PPolySim OS
Use case · powered by Roche Limit

Roche Limit for a star's life

Simulate a star's life live in your browser. This runs the real Roche Limit solver — adjust the inputs, watch it respond instantly, and export the result. No install, no account.

Roche LimitLive

Controls

Presets

Inside the Roche limit, tidal forces from the primary exceed the satellite's own gravity and pull it apart — the origin of planetary rings. The rigid-body limit is d = R·(2·ρ_primary/ρ_sat)^(1/3). Drag the moon inside the red ring to shred it.

▶ Run in Python

Data Inspector

Roche limit1.26 R
Orbit2.5 R
Statusstable

Governing equation

Reading this result: Outside the Roche limit: at 2.5 R the moon has a 98% margin above the 1.26 R threshold, so its own gravity holds it together.

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

or unlock everything with Pro →

About this simulation

The full Roche Limit tool models a star's life 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 Roche Limit

Other ways to simulate a star's life

Frequently asked questions

How do I simulate a star's life?
Open this page and use the live Roche Limit 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 star's life from your own measurements.