The Real Lord of the Rings
Four hundred years after they were discovered, Saturn's
breath-taking rings remain a mystery.
February 12, 2002: Galileo Galilei was accustomed to extraordinary discoveries. Using his primitive telescope he had found new worlds orbiting Jupiter, watched planet-sized spots crossing the Sun, and explored craters on the Moon. But when Galileo turned his telescope toward Saturn in 1610, even he was amazed.
The planet looked nothing like others in the solar system. Through 17th century optics, Saturn appeared to be one bright star closely flanked by two dimmer ones -- a blurry suggestion of the planet's magnificent rings.
What Galileo did next was nearly as unusual as Saturn itself.
Above: Hubble Space Telescope images of Saturn and its rings. [more]
Nowadays anyone with a department store telescope can get a better view of Saturn's rings than Galileo did. Otherwise, matters stand much as they did four hundred years ago. First-time observers of the planet still step back from their telescopes speechless. And scientists are still puzzled.
"After all this time we're still not sure about the origin of Saturn's rings," says Jeff Cuzzi, a planetary scientist at the NASA Ames Research Center. Astronomers once thought that Saturn's rings formed when Saturn did: 4.8 billion years ago as the Sun and planets coalesced from a swirling cloud of interstellar gas. "But lately," Cuzzi says, "there's a growing awareness that Saturn's rings can't be so old."
Cuzzi speculates that some hundreds of millions of years ago -- a time when the earliest dinosaurs roamed our planet -- Saturn had no bright rings. Then, he says, something unlikely happened: "A moon-sized object from the outer solar system might have flown nearby Saturn where tidal forces ripped it apart. Or maybe an asteroid smashed one of Saturn's existing moons." The debris encircled the planet and formed the rings we see today.
Left: Saturn's rings might have formed only a few hundred million years ago when dinosaurs and their cousins roamed our planet. Credit: Humboldt State University [more]
Saturn's ring particles range in size from microscopic dust to barn-sized boulders. If you assembled them all in one place, notes Cuzzi, you would have enough material to make an icy satellite one or two hundred kilometers wide -- much like Saturn's present-day moon Mimas.
The debris layer is extraordinarily thin, he marvels. "Saturn's rings are 250,000 km wide, but only a few tens of meters thick. A sheet of paper the size of San Francisco would have about the same ratio of width to depth." Indeed, if you made a 1-meter-wide scale model of Saturn, the rings would be 10,000 times thinner than a razor blade.
Cuzzi says there are two reasons to believe the rings are young:
First, they are bright and shiny like something new. It's no joke, he assures. The wide-spanning rings sweep up space dust (bits of debris from comets and asteroids) as Saturn orbits the Sun. Rings much older than a few hundred million years would be darkened by accumulated dust. "The fact that they're bright suggests they're young," he says.
Above: Saturn's rings are very thin. Astronomers using the Hubble Space Telescope captured this image of the rings edge-on in 1995. Star-like objects in the ring plane are icy satellites. [more]
Second, small moons that orbit through the outermost regions of the ring system are gaining angular momentum at the expense of the rings. "During the next few hundred million years," explains Cuzzi, "the outer half of the rings will fall toward the planet, and the little moons -- called shepherd satellites -- will be flung away. This is a young dynamical system."
The first argument (shiny rings) is less certain than the second (angular momentum), he cautions, "because we're not sure there's enough dust at the orbit of Saturn to pollute and blacken the rings." NASA's Cassini spacecraft will measure the dust population when it reaches Saturn in 2004. Then, perhaps, there will be no doubt.
Right: Saturn's 200 km-wide moon Mimas, also known as the "Death Star" satellite because of its distinctive impact crater, is about as massive as Saturn's rings. [more]
Cuzzi hopes Cassini will solve other ring-mysteries, too. "In the early '80's," he recalls, "the Voyager spacecraft visited Saturn and took close-up pictures that revealed many strange things in the rings, including spokes, braids and waves.
"Some of the waves have a spiral shape, like the spiral arms of galaxies," says Cuzzi. To an astronaut floating among the rings, such waves would appear to be gentle swells, a few kilometers high and hundreds of kilometers wide. They move around the rings every few days or weeks. "We understand these spiral waves," he added. They're triggered by gravitational tugs from Saturn's moons -- the same ones that are sapping the rings' angular momentum.
Other structures, like spokes and irregular ripples, are puzzling. Some of them might be signs of space rocks plunging through the ring system. Others might be spawned by tiny moonlets, as yet undiscovered, plowing through Saturn's rings. "Cassini, which will orbit Saturn for years, should provide some answers," he says.
In many science fiction tales, alien visitors are amazed by Saturn as if there were no ringed planets back in their own solar system. According to Cuzzi, Saturn's rings might be rare indeed. "If they are as short-lived as we think, we're lucky to be here at just the right time to see them."
Actually, other giant planets in our solar system do have rings, but they are very dark and millions of times less massive than the rings of Saturn. Jupiter's rings are made of bits of dust that fly off Jupiter's moons when they are struck by meteorites. No one is sure what made the black rings of Neptune and Uranus, although Cuzzi notes they could be debris from kilometer-sized moonlets that were struck by asteroids.
In another few hundred million years, if Cuzzi is right, Saturn's rings will sag inward and our solar system will become a little more ordinary. Perhaps by then star-faring humans will have seen countless ringed planets elsewhere in the Galaxy and won't care much what happens to Saturn. On the other hand, maybe Saturn's rings really are a Galactic wonder, and super-engineers of the distant future will take measures to preserve them.
No one knows.
We can only be sure that Saturn's rings are lovely now. And if they are indeed fleeting, as such ages are reckoned for stars and planets, their short life makes them even more wonderful. Don't miss them!
Editor's Note: This month is a good time to see Saturn. Northern-hemisphere sky watchers canhigh overhead after sunset; it is one of the brighter stars in the sky. Southern-hemisphere observers should near the northern horizon. On Feb. 20th, Saturn will have a close encounter in the sky with Earth's Moon. Stay tuned to Science@NASA for details.... Web Links and more...
Why are Saturn's rings so thin? Cuzzi explains: In the beginning, the rings might have been "fat" -- like a bagel or doughnut -- but they would have flattened over time because collisions between ring particles are inelastic. (An inelastic collision is like two lumps of clay colliding; they don't bounce.) "If there were large vertical motions among the ring particles, those motions would be damped by collisions." Ring particles would "settle" into their average orbital plane, and the rings would become more like an old-fashioned phonograph record than a bagel.
Cassini-Huygens Mission -- (JPL) learn more about the Cassini spacecraft, which will reach Saturn in 2004 to explore the ringed planet and its intriguing satellite Titan.
Galileo Discovers Saturn's Rings -- (Rice University) learn more about Galileo's observations of Saturn and the anagram he used to report his discovery of the rings, from Rice University
Jupiter's rings formed from dust blasted off tiny moons -- (Astronomy Now) NASA's Galileo spacecraft solves the mystery of Jupiter's moons.
Join our growing list of subscribers - sign up for our express news delivery and you will receive a mail message every time we post a new story!!!