Saturn may have flown solo for billions of years, almost its entire existence, before getting its stunning set of rings, a new study suggests.
An Italian-led team has reported in the journal Science that Saturn’s primary rings appear to be just 10 million to 100 million years old.
The gas giant Saturn, on the other hand, is 4.5 billion years old, like all the other planets in our solar system.
We’re seeing #Saturn’s rings at just the right time. Scientists estimate that this spectacular phenomenon is no more than 100 million years old—a short time during the life of the solar system—and the rings won’t last forever. Learn more: https://t.co/KWDIKAbwmm pic.twitter.com/upQ9ZlV1wY
— NASA Solar System (@NASASolarSystem) December 17, 2018
The findings are based on data collected by Nasa’s Cassini spacecraft while repeatedly diving between Saturn and its rings in 2017, shortly before its demise.
By estimating the mass of the rings through gravity measurements, the researchers gauged the age of the three main rings: A, B and C.
It is still a mystery, though, how these icy rings formed.
Scientists suspect a collision between two of Saturn’s many moons or perhaps a moon and comet.
The rings are made mostly of ice.
The remaining 1% is dust and possibly organic contaminants.
Overall, the material ranges in size from tiny particles, to pebbles, to boulders.
How old are #Saturn’s rings?
Data from @CassiniSaturn suggest they’re younger than the planet, forming 10–100 million years ago when dinosaurs lived on Earth: https://t.co/RVXU5Lqysh pic.twitter.com/1VjKmbMkvW
— NASA JPL (@NASAJPL) January 17, 2019
Lead researcher Luciano Iess, a planetary scientist at Sapienza University in Rome, said orbital motion sprayed the dust and other contaminants onto the icy rings at a constant rate.
His team calculated the length of time it would take for the contaminants to accumulate, it turned out to be a “short” 10 million to 100 million years.

But Mr Iess said there was little consensus for that theory.
Mr Iess said Nasa’s Voyager spacecraft, as well as Cassini, had already provided clues that the rings had not formed with Saturn.
“But now we have much more concrete evidence, which was only possible to obtain during the final phase of the mission, called the Grand Finale,” he wrote in an email.

The masses of Saturn’s fainter D, F, G and E rings are considered negligible, the researchers wrote.
Saturn’s E ring, meanwhile, has its own unique source: plumes of water vapour streaming into space from the moon Enceladus, believed to harbour an ocean beneath its surface.
The Cassini-Huygens mission launched #OTD in 1997 aboard a Titan IVB/Centaur rocket at Cape Canaveral Air Station! It took seven years for the spacecraft to reach Saturn. Image on the right is a true-color view of Saturn from @CassiniSaturn taken in 2011. pic.twitter.com/luGQ1LRyCk
— NASA History Office (@NASAhistory) October 15, 2018
Mr Iess noted the latest findings are “another gift we received from this beautiful mission”.
“Cassini, like all giants, has left a legacy that will last for a long time,” he said.
Cassini was launched from Florida in 1997.
It carried the European probe named Huygens, which separated and landed on Saturn’s moon Titan in 2005.

