A planet’s spin describes how quickly it rotates around its axis. Although a planet’s rotation can change over long periods, scientists would expect it to remain nearly constant over the few years of observation.
Measurements from NASA’s Cassini spacecraft once seemed to show that Saturn’s spin was changing, but the planet itself wasn’t speeding up or slowing down.
The apparent change came from Saturn’s aurora: winds in the upper atmosphere create electrical currents that affect the auroral signal scientists use to measure the planet’s rotation.
New observations from the James Webb Space Telescope help explain what drives those winds: the aurora heats Saturn’s atmosphere in specific places, and that uneven heating drives winds.
The winds then produce currents that power the aurora, which heats the atmosphere again. This self-sustaining cycle affects the signal, making Saturn’s spin appear to change.
Read More
Find all the latest news on Saturns's moons, including Titan, the most Earth-like world in the Solar System, here.
Latest News About Saturn
Hubble observes mysterious spokes in Saturn's rings
September 4, 2026
The mystery of the features seen in Saturn's icy rings deepens.
Read more
NASA’s Hubble tracks new decagon encircling Saturn’s south pole
September 2, 2026
This discovery marks the first time a large, regular-sided jet pattern has been observed in the planet's southern hemisphere.
Read more
Saturn’s changing “rotation rate” was never caused by the planet speeding up or slowing down, but by powerful winds high in its atmosphere.
Read more
Saturn's magnetic field is curiously warped, and one of its moons may be to blame
April 1, 2026
"A better understanding of Saturn’s environment is especially urgent now as plans for our return to Saturn and its moon Enceladus start to be developed."
Read more
Are Saturn's rings made of a lost, shattered moon?
If the sun were as tall as a typical front door, the Earth would be the size of a nickel and Saturn would be about as big as a volleyball.
From Saturn’s surface, the Sun appears about one-tenth as large as it does from Earth and sunlight appears about 90 times dimmer.
Saturn is twice as far away from the Sun as the Jupiter is, and the farthest planet that can be seen with the naked eye from Earth.
Saturn is the least dense planet in the solar system because it is mostly made of gas; it is the only planet less dense than water!
Saturn emits about 2.3 times the energy it receives from the Sun. This energy is thought to come from the continued cooling of the planet after its gravitational collapse during the formation of the solar system. Because of this, the weather on the planet is internally driven: it depends on the energy emitted by the planet itself. On the other hand, the weather on Earth is externally driven, by the sun!
Saturn has some of fastest winds in the solar system; winds have been measured up to the speed of 1800 kilometers per hour.
The planet’s rings are made up of bits of ice, dust and rock; these can range from the size of a grain of sand up to sizes larger large buildings. The rings also contain moonlets (likely chunks of the ancient body that broke up to produce Saturn’s rings) and ‘propeller’ structures (gaps in ring material thought to be caused by the moonlets). The evidence for moonlets and ‘propeller’ structures suggests there is a dynamic between Saturn’s moons and rings.
The planet has been observed to have hexagonal, and even decagonal jet streams at its north and south poles.