Saturn is one of a few planets in our solar system surrounded by rings.
Curious Kids is a series for children in which we ask experts to answer questions from kids.
Why do Uranus and other planets have rings around them? (Lesedi, 6, Soweto, South Africa)
For a very long time, Saturn was thought to be the only planet in our solar system with rings. The rings around Saturn were discovered by an astronomer called Galileo Galilei nearly 400 years ago. He used a very simple telescope that he constructed himself from lenses and pointed it at the planets in the night sky.
One of the first objects he looked at was Saturn. At first he thought that Saturn had two large moons on either side of the planet because his telescope wasn’t very good and only produced very blurry images.
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Since then, astronomers – who study the universe and everything in it, like planets – have used bigger and better telescopes to find rings around all of the outer gas giant planets: Jupiter, Saturn, Neptune and Uranus. These planets, unlike others in our system, consist largely of gas.
We’re not sure how the rings work or how they formed, but there are a few theories.
Different theories
The first theory states that the rings formed at the same time as the planet. Some particles of gas and dust that the planets are made of were too far away from the core of the planet and could not be squashed together by gravity. They remained behind to form the ring system.
The second theory is that the rings were formed when two of the moons of the planet, which had formed at the same time as the planet, somehow got disturbed in their orbits and eventually crashed into each other (an orbit is the circular path that the moon travels on around the planet). The stuff that was left behind in this huge smash could not come together again to form a new moon. Instead, it spread out into the ring systems we see today.
Since we don’t have the answers yet, we keep exploring and testing different theories.
What we do know is that the rings around the various planets are all slightly different from one another, but they all share some characteristics too.
First, they are all much wider than they are thick. The rings of Saturn, for example, are about 280,000 kilometers (173,983 miles) wide, stretching away from the planet, but only 200 meters thick. That’s like having a normal pancake on your plate for breakfast that is 14 kilometers wide (8.6 miles).
The other thing that all ring systems share is that they are all made of small particles of ice and rock. The smallest of these particles are no bigger than dust grains, while the largest of the particles are about 20 meters in diameter – about the size of a school hall. All the rings around the planets also contain gaps that are sometimes many kilometers wide, and at first nobody could figure out why. We later learned that the gaps were caused by small moons that had gobbled up all the material in that particular part of the ring system.
The biggest difference between the rings of Saturn and the other gas giant planets is that the particles that make up the rings of Saturn are very good at reflecting the light from the sun back toward the Earth. That means they appear to be very bright, which is why we can see the rings from Earth using a normal telescope. The extremely large number of particles trapped in the rings of Saturn also make the rings much bigger and wider; that’s another reason they’re easier to see than the rings of the other gas giant planets.
The particles that make up the rings of Uranus and Neptune contain elements that were darkened by the sun. These dark particles look very similar to pieces of coal or charcoal like you’d use to make a fire. This makes them much more difficult to see because they don’t reflect as much of the sun’s light back to us.
New discoveries
This is an exciting time for astronomy. More and more satellites and space probes are being launched from all over the world, which allows us to investigate the outer planets of our solar system. That means astronomers will have the chance to study these rings – and one day, hopefully, we’ll be able to answer all of your questions and more.
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A look at Cassini spacecraft's photos of Saturn
A look back at Cassini spacecraft's amazing photos of Saturn, rings, moons
Space Cassini Saturn Photo Gallery
This Jan. 16, 2017 image made available by NASA shows one of Saturn's moons, Daphnis, as it grazes the outer edges of the planet's rings. The 5-mile (8 kilometer) moon orbits within the 42-kilometer (26-mile) wide Keeler Gap. The little moon's gravity raises waves in the edges of the gap in both the horizontal and vertical directions. (NASA/JPL-Caltech/Space Science Institute via AP)
Space Cassini Saturn Photo Gallery
This Jan. 28, 2016 image made available by NASA shows Saturn's rings, including the darker series of bands called the Cassini Division between the bright B ring, left, and dimmer A ring, right. It is almost as wide as the planet Mercury. The 2,980-mile-wide (4,800-kilometer-wide) division in Saturn's rings is thought to be caused by the moon Mimas. (NASA/JPL-Caltech/Space Science Institute via AP)
Space Cassini Saturn Photo Gallery
This Feb. 15, 2016 image made available by NASA shows cracks in Enceladus' icy shell caused by tectonic stresses, as seen from the Cassini spacecraft. Such features are also believed to be relatively young based on their lack of impact craters - a reminder of how geologically active the Saturninan moon is. (NASA/JPL-Caltech/Space Science Institute via AP)
