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Saturn's Hexagonal Storm

At Saturn's north pole sits one of the strangest atmospheric structures in the solar system: a persistent storm shaped like a perfect hexagon.

The Phenomenon

This hexagonal cloud storm is a jet stream with turbulent, unstable weather. It raises big questions for scientists: is Saturn just a giant ball of gas?

Saturn Hexagon Storm

Image taken by NASA. By NASA/JPL-Caltech/Space Science Institute [Public domain], via Wikimedia Commons

Key Facts About the Storm

Size: about 13,800 km across — the entire Earth (diameter 12,700 km) would fit inside it.

Duration: it has been active for decades since its discovery, and possibly centuries before that.

Discovery: spotted in the early 1980s by NASA's Voyager 1 and 2 probes.

First video: in 2009 the Cassini mission captured a video of the storm in motion.


Why Does It Last So Long?

On Earth, a storm only lasts a few days. Mountains and solid structures break storms apart and scatter them. So if Saturn's storm never dissolves, does that mean there are no solid structures like mountains? Is Saturn really just a gas giant?

The Vortex in False Color

The Cassini probe photographed the central vortex of the storm using color filters that reveal details of the atmospheric structure invisible to the naked eye.

Saturn Hexagon Storm Vortex in False Color

The hexagonal storm vortex in false color.


The Storm's Rotation

The animated image below was taken by the Cassini probe on November 10, 2006 and shows the rotation of the hexagonal storm at Saturn's north pole.

Saturn Hexagon Storm Rotation

By NASA [Public domain], via Wikimedia Commons

More About the Hexagon

Click on any element to learn more.

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