Make the rings vanish
Ring-plane crossing
Hide the rings
Tilt Saturn. At what angle do the rings disappear?
Tilt the ring plane toward edge-on. Why did Galileo lose the "ears" in 1612?
Tilt Saturn. Can you make the rings disappear?
Your turn
Each lab is one step from the video. Change things and see what happens.
Each lab isolates one step. Facts from NASA, ESA, OpenStax and Britannica; the pictures are not to scale.
Tap, drag and slide.
Tilt Saturn. At what angle do the rings disappear?
Tilt the ring plane toward edge-on. Why did Galileo lose the "ears" in 1612?
Tilt Saturn. Can you make the rings disappear?
Zoom in and speed up. Which chunk wins the race, inner or outer?
Compare lap counts in the inner and outer lanes. Why does a ring shear instead of spinning rigidly?
Zoom in. Do the pieces close to Saturn go faster?
Simplified picture: far fewer chunks than real, not to scale.
Shrink the main rings to a model. How thick would it be?
Scale the main rings (≈270,000 km wide, ~10 m thick) to any width. How does the thickness compare with paper?
Make the rings small. Are they still thin?
Uses the main rings (about 270,000 km wide) and a typical 10 m thickness from NASA.
Drag the moon toward Saturn. Where does it come apart?
Drop a moon inside and outside the idealized Roche limit (≈2.44 Saturn radii). What happens to the debris?
Drag the moon close to Saturn. What happens?
A simplified model: real break-up depends on the moon's size, strength and density.
Turn Pan off. How fast does the gap fill in?
Toggle Pan and watch the lane. What keeps a gap sharp-edged?
Turn Pan off, then on. What happens to the lane?
The strip is the A ring "unrolled"; motion is relative to Pan and sped up.
Slide through time. When were the rings bright, and when might they fade?
Scrub one "young rings" scenario from 600 Myr ago to 400 Myr ahead. Which parts are measured, and which are debated?
Slide back and forward. Watch the rings come and go!
One possible history based on the "young rings" idea. The real age is still debated.
Saturn's rings are made of lots and lots of pieces of ice. Scientists think an icy moon came too close to Saturn and broke apart.
Long ago, a man named Galileo looked at Saturn with a telescope. He saw two bumps, like ears! Later the ears were gone. They were really rings, turned sideways.
The rings look like one shiny plate. But up close they are lots of pieces of ice. Some are tiny like sand. Some are as big as a house! Every piece goes around Saturn, like a tiny moon.
The rings are super wide, much wider than Earth. But they are very thin, only about as tall as a house.
Saturn's gravity pulled harder on the near side of an icy moon than on its far side. The moon got stretched, like soft dough, and gently came apart. The pieces spread out into a flat ring.
The rings are slowly falling into Saturn, like a very slow rain. We are lucky to see them shine!
Want more? See how planets are made and why Pluto is not a planet. ← More explainers
Saturn's rings are the leftovers of something that got too close. Scientists think they are pieces of comets, asteroids or shattered moons that broke up before they reached the planet, torn apart by Saturn's powerful gravity.1 The pieces kept crashing into each other, breaking into smaller bits, and spread out into a flat disc around Saturn's middle.11
Close to a giant planet, gravity doesn't just pull. It stretches. Inside a boundary called the Roche limit, that stretch is strong enough to rip a moon apart, and it also stops the loose pieces from ever clumping back into a moon.86 So instead of a moon, Saturn has rings.
From Earth the rings look like one solid, shiny disc. They aren't. They are billions of small chunks of ice and rock coated with other materials such as dust, and almost all of it is water ice.12 That clean ice is why they're so bright: they reflect about 60% of the sunlight that hits them, while the dark rings of Uranus and Neptune reflect only about 5%.6
The pieces come in every size. NASA says the ring particles mostly range from tiny, dust-sized icy grains to chunks as big as a house. A few particles are as large as mountains.1 If you could float inside the rings, OpenStax says it would probably look like a bright cloud of floating snowflakes and hailstones, with a few snowballs and bigger lumps.6
Every chunk is like a tiny moon, following its own orbit around Saturn. The inner ones go around faster than the outer ones, so the rings don't turn like one solid record.61 Back in 1857, James Clerk Maxwell used maths to show the rings could only be stable if they were made of huge numbers of small pieces. A solid ring would be torn apart.8
They're enormous and incredibly thin. In NASA's words, "Saturn's ring system extends up to 175,000 miles (282,000 kilometers) from the planet, yet the vertical height is typically about 30 feet (10 meters) in the main rings."1 Measured edge to edge, the ring system wouldn't fit in the gap between Earth and the Moon, which is 384,400 km on average.315
| Measurement | Value | Source |
|---|---|---|
| How far the ring system reaches from Saturn | up to 282,000 km (175,000 miles) | NASA1 |
| Diameter of the bright main rings | about 270,000 km | Britannica8 |
| Typical thickness of the main rings | about 10 m (30 feet) | NASA12 |
| Thickest parts of the main rings | under about 100 m in most places | NASA/JPL3 |
| Cassini Division (gap between rings A and B) | 4,700 km (2,920 miles) wide | NASA1 |
To feel how thin that is, shrink the main rings to the width of a football field (about 100 m). At the same scale, 10 m of thickness becomes about 0.004 mm, far thinner than a sheet of paper (about 0.1 mm).
