Iron Rain Column: Stokes Settling & Core Growth (2D)
Interactive 2D side-view sedimentation-column model of planetary core formation: molten iron droplets fall through a silicate magma ocean, their velocity integrated from the real F=ma force balance (gravity, buoyancy, Stokes drag) rather than assumed instantaneous, feeding a growing core layer while live Reynolds-number and relaxation-time diagnostics show exactly when the Stokes approximation holds.
This 2D companion to the 3D planetary-differentiation sim recreates the same molten-iron "rain" as a vertical sedimentation column instead of a full sphere — the standard way settling experiments are actually visualized. Rather than assuming each droplet is already moving at its Stokes terminal velocity, every droplet's velocity is integrated from the real force balance (gravity and buoyancy against viscous drag), using an exact exponential solution because the underlying relaxation is numerically stiff at these droplet sizes. The result converges to the identical terminal-velocity formula the 3D sim uses, but arrives there through genuine dynamics — and the panel surfaces two diagnostics the 3D sim never computes: the relaxation time constant itself, and a live Reynolds number that flags exactly when the slider settings have pushed the system outside Stokes' law's valid regime. Tune grain size, mantle viscosity and gravity to watch the core layer grow from real conservation of settled volume.
A 2D sedimentation-column model of planetary core formation: molten iron droplets fall through a silicate magma ocean with velocity integrated from the real F=ma force balance (gravity, buoyancy, Stokes drag) via an exact exponential relaxation solver, feeding a growing core layer, with live Reynolds-number and relaxation-time diagnostics showing exactly when the Stokes terminal-velocity approximation holds.
2D · HTML5 Canvas 2D · 60 FPS target · runs fully client-side, no install