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February 20, 2013

Saturn's kinky rings explained

The first time you see Saturn's rings through a telescope is amazing. It can change your life — literally, as it did for me when I was a wee lad.

The rings are shocking through a big telescope. Even through a small one you can see them clearly, and with a big one you can start to see some details, like the big Cassini Division, a dark gap slicing the main ring system in two.

But there's nothing like being there. The Cassini spacecraft (named after the Italian astronomer Giovanni Cassini, who discovered his eponymous division) has been orbiting Saturn since 2004. A masterwork of engineering, Cassini has returned thousands upon thousands of incredible images, showing amazing details in the rings.

On Dec. 25, 2012, from a distance of 1.1 million kilometers (680,000 miles), it took this phenomenal shot of Saturn's outer rings [see photo].

Saturn is off the frame to the upper left in this picture. Cassini was just over the plane of the rings, looking at them from a shallow angle. The sun is shining down on them, so they look very bright.

The main A ring is to the upper left, and you can see the Keeler gap, a narrow (40 km/25 mile) empty region in the rings, where the ice particles that make up the rings have been swept clear by the gravity of the tiny moon Daphnis.

But the star of this show is the weird F ring (the rings were named in order of discovery, not distance from Saturn). To give you a sense of scale, the division between the A and F rings is about 3,000 km (1,800 miles), roughly the distance from New York City to Denver, Colo.

The ring is narrow, and that's no accident. Orbiting just inside and outside of it are two very small moons named Prometheus and Pandora, and they act as shepherds, constraining the ice particles into that narrow strand. Due to the vagaries of orbital mechanics, most of the particles that stray outward or inward from the ring are gently nudged back into it by the moons' gravity.

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