🔭 Exoplanet Transit: Limb Darkening, Light-Curve Fit and Detection Limit

Watch a planet cross its star, build the folded light curve point by point, fit the planet radius and see how limb darkening, impact parameter and photometric noise decide whether a transit can be detected.

3D · Three.js / WebGL renderer · 60 FPS target · runs fully client-side, no install