
Three of Saturn’s moons — Tethys, Enceladus and Mimas — as seen from NASA’s Cassini spacecraft [image credit: NASA/JPL]
Enceladus is in a 2:1 resonance with a moon named Dione, but Tethys – another major moon of Saturn – orbits between them and is in a 1:2 resonance with Mimas, whose orbit lies inside that of Enceladus. So the order of proximity to the planet is Mimas, Enceladus, Tethys, Dione. The study looks at how the Enceladus-Dione part of this unusual set-up could have come into being. Talking of speed, all four moons orbit their very large planet in less than three days (Mimas in less than one day).
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Enceladus, one of Saturn’s moons, is currently being tugged around and heated up by another moon named Dione, says AAS Nova.
How the two ended up in this arrangement is a mystery, since to get there, Enceladus must have avoided getting caught up in a resonance with another moon named Tethys.
A recent article offers a possible explanation: Enceladus may have blitzed over to its current position in a short-lived burst of speed.
Dynamic Moons
We typically imagine that moons circle their host planets with clockwork regularity, meaning that they precisely trace out the same path at the same speed for all time. However, true reality cannot be described by a system composed of rigid gears.





















