Blazars are galaxies whose central supermassive black hole, weighing millions to billions of times our Sun’s mass, blasts a particle jet almost directly toward us at nearly the speed of light.

This track sonifies a decade of gamma rays from the blazar TXS 0506+056 detected by NASA’s Fermi Gamma-ray Space Telescope between August 2008 and May 2018. The percussive sounds match the energy of the detected gamma rays. Unprecedented flaring activity began in April 2017 and continued for months. On Sept. 22, 2017, an observatory at the South Pole detected a high-energy neutrino thought to have originated from the blazar. Credit: NASA/DOE/Fermi LAT Collaboration., Matt Russo and Andrew Santaguida/SYSTEM Sounds

Blazar Flare Sonification

When a star like the Sun begins to run out of helium to burn, it will blow off huge clouds of gas and dust. These outbursts can form spectacular structures such as the one seen in the Cat's Eye nebula. This image of the Cat's Eye contains both X-rays from Chandra around the center and visible light data from the Hubble Space Telescope, which show the series of bubbles expelled by the star over time. To listen to these data, there is a radar-like scan that moves clockwise emanating from the center point to produce pitch. Light that is further from the center is heard as higher pitches while brighter light is louder. The X-rays are represented by a harsher sound, while the visible light data sound smoother. The circular rings create a constant hum, interrupted by a few sounds from spokes in the data. The rising and falling pitches that can be heard are due to the radar scan passing across the shells and jets in the nebula.  (Credit: NASA/CXC/K. Arcand and SYSTEM Sound/M. Russo & A. Santaguida, 2021)

Cat's Eye Nebula Sonification

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

白炎 (Hakuen)

モーブホール (Mauve hole)

Artwork by Andrei Alecsandru
Music written and mastered by Ivo São Bento.
Released February 4, 2022
Ivo São Bento, sonic concepts.

Demo2-2

42! (yottsuu!)

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