Home Science Space Listen to Saturn: Radio Emissions of the Planet and Enceladus

Listen to Saturn: Radio Emissions of the Planet and Enceladus

New research from NASA’s Cassini spacecraft’s up-close Grand Finale orbits shows a surprisingly powerful and dynamic interaction of plasma waves moving from Saturn to its rings and its moon Enceladus. The observations show for the first time that the waves travel on magnetic field lines connecting Saturn directly to Enceladus.

The field lines are like an electrical circuit between the two bodies, with energy flowing back and forth. Researchers converted the recording of plasma waves into a “whooshing” audio file that you can hear — in the same way a radio translates electromagnetic waves into music. In other words, Cassini detected electromagnetic waves in the audio frequency range — and on the ground, it was possible to amplify and play those signals through a speaker. The recording time was compressed from 16 minutes to 28.5 seconds.

Much like air or water, plasma (the fourth state of matter) generates waves to carry energy. The Radio Plasma Wave Science (RPWS) instrument onboard NASA’s Cassini spacecraft recorded intense plasma waves during one of its closest encounters to Saturn. Ali Sulaiman, a planetary scientist at the University of Iowa, Iowa City, and a member of the RPWS team, said:

Sulaiman is the lead author of a pair of papers describing the findings, published in Geophysical Research Letters. The interaction of Saturn and Enceladus is different from the relationship of Earth and its Moon. Enceladus is immersed in Saturn’s magnetic field and is geologically active, emitting plumes of water vapor that become ionized and fill the environment around Saturn.


Our own Moon does not interact in the same way with Earth. Similar interactions take place between Saturn and its rings, as they are also very dynamic. The recording was captured on Sept. 2, 2017, two weeks before Cassini was deliberately plunged into the atmosphere of Saturn. The recording was converted by the RPWS team at the University of Iowa, led by physicist and RPWS Principal Investigator Bill Kurth.

 Provided by: Jet Propulsion Laboratory [Note: Materials may be edited for content and length.]

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  • Troy was born and raised in Australia and has always wanted to know why and how things work, which led him to his love for science. He is a professional photographer and enjoys taking pictures of Australia's beautiful landscapes. He is also a professional storm chaser where he currently lives in Hervey Bay, Australia.

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