Encke’s gap
Quick Summary
Encke's Gap is a notable feature within Saturn's A ring, located at approximately 2.21 Saturn radii from the planet's center. This gap is a region where fewer particles are present, creating a visible division within the ring system.1
The existence of such gaps, including Encke's Gap, is theorized to be caused by the gravitational influence of small moons orbiting within or near the gap. These moons, sometimes referred to as "shepherd moons," can clear out particles through gravitational perturbations. In the case of Encke's Gap, the moon Pan has been discovered within it, supporting this theory.1
Johann Franz Encke, a German astronomer, is credited with discovering this gap, which now bears his name. His work in astronomy also included establishing the orbital period of Encke's Comet and deriving a value for the solar parallax.2
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