Space Cassini Saturn Photo Gallery
This May 21, 2016 image made available by NASA shows the shadow of Saturn on its rings. The changing length of the shadow marks the passing of the seasons on Saturn. The moon Mimas is a few pixels wide, near the lower left in this image. (NASA/JPL-Caltech/Space Science Institute via AP)
Space Cassini Saturn Photo Gallery
This 2007 image made available by NASA shows a hydrocarbon sea named Ligeia Mare on Saturn's moon Titan, as seen by the Cassini spacecraft. Slight changes observed over several passes indicates that Titan's seas are not stagnant, but rather, dynamic environments. Ligeia is Titan's second-largest liquid hydrocarbon sea, and has a total area of about 50,000 square miles (130,000 square kilometers), making it 50 percent larger than Lake Superior on Earth. (NASA/JPL-Caltech/ASI/Cornell via AP)
Space Cassini Saturn Photo Gallery
This Dec. 3, 2015 image made available by NASA shows three of Saturn's moons - Tethys, above, Enceladus, second left, and Mimas, seen from the Cassini spacecraft. (NASA/JPL-Caltech/Space Science Institute via AP)
Space Cassini Saturn Photo Gallery
This Jan. 10, 2012 image made available by NASA shows Saturn and one of its moons, Tethys, as seen from the Cassini spacecraft. (NASA/JPL-Caltech/Space Science Institute via AP)
Space Cassini Saturn Photo Gallery
This Aug. 12, 2009 composite image made available by NASA shows Saturn in equinox seen by the approaching Cassini spacecraft. Saturn's equinox occurs only once in about 15 Earth years. (NASA/JPL/Space Science Institute via AP)
Space Cassini Saturn Photo Gallery
This July 19, 2013 image made available by NASA shows Saturn's rings and planet Earth, center right, as seen from the Cassini spacecraft. (NASA/JPL-Caltech/Space Science Institute via AP)
Space Cassini Saturn Photo Gallery
This May 4, 2014 image made available by NASA shows the persistent hexagonal cloud pattern on Saturn's north pole, as seen from the Cassini spacecraft. The hexagon is similar to Earth's polar vortex, which has winds blowing in a circular pattern around the polar region, and is nearly 25,000 kilometers (15,000 miles) across. Nearly four Earths could fit inside it. (NASA/JPL-Caltech/Space Science Institute via AP)
Space Cassini Saturn Photo Gallery
This May 21, 2015 image made available by NASA shows Saturn's moon Dione crossing the face of the gas giant, in a phenomenon astronomers call a transit. Transits play an important role in astronomy and can be used to study the orbits of planets and their atmospheres, both in our solar system and in others. (NASA/JPL-Caltech/Space Science Institute via AP)
Space Cassini Saturn Photo Gallery
This Aug. 14, 2014 image made available by NASA shows shadows of Saturn's rings projected on the southern hemisphere of the gas giant. The moon, Tethys, is at lower right, and Mimas, is seen as a slight crescent against Saturn's disk above the rings, at about 4 o'clock. (NASA/JPL-Caltech/Space Science Institute via AP)
Space Cassini Saturn Photo Gallery
This Aug. 23, 2014 image made available by NASA shows the fluid dynamics in Saturn's uppermost cloud layers. (NASA/JPL-Caltech/Space Science Institute via AP)
Space Cassini Saturn Photo Gallery
This Sept. 24, 2015 image made available by NASA shows the moons Enceladus, foreground, and Tethys temporarily aligned off the plane of Saturn's rings, as seen from the Cassini spacecraft. (NASA/JPL-Caltech/Space Science Institute via AP)
Space Cassini Saturn Photo Gallery
This Aug. 17, 2015 image made available by NASA shows the rough and icy crescent of Saturn's moon Dione as seen by the Cassini spacecraft. (NASA/JPL-Caltech/Space Science Institute via AP)
Space Cassini Saturn Photo Gallery
This Nov. 13, 2015 composite image made available by NASA shows an infrared view of Saturn's moon, Titan, as seen by the Cassini spacecraft. The near-infrared wavelengths in this image allow the cameras to penetrate the haze and reveal the moon's surface. (NASA/JPL/ESA/Italian Space Agency via AP)
Space Cassini Saturn Photo Gallery
This Feb. 10, 2015 image made available by NASA shows the slightly irregular horizon of the Saturnian moon, Rhea. The surface of Rhea (949 miles or 1527 kilometers across) has been sculpted largely by impact cratering. On more geologically active worlds like Earth, the craters would be erased by erosion, volcanoes or tectonics. (NASA/JPL-Caltech/Space Science Institute via AP)
Space Cassini Saturn Photo Gallery
This March 25, 2015 image made available by NASA shows the crescents of three of Saturn's moons - Titan, right; Mimas, bottom, and Rhea, left. Titan appears fuzzy because of its cloud layers. Rhea's cratered surface shows a rough texture. (NASA/JPL-Caltech/Space Science Institute via AP)
Space Cassini Saturn Photo Gallery
This Aug. 11, 2013 image made available by NASA shows Saturn and one if its moons, Titan, seen from the Cassini spacecraft. Titan's crescent nearly encircles its disk due to the small haze particles high in its atmosphere scattering the incoming light of the distant Sun. (NASA/JPL-Caltech/Space Science Institute via AP)
Space Cassini Saturn Photo Gallery
This Feb. 17, 2005 image made available by NASA shows plumes of water ice and vapor from the south polar region of Saturn's moon Enceladus. The activity is understood to originate from the moon's subsurface ocean of salty liquid water, which is venting into space. (NASA/JPL/Space Science Institute via AP)
Space Cassini Saturn Photo Gallery
This April 26, 2017 photo made available by NASA shows turbulent clouds at Saturn's north pole, as seen from the Cassini spacecraft. (NASA/JPL-Caltech/Space Science Institute via AP)

