Every half hour, Saturn's rings lose enough water to fill an Olympic swimming pool. That is NASA's estimate, published in December 2018 from a study led by James O'Donoghue, and at that pace the rings have somewhere between 100 and 300 million years left. So imagine the pace holds. Imagine they go.
In this episode: where the rain comes from, from the dark bands Voyager 2 saw in 1981 to the Keck telescope and Cassini's 22 dives between Saturn and its rings in 2017. What a Saturn without rings would look like from Earth, and why we already saw one in March 2025, when the rings turned edge-on and a sheet about 10 meters thick vanished from view. How Cassini weighed the rings while falling through Saturn's gravity, and why that weight, roughly 40 percent of the moon Mimas, points, in JPL's words, to rings that may have formed during the age of dinosaurs. Then Beyond the Obvious: the rings on a timeline against Saturn's 4.5 billion years, the first dinosaurs, the asteroid and Homo sapiens. We lay out the argument of 2019 to 2026 over whether the rings are young at all, the lost moon Chrysalis, and the part you can check yourself: on October 4, 2026, Saturn is at opposition, its closest to Earth this year, up all night. We close with a question closer to home: are we sure how our own Moon was born?
Every figure comes from NASA, JPL, Science, Nature Astronomy and Nature Geoscience pages, linked in the video description on YouTube. Where the sources don't explain something, we say so.
Watch the video edition: https://www.youtube.com/watch?v=4Z05gIIf7nA
Narration: synthetic voice. Research, writing and editing: human work. Echoes of the Void.