The crown jewel of our solar system has rings, moons, and much more to explore
At a glance
Saturn is the second-largest planet, boasting a stunning set of rings that can be seen in backyard telescopes. By studying Saturn and comparing it to similar exoplanets, we learn how solar systems evolve.
Its complex, planet-like moons make Saturn a solar system unto itself. Titan can help us learn the possible starting ingredients for life on Earth and elsewhere, while Enceladus has a subsurface ocean that could contain life.
You can support Saturn exploration by sharing stunning pictures from our image library, cheering on NASA’s upcoming Dragonfly mission to Titan, and learning how to be a space advocate for future outer planets missions.
Why study Saturn?
The real Lord of the Rings is Saturn, a massive outer planet boasting a set of rings about 27 Earths wide. Being a gas giant like Jupiter, Saturn shares many of its attributes: a strong magnetic field generated by churning metallic hydrogen deep inside, raging storms in its gaseous upper atmosphere, and a diversity of planet-like moons that are worlds unto themselves. Saturn’s rings and larger moons are visible even from small backyard telescopes.
Saturn was born right after Jupiter, roughly 4.5 billion years ago in the solar system’s early days. Both planets probably formed closer to the Sun and then migrated out to their current positions about 4 billion years ago. Their gravity likely lofted asteroids and comets all over the solar system, some of which slammed into early Earth and may have brought water here.
We know of more than 4,000 exoplanets—worlds orbiting other stars—and the statistics show us that most stars have planets. Many are Jupiter and Saturn-like words close to their stars, supporting the idea that our own gas giants moved during the solar system’s early days. One exoplanet we’ve found appears to have rings 200 times wider than Saturn’s! By studying Saturn and comparing it to similar exoplanets, we learn how solar systems evolve.
NASA / JPL-Caltech / SSI / Gordan Ugarkovic
Saturn's rings in color
Cassini took the images for this view across all of Saturn's main rings with its wide-angle camera on 17 April 2009. A shadow of one of the moons (perhaps Mimas?) is being cast on the rings.
What are Saturn's rings like up close?
Saturn’s rings are made from chunks of mostly water ice ranging in size from dust specks to houses to mountains. The largest chunks, known as moonlets, have enough gravity to clear small gaps, distort the rings’ shape, and cause wave-like disturbances.
Where did Saturn's rings come from?
Scientists think Saturn’s rings formed when either a large moon got too close to Saturn and was ripped apart due to intense gravitational forces or that the rings are simply leftover material from the time Saturn formed. The rings are being gradually pulled into Saturn and will disappear completely within 300 million years. We don’t know why the other giant planets Jupiter, Uranus and Neptune don’t have such a stunning set.
Like our other 3 outer planets, Saturn is a solar system unto itself, with many compelling targets for study. The ringed planet has at least 82 moons, the largest of which are active, planet-like worlds.
NASA / JPL-Caltech / Montage by Emily Lakdawalla / Processing by Processing by Ted Stryk, Gordan Ugarkovic, Emily Lakdawalla, and Jason Perry.
Larger than Mercury, Titan has an orange, hazy atmosphere that was probably similar to Earth’s before life arose here around 3.5 billion years ago. Complex, organic molecules—one of the building blocks for life as we know it—form Titan’s atmosphere and rain from the skies. By studying Titan, we can learn the possible starting ingredients for life on Earth and elsewhere.
At just 500 kilometers (310 miles) wide, Enceladus could fit comfortably inside the U.S. state of Arizona. But this moon has a big secret under its icy crust: a saltwater ocean, which leaks into space via geysers on the surface to form one of Saturn’s outer rings. We know the ocean contains complex organic materials. Could it also contain life?
Mimas boasts a massive crater that makes it eerily similar to the Death Star from Star Wars. It too may have a subsurface ocean, though material from the ocean does not appear to leak up to the surface.
The photogenic oddballs
Some of Saturn’s smaller moons are among the most photogenic in our solar system. Dione and Rhea are cratered snowball worlds with rocky cores. Hyperion looks like a giant sponge or coral reef. Iapetus is two-faced, with an icy half and a dark half coated with material coming from the comet-like moon Phoebe. And then there’s Pan, a moon whose gravity has grabbed enough material from Saturn’s rings to make it look like a flying saucer!
NASA / JPL-Caltech / SSI / Kevin M. Gill
Color view of the plumes of Enceladus
A true-color view of Enceladus' southern plumes.
How do we study Saturn?
Christiaan Huygens first glimpsed Saturn’s rings and the planet’s largest moon Titan through a telescope in the 1650s. Shortly thereafter, Giovanni Cassini found 4 more moons and the planet’s largest ring gap, now named the Cassini Division in his honor.
NASA’s Pioneer 11 was the first spacecraft to visit Saturn, flying past the planet in 1979 and revealing yet another outer ring. Voyager 1 flew by a year later, swinging by Titan to get a good look at the moon’s thick orange atmosphere. Voyager 2 flew closer to Saturn itself, discovering the planet’s upper atmosphere was a chilly -200 degrees Celsius (-328 degrees Fareneheit), and finding trace amounts of ammonia crystals that give Saturn its pale yellow hue.
In 2004, Cassini-Huygens, a joint robotic mission by NASA and the European Space Agency, became the first spacecraft to orbit Saturn. One of the most revolutionary space missions of all time, Cassini spent 13 Earth years—almost half a Saturn year—watching how the planet and its moons changed with the seasons as they orbited the Sun.
