogenio (ciclo CNO)25,0 MeV por nucleo de helio
Temperatura de combustao de silicioacima de 3 bilhoes de K
Ponto final de fusaoferro-56 (energia de ligacao maxima)

Walk the controls in the step-by-step guide, or compare options in vs alternatives. Open the Stellar Nucleosynthesis 3D Explorer.

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