100 m × (10 m ÷ 270,000,000 m) ≈ 0.000004 m = 0.004 mm
That thinness explains Galileo's puzzle. When Earth lines up with the plane of the rings, we see them edge-on, and they almost disappear.813 Saturn takes about 30 Earth years to go around the Sun, so this happens about every 15 years.2
Gravity gets weaker with distance. So when a moon orbits close to Saturn, Saturn pulls harder on the moon's near side than on its far side. That difference is a tidal force, and it stretches the moon. It's the same kind of stretch the Moon puts on Earth's oceans to make tides.8
Far from the planet, a moon's own gravity easily holds it together. But closer in there is a line called the Roche limit: the closest a fairly large moon can get before tidal forces tear it apart. For Saturn it's about 2.44 times Saturn's radius, roughly 147,000 km from the planet's centre. Saturn's main rings lie inside it.8
Scientists aren't sure which object was destroyed. It might have been a comet, or an icy moon.85 OpenStax also describes a second idea: some rings may be material that never managed to clump into a moon in the first place. In both ideas, the planet's tidal forces do the key job.6 Small, solid moons a few tens of kilometres across can survive inside the Roche limit, because their rock and ice hold them together, not just gravity.8
The rings are named with letters in the order they were discovered. Going outward from Saturn, NASA lists the D ring, C ring, B ring, Cassini Division, A ring, F ring, G ring, and finally, the E ring, plus the very faint Phoebe ring much farther out.1 The main rings are A, B and C. The B ring is the brightest and most tightly packed.6
Up close, each main ring splits into many narrower ringlets. NASA Space Place says there may be 500 to 1,000 of them.12 The E ring is different: much of its material comes from water jets on the moon Enceladus.2
Some gaps and sharp edges are carved by small moons. The little moon Pan orbits inside the Encke Gap in the A ring, which is about 325 km (200 miles) wide. Ring particles closer to Saturn move faster than Pan and pass it, and each time they get a gravitational "kick" from Pan. That keeps the gap open and sends waves through the ring.4 Moons that shape rings like this are called shepherd moons. The narrow F ring is shepherded by two tiny moons, Pandora and Prometheus.3
This is where scientists still disagree. Saturn itself is about 4.5 billion years old.9 For a long time people assumed the rings were just as old.10
Then came the dust test. Tiny grains of space dust keep falling on the rings, slowly darkening the ice. It works like dust settling on a clean carpet: the cleaner the rings are, the younger they should be. Measurements from the Cassini spacecraft's Cosmic Dust Analyzer led one team to say the rings are no more than 400 million years old.9 NASA describes the main rings as "perhaps only a few hundred million years old".3
Not everyone agrees. Some scientists argue that rings can look young without being young, for example if something cleans the ice or the dust rate has changed. So the age is still being debated.10
Yes, slowly. Ice from the rings is pulled into Saturn as a dusty "ring rain". NASA researchers estimate the rain alone drains enough water to fill an Olympic swimming pool in half an hour. At that rate the rings would be gone in 300 million years. Add the ring material Cassini saw falling into Saturn's equator, and they may have less than 100 million years left.5 If that's right, we're lucky to be around while Saturn wears them.
Don't confuse this with the rings "disappearing" from view. That happens about every 15 years when the rings turn edge-on to Earth, and they come back.13
No. All four giant planets have rings.6 Jupiter's are faint and made of small, dark particles, probably dust knocked off its small inner moons.14 Uranus and Neptune have narrow, dark rings with wide empty gaps between them.6 Only Saturn's are big, bright and icy.
Galileo saw them first, in 1610, through one of the first telescopes. He didn't know what they were. To him they looked like "ears" on either side of the planet.7 Two years later the ears were gone, because Earth had crossed the ring plane.8 In 1655 Christiaan Huygens worked out that Saturn is surrounded by a ring, though he thought it was solid.7 In 1675 Gian Domenico Cassini spotted the big gap now called the Cassini Division.6 Four spacecraft have visited: Pioneer 11, Voyager 1, Voyager 2 and Cassini, which orbited Saturn for 13 years until 2017.12
Keep exploring: see how the planets formed, why Pluto is not a planet, and how gravity works.
Scientists think a moon, comet or other icy body came too close to Saturn. Saturn's gravity pulled harder on its near side than its far side and tore it apart. The pieces spread out into a flat disc of ice chunks circling the planet: the rings.
Bright rings need lots of ice that comes close enough to a planet for its gravity to rip it apart. Every planet has such a danger zone, called the Roche limit. Scientists think an icy moon, comet or similar body strayed inside Saturn's Roche limit and was torn to pieces. Saturn is a gas giant about 9 times wider than Earth. Earth has no icy body orbiting close enough to be torn apart, so it has no rings today.
Almost entirely water ice, with some rock and dust mixed in. NASA says the pieces range from tiny dust-sized grains to chunks as big as a house, and a few are as large as mountains.
There are seven main named rings: D, C, B, A, F, G and E (from the planet outward), plus the faint Phoebe ring. Up close, each main ring is made of many narrower ringlets. NASA Space Place says there may be 500 to 1,000 of them.
Yes, slowly. Ice from the rings rains down into Saturn. NASA researchers estimate the rings could be mostly gone in a few hundred million years, or even less than 100 million. From Earth the rings also seem to vanish for a while about every 15 years, but that's only because they turn edge-on to us.
Saturn. Its seven main rings are made of hundreds of narrower ringlets. NASA Space Place puts the number at maybe 500 to 1,000.
Yes. All four giant planets have rings. Jupiter's are faint and made of dark dust, and Uranus and Neptune have narrow, dark rings. Only Saturn's are big, bright and icy enough to see easily with a small telescope.