PPolySim OS
For Educators · Star Lifecycle

Star Lifecycle for a species migration

Built for educators teaching it to a class. Drop a live demo into a lecture or assign it as a shareable link — no lab installs. Simulate a species migration live below — adjust the inputs and watch it respond, right in your browser.

Hertzsprung-Russell DiagramLive

Controls

Presets

The H-R diagram plots stars by temperature and luminosity, revealing the main sequence (a diagonal band), red giants, supergiants, and white dwarfs. Your star (pink ring) sits on the main sequence where luminosity scales as T⁴.

▶ Run in Python

Data Inspector

Spectral classG
Luminosity1.00 L☉
Temperature5,778 K

Governing equation

Reading this result: A cool orange K-type star: lower temperature places it low-right on the main sequence, dimmer and longer-lived than the Sun.

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

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.

or unlock everything with Pro →

More with Star Lifecycle

Frequently asked questions

Is this good for educators?
Yes — this version of "Star Lifecycle for a species migration" is framed for educators teaching it to a class. Drop a live demo into a lecture or assign it as a shareable link — no lab installs.
Do I need to install anything?
No. It runs in any modern browser, free, with no account required.