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Kapan memakai 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.


Angka utama nukleosintesis bintang

Angka utama nukleosintesis bintang dalam satu panel: Stellar Nucleosynthesis 3D Explorer membandingkan rantai pp 26.7 MeV, CNO 25.0 MeV, pembakaran silikon di atas 3 miliar K, dan endpoint besi-56.

Compare angka utama nukleosintesis bintang: rantai pp, siklus CNO, pembakaran silikon, dan titik akhir besi.
Nukleosintesis: rantai pp, siklus CNO, pembakaran silikon, dan titik akhir besi.
KuantitasNilai
Pembakaran hidrogen (rantai pp)26,7 MeV per inti helium
Pembakaran hidrogen (siklus CNO)25,0 MeV per inti helium
Suhu pembakaran silikondi atas 3 miliar K
Titik akhir fusibesi-56 (energi ikat puncak)

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