This track sonifies the Chandra Deep Field South, the deepest X-ray exposure ever made, comprising over 81 days of observations with NASA’s Chandra X-ray Observatory. 

Moving from bottom to top, the colors in the image determine the tones played. More specifically, colors toward the red end of the rainbow rumble as lower tones, while colors containing more purple play as higher ones. White areas in the image are heard as white noise. Almost all of the sources represented in the image are black holes or galaxies. Most of the former are supermassive black holes that reside at the centers of galaxies. The wide range of musical frequencies represents the full range of X-ray colors collected by Chandra from this region. Note that as the piece scans upward, the stereo position of the sounds provides clues about the position of the sources from left to right. 

Credit: NASA/CXC/Penn State/B.Luo et al.; Sonification: NASA/CXC/SAO/Kimberly Arcand, SYSTEM Sounds (Matt Russo, Andrew Santaguida)

Chandra Deep Field 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. Each of the four types of light captured by NASA’s Spitzer Space Telescope, Hubble Space Telescope, Galaxy Evolution Explorer, and Chandra X-ray Observatory has their own unique frequency range. At wavelengths where the spiral arms are prominent, the pitch creeps upward as the spiral extends 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: X-ray: NASA/CXC/Wesleyan Univ./R.Kilgard et al; UV: NASA/JPL-Caltech; Optical: NASA/ESA/S. Beckwith & Hubble Heritage Team (STScI/AURA); IR: NASA/JPL-Caltech/ Univ. of AZ/R. Kennicutt; Sonification: NASA/CXC/SAO/Kimberly Arcand, SYSTEM Sounds (Matt Russo, Andrew Santaguida)

M51 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 infrared data from NASA’s Spitzer Space Telescope. 

At this wavelength, the spiral arms are prominent, so the pitch creeps upward as the spiral extends 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: IR: NASA/JPL-Caltech/ Univ. of AZ/R. Kennicutt; Sonification: NASA/CXC/SAO/Kimberly Arcand, SYSTEM Sounds (Matt Russo, Andrew Santaguida)

M51 Infrared Sonification

Messier 51 (M51) is perhaps better known by its nickname of the Whirlpool Galaxy because its face-on orientation to Earth reveals its wound-up spiral arms. This gives telescopes here a view of another spiral galaxy similar to our Milky Way, whose structure we cannot observe directly from our position within 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 X-ray data from NASA’s Chandra X-ray Observatory.

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, including many stellar-sized black holes. 

Credit: X-ray: NASA/CXC/Wesleyan Univ./R.Kilgard et al; Sonification: NASA/CXC/SAO/Kimberly Arcand, SYSTEM Sounds (Matt Russo, Andrew Santaguida)

M51 X-ray 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

Measurements collected by the Waves instrument aboard NASA’s Juno spacecraft during its close flyby of Jupiter’s moon Europa on Sept. 29, 2022 have been converted to an audible frequency. The variation of frequency of the plasma waves observed near Europa can be heard as the plasma density varies.
For more information about NASA’s Juno mission, visit: http://nasa.gov/juno and https://missionjuno.com 
Details about the Europa flyby can be found at: https://www.nasa.gov/feature/jpl/nasa-s-juno-will-perform-close-flyby-of-jupiter-s-icy-moon-europa
Credit: NASA/JPL-Caltech/SwRI/Univ of Iowa

Audio from NASA’s Juno Mission: Europa Flyby

The system called R Aquarii contains two stars — a white dwarf and a red giant — in orbit around each other. In a composite visual image, Hubble data (red and blue) reveal spectacular structures that are evidence of outbursts generated by the pair of stars buried at the center of the image. X-rays from Chandra show a jet from the white dwarf banging into the material surrounding it and creating shock waves. In the sonification of R Aquarii, the piece evolves as a radar-like scan of the image, clockwise starting at the 12 o’clock position. The volume changes in proportion to the brightness of sources in Hubble’s visible light and Chandra’s X-ray image, while the distance from the center dictates the musical pitch (higher notes are farther out). The deep thuds toward the four corners are “diffraction spikes,” which are artifacts from the bright central star. Listeners can hear jets from the white dwarf as the cursor travels near the two o’clock and eight o’clock positions. The ribbon-like arcs captured by Hubble create a rising and falling melody that sounds similar to a set of singing bowls (metal bowls that produce different sounds and tones when struck with a mallet), while the Chandra data are rendered to sound more like a synthetic and windy purr.
NASA/CXC/SAO/K.Arcand, SYSTEM Sounds (M. Russo, A. Santaguida)

R Aquarii Sonification

beat 03 - sleep bleep

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

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 1

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.

M51 X-ray Sonification

NASA

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