It turns out that Saturn’s rings are much younger than we thought. A new study led by physicist Sascha Kempf from the University of Colorado Boulder has confirmed that the rings are relatively young: They are at most 400 million years old, while Saturn itself is 4,500 million years old.
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Saturn’s rings have been fascinating scientists and non-scientists alike for 400 years. In 1610, Galileo Galilei saw the rings for the first time through his 20-power telescope. However, the rings didn’t appear to him sharply as “rings” but looked more like “ears”. In 1859, James Maxwell proposed that a ring couldn’t be one solid piece but instead was composed of countless small pieces, all independently orbiting Saturn. Throughout the whole 20th century, scientists assumed that the rings had always accompanied Saturn since the birth of the planet, but there was not yet any evidence to prove or disprove the idea.
Kempf and his colleagues managed to calculate the age of Saturn’s rings by studying a usual object: dust.
In the Solar System, tiny grains of rock are constantly zooming around. When they hit a Saturn’s ring, some of the grains stay behind, forming a thin layer of dust and staining the color of the ring, which is mainly made of shiny water-ice. The researchers thought that they could measure how fast the dust accumulated on the rings over a period of time and then calculate how much time it took for the rings to be covered by the current amount of dust.
In order to study the dust, the researchers used an instrument called the Cosmic Dust Analyzer, which was aboard the Cassini spacecraft that was intentionally plunged into Saturn’s deadly atmosphere in 2017. For 13 years, the instrument collected over 2 million grains of dust and recorded each grain’s velocity. The researchers used this velocity information to determine the likely origin of each grain. For example, slow grains were more likely to come from within the Saturnian system (like from a Saturn’s satellite) and fast grains were more likely to come from outside the Saturnian system. The researchers focused on the grains that most likely came from outside the Saturnian system. There were only 163 that fitted the description but that was enough for a breakthrough. These 163 grains took up some space on Saturn’s rings over a period of time, providing the researchers of the rate at which the dust accumulates on the rings. Then we know for a fact that currently, the dust takes up 0.1% to 2% of the rings. For the dust to build up to that amount on the rings, it takes around 100-400 million years.
In our Solar System, none of the rocky planets have rings. The other gas giants – Jupiter, Uranus, and Neptune – have rings, but their rings are nowhere as colorful, luminous, and colossal as Saturn’s rings. This begs millions of questions: Where did the rings come from? When did they first appear? Will they disappear?
The first estimation of the age helps point the studies on Saturn’s rings to a more focused direction. With a lot of hard work and a little bit of luck, we’ll be able to uncover all the mysteries that the rings hold in the very near future.
Wrriten by Trang Nguyen
Kempf, S., Altobelli, N., Schmidt, J., Cuzzi, J. N., Estrada, P. R., & Srama, R. (2023). Micrometeoroid infall onto Saturn’s rings constrains their age to no more than a few hundred million years. Science Advances, 9(19).