
Physics / Astronomy
Galaxy (Barnes-Hut N-body)
A spiral galaxy star by star: gravity alone winds up the arms.
Available for Windows
200 interactive modules span mechanics, waves, optics, electromagnetism, quantum phenomena, fluids and thermodynamics. Work with physical objects, inspect detailed 3D apparatus and connect the motion to live measurements.
200 modules · Page 1 / 10

Physics / Astronomy
A spiral galaxy star by star: gravity alone winds up the arms.

Physics / Astronomy
Gravitating many-body systems: from the Solar System to choreographies.


Physics / Astronomy / Engineering
Variable mass and the Tsiolkovsky equation, staging and gravity.


Physics
Normal modes, beats and waves in a chain of 2–8 masses coupled by springs.

Physics
Mass-spring cubes, membranes and chains, plus sixteen exact modes of a fixed square membrane. Strike a point, excite a mode or drive a resonance.





Physics
A heavy ball on a rope from a rotating arm: it lags the arm and swings outward by inertia; cut the motor and the orbit spirals back in.

Physics / Astronomy
Roemer 1676: Io's eclipses arrive late when Earth is far from Jupiter, and the residuals of the fit measure the speed of light.

Physics
A bob swept round a cone: tension leans in, its horizontal part is the centripetal force, and only one spin rate holds the angle steady.

Physics / Earth
Shake a building at its own frequency, then tune a roof damper and watch the sway die.



Physics
White light through a prism: dispersion, rainbow, total internal reflection.


Physics / Astronomy
Ptolemy vs Copernicus: the same planets, two frames. Pin the Earth and epicycles appear by themselves - Mars walks backwards once per synodic period.
Some modules belong to more than one Suite. Shared experiments have one description here.