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Saturn's north pole has a six-sided jet stream wider than Earth
A hexagonal pattern in Saturn's atmosphere spans about 30,000 km and has persisted for decades, yet no solid surface shapes it. The corners contain rotating vortices, and the jet stream's speed drops at the vertices.
Saturn's north polar region is ringed by a jet stream shaped like a hexagon — a pattern that stunned scientists when the Voyager spacecraft first photographed it in the early 1980s. The six-sided flow is a wind current in the atmosphere, not a feature on any solid ground, since Saturn has no surface to carve it. Each of the six corners hosts a swirling vortex, and the winds slow where the flow bends at those vertices. [1][2]
A storm that kept its shape
The hexagon is a meandering jet stream — a fast band of eastward wind whose path forms a stable six-sided wave. Because the pattern sits in the atmosphere rather than on terrain, its persistence puzzled researchers: it survived for decades between Voyager's flybys and Cassini's arrival, and has continued since. [1][3]
Cassini gave the first close, long-term view. After arriving in 2004, the spacecraft observed the north pole in detail from 2006 onward, tracking the hexagon's rotation and the vortices at its corners. Cassini's infrared and visible-light instruments showed the hexagon rotating with the planet and revealed a large cyclone at the center of the polar region. [1][2]
Why the corners spin
- At each of the six vertices, the jet stream curls into a compact vortex, creating a ring of small cyclones around the pole. [2]
- The wind speed drops at the vertices and rises along the straight edges, a signature of the meandering flow rather than a rigid shape. [1]
- Laboratory rotating-tank experiments and computer models reproduce polygonal jets, suggesting the pattern emerges from fluid dynamics in a rotating atmosphere. [3]
Not unique, but the biggest
Polygonal jet streams are not exclusive to Saturn. Earth's polar stratospheric vortex can take on wavy, sometimes triangular shapes, and laboratory experiments have produced hexagons and other polygons in rotating fluids. Saturn's stands out for its scale and longevity, making it a natural laboratory for studying how planetary atmospheres organize themselves. [3]
- 1980–1981
Voyager 1 and 2 fly past Saturn and photograph the hexagonal jet stream at the north pole.
- 2004
Cassini arrives at Saturn, beginning a 13-year mission.
- 2006
Cassini begins detailed observations of the north polar hexagon and its central cyclone.
- 2017
Cassini's Grand Finale ends the mission, but the hexagon remains a target for future study.
Sources
- Saturn's Hexagon in Motion NASA
- Cassini: Saturn's Hexagon NASA Science
- The Hexagon of Saturn European Space Agency