Orbital distribution of 616 possible meteorite falls detected by GFO, FRIPON, or EFN sensors (blue) versus KDE estimated PDF (red) using a Gaussian kernel with a bandwidth of 0.15 and ensuring any sample crossed the torus traced out by the Earth’s orbit. The meteorite falls were identified using α − β parameters as described in Sansom et al. (2019) using a minimum end mass of 1 g. This PDF, approximating the corresponding sporadic population, was used to estimate the degree of random association in the population via Monte Carlo simulations.