Kirkwood gaps are regions in the asteroid belt where there is a noticeable scarcity of asteroids, typically occurring at specific distances from the Sun. These gaps arise due to gravitational interactions with nearby planets, particularly through the phenomenon of orbital resonances, where the gravitational forces exerted by a planet can clear out certain orbits by destabilizing the orbits of asteroids. Understanding Kirkwood gaps helps illustrate how planetary dynamics influence the distribution and behavior of celestial objects in our solar system.
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