Top 50: Science

The core of our Milky Way galaxy is densely packed with gas, dust, stars, and stellar remnants, but its centerpiece is a monster black hole with a mass of 4 million Suns called Sagittarius A* (pronounced “A-star”).

This sonification tracks an image of the galactic center captured by NASA’s Chandra X-ray Observatory, Hubble Space Telescope, and Spitzer Space Telescope in X-ray, optical, and infrared light, respectively. A different instrument represents each observatory, with a xylophone for Chandra, a violin for Hubble and a soft piano for Spitzer. The translation begins on the left side of the image and moves to the right, with sounds representing the positions and brightness of the sources. The light of objects located toward the top of the image have higher pitch, while the intensity of the light controls the volume. Stars and compact sources emerge as individual notes, while extended clouds of gas and dust produce an evolving drone. A crescendo happens in the brightest region of the image, where the supermassive black hole resides. The Hubble image outlines energetic regions where stars are being born, while Spitzer’s infrared data show glowing clouds of dust containing complex structures. X-rays from Chandra reveal gas heated to millions of degrees from stellar explosions and outflows from Sagittarius A*. 

Credit: X-ray: NASA/CXC/SAO; Optical: NASA/STScI; IR: Spitzer NASA/JPL-Caltech; Sonification: NASA/CXC/SAO/Kimberly Arcand, SYSTEM Sounds (Matt Russo, Andrew Santaguida)

Galactic Center Sonification

Messier 51 (M51) is perhaps better known by its nickname, the Whirlpool Galaxy, because its face-on orientation to us highlights its winding spiral arms. This gives our telescopes a different perspective on a spiral galaxy similar to our Milky Way, whose structure we cannot observe directly since we’re inside it. The sonification tracks along a line emanating from the galaxy's core to the edge of the image and scanning clockwise. The light encountered by this line has been mapped to the notes of a melodic minor scale. The sequence represents optical data from NASA’s Hubble Space Telescope. 

At this wavelength, the spiral arms are prominent, so the pitch creeps upward as the spiral stretches farther from the core. The bright core, which harbors a supermassive black hole, produces a constant low hum punctuated by short sounds from compact bright sources within the galaxy. 

Credit: Optical: NASA/ESA/S. Beckwith & Hubble Heritage Team (STScI/AURA); Sonification: NASA/CXC/SAO/Kimberly Arcand, SYSTEM Sounds (Matt Russo, Andrew Santaguida)

M51 Optical Light Sonification

The joint ESA/Jaxa BepiColombo mission flew past Mercury for the first time on 1 October 2021, capturing data with the magnetometer onboard ESA’s Mercury Planetary Orbiter. A sonification of the magnetic field data is presented here.  
 
Two synthesizers can be heard, which are controlled by three characteristics of the magnetic field. The first synthesizer's pitch represents the slowly changing magnitude of the background magnetic field. First the solar wind is heard, then the increase and decrease of the planetary magnetic field, and then the solar wind again. The lower the pitch, the more intense the magnetic field. 
 
The pitch of the second synthesizer is controlled by the variations of the magnetic field magnitude. A more turbulent magnetic field is represented by a faster change in pitch. The magnetosheath crossing after closest approach is very prominent. 
 
Using the amplitude envelope as a control for the volume of the second synthesizer emphasises the different magnetospheric regions.
 
Full story 
https://www.esa.int/Science_Exploration/Space_Science/BepiColombo/BepiColombo_s_first_tastes_of_Mercury_science

Credit: ESA/BepiColombo/MPO-MAG/IGEP-IWF-IC-ISAS

Image credit: ESA/ATG medialab

Sound of the solar wind at Mercury

A near-infrared image of the Cosmic Cliffs in the Carina Nebula, captured by NASA’s Webb Telescope, has been mapped to a symphony of sounds. This track includes sounds from just the top half of the image, which resembles a dark blue night sky. The gas and dust that are represented in blue hues have been translated to windy, drone-like sounds. The sonification scans the image from left to right.
 
This sonification does not represent sounds recorded in space. Two musicians mapped the telescope’s data to sound, carefully composing music to accurately represent details the team would like listeners to focus on. In a way, this sonification is like modern dance or an impressionist painting – it converts Webb’s image to a new medium to engage and inspire listeners.

Brighter light in the image is louder. The vertical position of light also dictates the frequency of sound. For example, bright light near the top of the image sounds loud and high, but bright light near the bottom is loud and lower pitched.

Learn more: https://www.nasa.gov/feature/goddard/2022/nasa-webb-s-first-full-color-images-data-are-set-to-sound

Credits: Image: NASA, ESA, CSA, and STScI; Accessibility Production: NASA, ESA, CSA, STScI, and Kimberly Arcand (CXC/SAO), Matt Russo and Andrew Santaguida (SYSTEM Sounds), Quyen Hart (STScI), Claire Blome (STScI), and Christine Malec (consultant).

Webb’s Cosmic Cliffs Sonification: Sky

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

Voyager 1's plasma wave instrument detected the vibrations of dense interstellar plasma, or ionized gas, from October to November 2012 and April to May 2013. This sound reproduces the amplitude and frequency of the plasma waves as "heard" by Voyager 1.

Voyager: Interstellar Plasma Sounds

Solfeggio frequencies recorded on the morning of the winter solstice copyright Tai Inoue at Nature Sounds 2011 

Windy Winter Solstice - Lakefield National Park, Cape York

The Voyager 1 spacecraft has experienced three "tsunami waves" in interstellar space. Listen to how these waves cause surrounding ionized matter to ring. More details on this sound can be found here: http://www.nasa.gov/jpl/nasa-voyager-tsunami-wave-still-flies-through-interstellar-space/

Voyager 1: Three "Tsunami Waves" in Interstellar Space

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

Juno: Crossing Jupiter's Bow Shock

Plasmaspheric hiss waves as heard by NASA’s Polar mission as it passed around Earth.

Credits: NASA/University of Iowa

Plasmaspheric Hiss

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

New research from the up-close Grand Finale orbits of NASA’s Cassini mission shows a surprisingly powerful interaction of plasma waves moving from Saturn to its moon Enceladus. Researchers converted the recording of plasma waves into a “whooshing” audio file that we can hear -- in the same way a radio translates electromagnetic waves into music. Much like air or water, plasma (the fourth state of matter) generates waves to carry energy. The recording was captured by the Radio Plasma Wave Science (RPWS) instrument Sept. 2, 2017, two weeks before Cassini was deliberately plunged into the atmosphere of Saturn. 

For more information, visit: https://saturn.jpl.nasa.gov 

Credit: NASA/JPL-Caltech/University of Iowa

Sounds of Saturn: Hear Radio Emissions of the Planet and Its Moon Enceladus

The Stanford Experimental Physics Lab sonified data from the European Space Agency and NASA's Solar and Heliospheric Observatory (SOHO). This humming sound captures the Sun’s natural vibrations and provides scientists with a concrete representation of its dynamic movements.

For more solar sounds, visit: http://soi.stanford.edu/results/sounds.html

Sun Sonification

One year and three trips around the Sun later, NASA's Parker Solar Probe heard some weird, sci-fi sounds from plasma within the solar wind -- and those sounds may answer unanswered questions about how the wind forms.

Parker Solar Probe - Whistler Mode Waves 2

Parker Solar Probe - Langmuir Waves

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.

Plasmaspheric Hiss

NASA

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