time-and-space.science/solar

Saturn

The rings are the famous part. The moons are where the questions are. Where it is right now, how big and how heavy, what goes round it, and what is still unexplained.

Saturn on its axis

One turn takes10.6 hours
Axis tilted26.73°
Its year29.5 Earth years
Turns per year24445.6

Turning here at one rotation every 12 seconds, which is 3,168 times real speed. What is not sped up: which way it turns, how far the axis leans, and how its day compares with every other planet's. The rings are the real ring system to scale: the faint C ring from 1.24 Saturn radii, the bright B ring, the Cassini Division as a genuine gap at 1.95, then the A ring with the Encke gap near its outer edge. How far open they look is set by the real 26.7-degree tilt, which is why they close to a line twice every Saturn year. The banding is real and genuinely this faint.

Sun, August 9, 2026

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Distances from the sun are in AU — one AU is the Earth’s average distance, 149,597,870 km — and the angle is where the body sits around its orbit, measured from the March equinox direction.

Saturn by the numbers

Width116,460 km — 9.14× Earth
Mass5.683 × 10^26 kg — 95.2× Earth
Surface gravity10.44 m/s² — 1.07× Earth
Day10.56 hours
Year29.45 Earth years
Distance from the sun9.537 AU on average — 9.02 to 10.05 AU
Sunlight takes79.3 minutes
Axial tilt26.73°
Temperature−140 °C at the cloud tops
Moons274
AtmosphereHydrogen and helium, with ammonia ice hazes that mute everything into shades of butterscotch

The mass is worked out from Saturn’s gravitational parameter and the gravity from that and its radius; the year comes from Kepler’s third law and the width is the same figure the simulator draws with. None of them is typed in beside the picture, so none of them can disagree with it.

The moons of Saturn

Saturn has 274 confirmed moons, of which the 9 below are large enough to be worth drawing. The rest are mostly a few kilometres of captured rubble on distant, tilted orbits. Every distance and period here is real, and they are not independent: each pair has to satisfy Kepler’s third law against Saturn’s mass, which is how this table is checked rather than trusted.

MoonDistanceOrbitWidth
Mimas185,539 km22.6 h396 kmOne crater a third of its own width
Enceladus237,948 km1.37 d504 kmVenting ocean water into space through cracks at its south pole
Tethys294,619 km1.89 d1,062 kmAlmost pure water ice, and lighter than water
Dione377,396 km2.74 d1,123 kmWispy cliffs of fresh ice, hundreds of metres high
Rhea527,108 km4.52 d1,528 kmSaturn’s second largest, and still only two fifths the width of our moon
Titan1,221,870 km15.9 d5,150 kmThick nitrogen air, rain, rivers and seas — of methane
Hyperion1,481,009 km21.3 d270 kmTumbles chaotically: it has no settled day length at all
Iapetus3,560,820 km79.3 d1,469 kmOne hemisphere as dark as coal, the other as bright as snow
Phoebe12,947,780 km550.3 d ↺213 kmGoes round backwards — captured, probably from the Kuiper belt

↺ marks a moon going round backwards. Watch this system move →

The moons of Saturn, one at a time

The table above has every figure — how far out, how long a lap takes, how wide. What follows is what those figures cannot tell you: what each one is actually like, who found it and when, and what is still argued about it.

Mimas

A 396 km ball of ice with a 130 km crater in it — a third of its own diameter.

Across396 km
Distance from Saturn185,539 km
One orbit22.6 hours
FoundWilliam Herschel, 1789

Still unsettled

That wobble means either a global ocean under 20–30 km of ice, or an elongated rocky core. In 2024 the ocean case strengthened sharply — and a young ocean under an old, cratered, unresurfaced crust is hard to explain either way.

Enceladus

500 km across, and it is spraying its ocean into space hard enough to build one of Saturn’s rings out of it.

Across504 km
Distance from Saturn237,948 km
One orbit1.37 days
FoundWilliam Herschel, 1789

Still unsettled

How long has the ocean lasted? Some models make it only tens of millions of years old, which would be an awkward coincidence for us to be watching now.

It has water, heat, and the right chemistry. Nobody has looked for anything living in it, and a plume you can fly through is the easiest sample in the outer solar system.