On Saturn itself, Cassini studied the hexagonal storm at the planet’s north pole first seen by Voyager 2 in 1981, and discovered a smaller, circular vortex on the south pole. The north pole storm is remarkably symmetric and has a central eyewall akin to Earth’s hurricanes. Cassini also observed a planet-wide megastorm that appears roughly every Saturn year—30 Earth years. The spacecraft also mapped the structure and shape of Saturn’s magnetic field and narrowed down the planet’s rotation rate—less than half an Earth day, even though Saturn is 9.5 Earths wide!
Shortly after its arrival at Saturn, Cassini released the European Huygens probe, which landed on Titan’s surface in 2005—a first for any world in the outer solar system. As Huygens descended, it gathered data on the complexchemistry happening in Titan’s atmosphere. Post-landing, the probe took the first ever images from Titan’s surface and survived for 2 hours, despite frigid temperatures of about -180 degrees Celsius (-292 degrees Fahrenheit).
NASA / JPL / ESA / UA
Huygens view of Titan's surface (colorized)
Huygens returned this photo after landing on Titan on January 14, 2005. It has been colorized based upon spectral data. The round objects in this image are pebbles and cobbles composed of ice. The surface is darker than originally expected, consisting of a mixture of water and hydrocarbon ice. There is also evidence of erosion at the base of these objects, indicating possible fluvial activity.
As it performed long, swooping orbits around Saturn, Cassini repeatedly buzzed many of the planet’s moons. The spacecraft’s cloud-penetrating radar pierced Titan’s orange haze, allowing scientists to create a global geologic surface map. Gravity measurements by Cassini and radio measurements by Huygens showed that Titan likely harbors a large subsurface ocean of water. Cassini also directly imaged Enceladus spewing water from its subsurface ocean into space. Mission operators flew the spacecraft directly through a plume, leading to the discovery of organic materials using Cassini’s onboard mass spectrometer, which determines the elemental makeup of materials passing through it.
NASA / JPL-Caltech
Titan's Lake District
Cassini flew past Titan 127 times during its time at Saturn. This map of Titan's lakes and seas near the moon's northern polar region was created from numerous Cassini radar scans. The three largest seas are Punga Mare (closest to the pole), Ligeia Mare, and the biggest, Kraken Mare.
Cassini performed what NASA dubbed the "Grand Finale" of its mission in 2017: a number of passes between Saturn and its inner rings. In these close encounters, Cassini measured the mass of the rings based on how the spacecraft was gently tugged towards them, and found them to weigh less than even the small moon Mimas, which is just 200 kilometers (124 miles) wide. Combined with the fact that the rings are bright, undarkened by constant space weathering, this hints that they are less than 100 million years old—very young in geological terms. Cassini ended its mission with an intentional plunge into Saturn in September 2017, becoming a permanent part of the planet it was sent to study.
Cassini makes the plunge
NASA's Cassini spacecraft plunges toward the gap between Saturn and its rings.
Cassini left an impressive legacy for future missions. As an all-purpose, flagship spacecraft, it was designed to answer general questions about Saturn and its moons, and help us figure out questions for new missions to answer.
The next—and at the moment, only—spacecraft heading to the Saturn system is Dragonfly. Dragonfly is a NASA mission to Titan scheduled to launch in 2026 and arrive in 2034. The spacecraft is an 8-bladed drone-like craft called a quadcopter that will make short flights around the surface.
NASA / JPL-Caltech / SSI / Val Klavans
Saturn and Titan in true color
Titan hovers near Saturn's rings in this true color view of the two worlds. This composite is comprised of images taken by the Cassini Imaging Science Subsystem (ISS) on 6 May 2012 from a distance of ~770,000 kilometers.
Dragonfly will study the chemicals that rain from Titan’s atmosphere onto the surface. Because we think Titan’s atmosphere is similar to Earth’s when life arose around 3.5 billion years ago, the mission will help us understand possible starting ingredients for life here and elsewhere.
Life as we know it needs 3 things: an energy source like sunlight, a liquid solvent like water, and complex, organic molecules that bond with one another. Titan has the latter, but it’s very cold and has methane and ethane on the surface instead of water. Dragonfly will, in a sense, be studying an alternate version of Earth to see what chemical processes are happening, and how that relates to both life as we know it and possible forms of life unlike anything we’ve ever imagined.
What can you do to support Saturn exploration?
Cassini gathered a treasure trove of beautiful images during its 13 years at Saturn, many of which can be found in our image library. By sharing the beauty of Saturn and its moons with others, you can help us build public support for future missions.
You can also cheer on NASA’s upcoming Dragonfly mission to Titan. Visit our Dragonfly mission page to learn more about why we’re sending this ambitious, flying spacecraft to Saturn’s largest moon, and how it will explore the surface.
Saturn's moon Titan has an atmosphere is similar to Earth’s when life arose here 3.5 billion years ago. By studying Titan, Dragonfly will help us understand possible starting ingredients for life on Earth and elsewhere.
Do you think NASA should get started building another mission to Saturn, or perhaps go looking for signs of life on icy Enceladus? Learn how NASA prioritizes the places we explore by learning about the decadal survey, a report prepared by the scientific community every 10 years.
Finally, learn why missions like Cassini and Dragonfly can’t happen without sustained support from NASA, the White House, Congress, the scientific community, industry, and the public—that means you! Take our Space Advocacy 101 course to learn the inner works of NASA, how Congress develops space legislation, and how to engage with your elected officials.
This page was written by Jatan Mehta in May 2020 and edited by Planetary Society staff writers.
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