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Blackbody & Radiation for a bouncing ball

Simulate a bouncing ball live in your browser. This runs the real Blackbody & Radiation solver — adjust the inputs, watch it respond instantly, and export the result. No install, no account.

Blackbody RadiationLive

Controls

Every warm object glows with a Planck spectrum. Heat it up and the peak shifts to shorter (bluer) wavelengths — that's why stars range from red to blue-white.

Presets

▶ Run in Python

Data Inspector

Temperature5778 K
Peak wavelength502 nm
Colorwhite/yellow

Governing equation

Reading this result: At 5778 K the Planck curve peaks at 502 nm, inside the visible band — Wien's law makes peak wavelength ∝ 1/T, so doubling the temperature halves the peak wavelength and shifts the glow toward blue.

Runs locally in your browser — free forever. Scale to the cloud when reality gets heavy.

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About this simulation

The full Blackbody & Radiation tool models a bouncing ball with the same numerics engineers and scientists use — running entirely client-side. Change any parameter and the result updates in real time, so you can build intuition, check a design, or teach the concept without spreadsheets or installs.

More you can do with Blackbody & Radiation

Other ways to simulate a bouncing ball

Frequently asked questions

How do I simulate a bouncing ball?
Open this page and use the live Blackbody & Radiation tool below — set your inputs and the simulation runs instantly in your browser using real numerics. No install, no account needed.
Is it free?
Yes. The simulation runs free in your browser. A one-time unlock or a Pro plan adds advanced parameters, saved presets, data import, and clean exports.
Can I use my own numbers?
Absolutely — every input is adjustable, and with data import you can drive a bouncing ball from your own measurements.