From Rock Tumbling to Telescope Mirror Grinding: How Optical Perfection Emerges from Random Motion

Abstract

When two glass disks are rubbed together by hand with an abrasive between them, their surfaces spontaneously converge to perfectly matching spherical curves, accurate to tens of nanometers. How does such optical precision emerge from an essentially random manual process? Starting from Preston's law of material removal, we derive a first-principles explanation. Symmetries of the grinding stroke imply that planes and spheres are the generic equilibria of the process. Their stability is governed by a hierarchy of timescales: small-scale irregularities decay exponentially on the grinding timescale $T_\text{grind}$, while large-scale deviations from a sphere diffuse away on the longer spherizing timescale $T_\text{sphere} \propto (R_\text{mirror}/R_\text{stroke})^2\, T_\text{grind}$. Gravity and finite disk size destabilize planar surfaces, but for sufficiently short strokes spheres remain stable ($T_\text{deform} \gg T_\text{sphere}$), with only their radius of curvature varying adiabatically. The same framework unifies telescope mirror grinding with everyday phenomena: rock tumbling (explaining why rotary tumbling rounds edges more than vibratory, and why neither produce spheres) and sanding (explaining why small flat surfaces inevitably round). These examples offer an accessible classroom context for stable and unstable equilibria, exponential relaxation, diffusion, multi-timescale analysis, and the emergence of the Laplacian operator from averaging over a local area.