Cassini Begins Saturn Ring Dives, Kicks Off Mission Finale

Saturns' rings animation
This NASA gif shows the different ring segments that surround Saturn. The narrow F ring marks the outer boundary of the main ring system. (Image credit: NASA/JPL-Caltech/Space Science Institute)

NASA's Cassini spacecraft begins a series of daring dives through Saturn's rings Nov. 30, the first step in the probe's "grand finale" investigation of the gas giant planet.

From Nov. 30 to April 22, Cassini will dive through the outer edge of Saturn's rings 20 times, once every seven days. The spacecraft will be entering uncharted territory, getting the closest look ever at Saturn's outer rings and its moons. NASA described this phase of the mission in a new video.

"We're calling this phase of the mission Cassini's Ring-Grazing Orbits, because we'll be skimming past the outer edge of the rings," Linda Spilker, Cassini project scientist at NASA's Jet Propulsion Laboratory (JPL) in California, said in a statement. "In addition, we have two instruments that can sample particles and gases as we cross the ring plane, so in a sense, Cassini is also 'grazing' on the rings." [Saturn's Hexagon, Rings and More 'Stared at' for Days - Cassini Time-Lapse Video]

This isn't the first time Cassini has broken new ground. Over its 12 years in Saturn's system, the probe has dropped a lander on Saturn's moon Titan, discovering the satellite's methane seas; discovered an underground ocean on the moon Enceladus; and investigated the origins of Saturn's strange, giant hexagonal jet stream. (Plus, Cassini discovered multiple new moons around Saturn.)

Cassini left for Saturn in 1997, taking a complicated path past Venus twice, Earth and then Jupiter to build up speed before reaching the ringed planet's system in 2004.

Cassini will pass through a faint outer ring for a few orbits, and then probe the outer reaches of Saturn's F ring, which marks the boundary of the main ring system. The F ring is about 500 miles (800 kilometers) wide — narrow compared to other rings — and features constantly changing streamers, filaments and dark channels that change over the course of hours, NASA researchers said in the statement.

"Even though we're flying closer to the F ring than we ever have, we'll still be more than 4,850 miles (7,800 km) distant." Earl Maize, Cassini project manager at JPL, said in the statement.

While there, Cassini will explore the many small moons orbiting within and near the rings (including Pandora, Atlas, Pan and Daphnis), scoop up ring particles and gas to analyze, and build an in-depth scan of the rings' structure.

NASA's Cassini spacecraft has racked up some impressive results during its 12-year mission at Saturn. (Image credit: NASA/ Jet Propulsion Laboratory-Caltech)

After the mission phase ends in April, Cassini will begin the "Grand Finale" proper, slinging around the moon Titan to begin 22 dives between Saturn and its rings, and finally turning to dive into the planet's atmosphere on Sept. 15. Researchers will use observations of the planet during this ring-grazing phase of to calculate how close the spacecraft can safely go during its dives before the final plunge, the scientists said.

That final dive will not only keep the spacecraft, running out of fuel, from contaminating Saturn's potentially habitable moons, but it will also provide an unprecedented view of the planet's gravity, composition and atmosphere.

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Sarah Lewin
Associate Editor

Sarah Lewin started writing for in June of 2015 as a Staff Writer and became Associate Editor in 2019 . Her work has been featured by Scientific American, IEEE Spectrum, Quanta Magazine, Wired, The Scientist, Science Friday and WGBH's Inside NOVA. Sarah has an MA from NYU's Science, Health and Environmental Reporting Program and an AB in mathematics from Brown University. When not writing, reading or thinking about space, Sarah enjoys musical theatre and mathematical papercraft. She is currently Assistant News Editor at Scientific American. You can follow her on Twitter @SarahExplains.