Tethys

Very nearly pure water ice — its density is a shade under water’s own.

Across1,062 km
Distance from Saturn294,619 km
One orbit1.89 days
FoundGiovanni Cassini, 1684

Dione

The wispy streaks across it turned out not to be wisps at all.

Across1,123 km
Distance from Saturn377,396 km
One orbit2.74 days
FoundGiovanni Cassini, 1684

Rhea

Saturn’s second largest moon, and it has a wisp of an atmosphere made of oxygen.

Across1,528 km
Distance from Saturn527,108 km
One orbit4.52 days
FoundGiovanni Cassini, 1672

Titan

The only moon with a real atmosphere — half again as thick as Earth’s at the surface — and the only other place with standing liquid on it.

Across5,150 km
Distance from Saturn1,221,870 km
One orbit15.9 days
FoundChristiaan Huygens, 1655

Still unsettled

Sunlight destroys atmospheric methane in about 30 million years. Something must be replacing it, and nobody knows what — cryovolcanism is the usual guess and has never been caught happening.

Its chemistry is the most complex prebiotic chemistry we can reach. Whether it goes anywhere at 94 kelvin is open.

Hyperion

It does not have a day. Its rotation is mathematically chaotic — there is no period to quote.

Across270 km
Distance from Saturn1,481,009 km
One orbit21.3 days
FoundBond, Bond and Lassell, independently, 1848

Iapetus

One side is as dark as coal, the other as bright as snow, and it wears a mountain range round its equator.

Across1,469 km
Distance from Saturn3,560,820 km
One orbit79.3 days
FoundGiovanni Cassini, 1671 — who noticed he could only see it on one side of Saturn, and correctly guessed one hemisphere was dark

Still unsettled

Nobody knows what built the equatorial ridge. A collapsed ring of its own, a seam from a re-merged body, and an upwelling have all been proposed and none is settled.

Phoebe

It goes round backwards, which is the giveaway: it did not form here.

Across213 km
Distance from Saturn12,947,780 km
One orbit550.3 days — backwards
FoundW. H. Pickering, 1899 — the first moon anywhere found on a photographic plate rather than by eye

When Earth and Saturn are next closest

Both planets are moving, so the gap between them swings enormously — and the closest approaches are not all equal, because the orbits are ellipses rather than circles. These are the next four, solved from the orbits rather than looked up.

October 4, 20268.434 AU — light takes 70.1 minutes
October 18, 20278.329 AU — light takes 69.3 minutes
October 30, 20288.233 AU — light takes 68.5 minutes
November 13, 20298.151 AU — light takes 67.8 minutes

Click a date to take the simulator there. These are minimum-distance moments, which fall near — but not exactly on — opposition.

Flying to Saturn: when to leave

A rocket cannot point at Saturn and fire. It has to leave Earth on an orbit around the sun whose far side touches Saturn’s orbit — half an ellipse — and it has to leave at the moment when Saturn will have arrived at that far side by the time the ship gets there. That is what a launch window is, and it is why they come round only every 12.5 months.

Next window opensJune 27, 2027
ArrivesFebruary 9, 2033
Flight time2,054 days — 5.6 years
Speed change to leave Earth’s orbit round the sun10.31 km/s
The burn itself, from a low Earth orbit7.30 km/s
Slowing down to stay at Saturn5.72 km/s
The window after thatJuly 11, 2028

Set Launch to: Saturn on the rocket launches page to see the ellipse, where Saturn is on launch day, and where it will be on arrival. Click the date to fly it.

What the flight path is, and is not

It is a minimum-energy transfer: the cheapest possible path, half an ellipse with Earth’s orbit at one end and the target’s at the other, solved against where the planets really are — so the arrival lands on the planet’s real distance from the sun and its real position on the day it gets there, not on a circle standing in for its orbit.

It is not a mission plan, and three things are left out on purpose. The orbits are treated as flat, so the real inclinations — Mars is tilted 1.85°, Jupiter 1.3° — cost a plane change this ignores. Real missions trade fuel for a faster arrival, so they leave within days or weeks of these dates rather than exactly on them. And anything going past Jupiter usually steals speed from a planet on the way instead of buying it with fuel, which changes both the date and the path.

