Where do most short-period comets originate?

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Most short-period comets originate from the Kuiper belt, a flattened disk of icy bodies located beyond the orbit of Neptune.12

Specifically, the Jupiter-family comets—a subset of short-period comets—are believed to originate from the scattered disk, which consists of Kuiper belt objects that have been perturbed into more eccentric and inclined orbits with perihelia near Neptune. Neptune then gravitationally scatters these objects inward toward the planetary region, where they can be captured into short-period orbits. While the Oort cloud is the primary source for long-period comets, the Kuiper belt is the established source for the majority of observed short-period comets.12