Start with mechanics
Projectile motion, orbital mechanics, and collisions build intuition for forces and energy — and they're visually immediate in the particle studio.
Move to fields and flow
The heat equation and a 2D fluid solver introduce PDEs and the idea of a field evolving in space and time.
Finish with dynamics and math
Lorenz chaos, the SIR epidemic model, and a symbolic-calculus session tie together nonlinear dynamics and the math underneath every simulation.