Courtesty of Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS)aboard NASA’s Van Allen Probes team at the University of Iowa

Chorus Radio Waves within Earth's Atmosphere

Saturn’s ocean-bearing moon also bears some spooky sounds! Here’s one captured by our Cassini spacecraft.

Cassini: Enceladus Sound

Saturn is a source of intense radio emissions, which were monitored by our Cassini spacecraft. The radio waves are closely related to the auroras near the poles of the planet. These auroras are similar to Earth's northern and southern lights. This is an audio file of radio emissions from Saturn.

Cassini: Saturn Radio Emissions #1

Cassini: Saturn Radio Emissions #2

Juno will improve our understanding of the solar system's beginnings by revealing the origin and evolution of Jupiter.

Juno: Entering Jupiter's Magnetosphere

Whistler waves as heard by the EMFISIS instrument aboard NASA’s Van Allen Probes as it passed around Earth.

Credits: NASA/University of Iowa

Whistler Waves

Chorus waves as heard by the EMFISIS instrument aboard NASA’s Van Allen Probes as it passed around Earth.

Credits: NASA/University of Iowa

Plasmawaves - Chorus

Hear intriguing radio waves that our Cassini spacecraft collected near Jupiter in January 2001.

Jupiter Sounds 2001

This recording was produced by converting into audible sounds some of the radar echoes received by Huygens during the last few kilometers of its descent onto Saturn's moon Titan. As the probe approaches the ground, both the pitch and intensity increase. Scientists will use intensity of the echoes to speculate about the nature of the surface.
Credit: ESA/NASA/JPL/University of Arizona

Radar Echoes From Titan's Surface

Before settling into orbit around Saturn, Cassini faced a white-knuckle ride through the plane of the planet’s rings. When converted into an audio file, the interstellar cacophony is reminiscent of a hellstorm on Earth.

Cassini Shields Up

These melodious tones are created at a special frequency in a plasma with a magnetic field. The frequency is set by the number of electrons in a given volume (the electron density) and the strength of the magnetic field. Hence, the frequency of these waves, called upper hybrid waves, can provide a very accurate measure of the density of the plasma; a fundamental property of the Jovian environment of interest to scientists. These emissions were acquired by Voyager 2 as it passed through the outer magnetosphere in 1979.

Voyager Plasma Sounds

Hello, we’re NASA. You may have seen our astronauts, rocket launches, or Mars rovers — but have you heard our sounds? From interviews with astronauts and engineers to stories that take you on a tour of the galaxy, NASA’s audio offerings let you experience the thrill of space exploration without ever leaving Earth.

Voyager Plasma Sounds

NASA

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