What it gets right is the thing worth teaching: why the window exists, why it comes round on the cadence it does, and why the cost of the trip is set by where two planets happen to be rather than by how far apart they are.

Saturn: things worth knowing

What we still don’t know about Saturn

Every one of these is genuinely unsettled — not simplified for the page, not waiting on a textbook update.

How old are the rings?

Cassini measured their mass and found it small, and their ice remarkably clean of the dust that constantly rains in — both of which suggest something that formed in the last 100 million years, long after the planet. Recent work argues that ring particles may shed pollution and stay looking young indefinitely, which would allow rings as old as Saturn. It is one of the sharpest open disagreements in planetary science, and it decides whether we are watching something rare and temporary or something permanent.

Where does Titan's methane come from?

Sunlight destroys atmospheric methane in around 30 million years, and Titan's has not run out. Something is resupplying it — cryovolcanism, or release from clathrates in the crust — and neither has been observed happening. Dragonfly, a nuclear-powered rotorcraft due to launch in 2028 and arrive in 2034, is designed to go looking.

Is Enceladus's ocean inhabited?

It has liquid water, a rocky seafloor, chemical energy, and — from a 2023 reanalysis of Cassini data — phosphates, the last of the elements considered essential for life as we know it. That is a complete list of ingredients and no evidence whatever of the thing itself. No mission is currently funded to go back.

What makes the hexagon?

A six-sided jet stream, 30,000 km across, has sat over Saturn's north pole for at least as long as we have been able to see it. Laboratory tanks of spinning fluid do produce polygons, so it is not magic — but why six, why so stable, and how deep it goes are not answered.

Recently learned about Saturn

March 2025128 new moons were confirmed in one announcement, taking Saturn's total to 274 — more than every other planet in the solar system combined.
2023JWST caught the Enceladus plume extending about 9,600 km, twenty times the width of the moon producing it, feeding a torus of water around Saturn. Cassini data reanalysed the same year showed phosphates in the plume material.

Findings reviewed August 2026. Space science moves; a date on a finding is part of the finding.

The rest of the system

Inward: Jupiter. Outward: Uranus. Or go back to the whole system, where every planet is on screen at once.

Make a link to a particular view

The date, the zoom, the span, the speed, the layers and any flight path are all in the address bar, so copying the URL shares exactly what is on screen. Set it up above, then take the link — it is the quickest way to hand a class one specific thing to look at.

The other simulator

This one is about the whole system. If the question is where the sun and the moon are from where you are standing — what time the sun comes up, why tonight's moon is the shape it is — that is the Sun, Earth & Moon movement simulator, which has a page for every city and a slider over a day, a week or a month.

Also: the classroom guide · sunrise & sunset by city · moon phase & moonrise · lunar eclipses · how the positions are worked out

Saturn: questions without settled answers

How old are the rings? Cassini measured their mass and found it small, and their ice remarkably clean of the dust that constantly rains in — both of which suggest something that formed in the last 100 million years, long after the planet. Recent work argues that ring particles may shed pollution and stay looking young indefinitely, which would allow rings as old as Saturn. It is one of the sharpest open disagreements in planetary science, and it decides whether we are watching something rare and temporary or something permanent.

Where does Titan's methane come from? Sunlight destroys atmospheric methane in around 30 million years, and Titan's has not run out. Something is resupplying it — cryovolcanism, or release from clathrates in the crust — and neither has been observed happening. Dragonfly, a nuclear-powered rotorcraft due to launch in 2028 and arrive in 2034, is designed to go looking.

Is Enceladus's ocean inhabited? It has liquid water, a rocky seafloor, chemical energy, and — from a 2023 reanalysis of Cassini data — phosphates, the last of the elements considered essential for life as we know it. That is a complete list of ingredients and no evidence whatever of the thing itself. No mission is currently funded to go back.

What makes the hexagon? A six-sided jet stream, 30,000 km across, has sat over Saturn's north pole for at least as long as we have been able to see it. Laboratory tanks of spinning fluid do produce polygons, so it is not magic — but why six, why so stable, and how deep it goes are not answered.

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