For Hobbyists & Makers · Nuclear Binding Energy
Nuclear Binding Energy for a cosmic-ray count
Built for hobbyists & makers exploring it for fun. Play with real physics and math, no license and no setup — just open and tinker. Simulate a cosmic-ray count live below — adjust the inputs and watch it respond, right in your browser.
Nuclear Binding EnergyLive
why stars shine and bombs work
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The binding energy per nucleon measures how tightly a nucleus is held together, peaking at iron-56. Light nuclei release energy by fusing toward that peak — the power source of stars; heavy nuclei release energy by splitting toward it — the basis of fission reactors and bombs. Iron is the ash where both paths end.
Data Inspector
BE per nucleon8.72 MeV
Total BE488 MeV
Energy pathfission releases energy
Governing equation
Reading this result: Iron-56 sits at the very peak — the most tightly bound nucleus, where neither fusion nor fission can extract any more energy.
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Frequently asked questions
- Is this good for hobbyists & makers?
- Yes — this version of "Nuclear Binding Energy for a cosmic-ray count" is framed for hobbyists & makers exploring it for fun. Play with real physics and math, no license and no setup — just open and tinker.
- Do I need to install anything?
- No. It runs in any modern browser, free, with no account required.