Jupiter-family comets are a group of comets with relatively short orbital periods, typically less than 20 years, that originate from the Kuiper Belt and are influenced by the gravitational pull of Jupiter. These comets often have low inclinations and their orbits are more circular compared to long-period comets. Their proximity to Jupiter allows them to be nudged into orbits that bring them closer to the Sun, leading to observable outbursts as they approach perihelion.
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