NASA has produced a new sonification, translation of astronomical data into sound, from the characteristic black hole at the center of the Perseus cluster of galaxies.
this black hole has been associated with sound since 2003 when astronomers discovered that the pressure waves it emitted caused ripples in the hot gas of the cluster that might be translated into a note, one that humans cannot hear, regarding 57 octaves below middle C.
In some ways, the new sonification is unlike anything done before. because it revisits the actual sound waves discovered in the Chandra X-ray Observatory data from NASA.
As explained by NASA in a statement, the popular misconception that there is no sound in space originates from in the fact that most of space is essentially a vacuum, it does not provide a medium for sound waves to propagate.
A cluster of galaxies, on the other hand, has copious amounts of gas that envelop the hundreds or even thousands of galaxies within it, providing a medium for sound waves to travel.
In this new sonification of Perseus, sound waves previously identified by astronomers were extracted and audible for the first time. The sound waves were drawn in radial directions, that is, away from the center. The signals were then resynthesized to the range of human hearing by boosting them 57 and 58 octaves above their actual pitch.
Another way of expressing this is that it is heard 144 quadrillion and 288 quadrillion times more than its original frequency. Radar-like scanning around the image allows you to hear waves emitted in different directions. In the visual image of this data, both blue and purple show X-ray data. captured by Chandra.
In addition to the Perseus cluster of galaxies, NASA has produced a new sonification of another famous black hole. Studied by scientists for decades, the black hole in Messier 87 (M87) gained celebrity status in science following being imaged by the Event Horizon Telescope (EHT) project in 2019.
This new sonification does not present the EHT data, but analyzes data from other telescopes that observed M87 on much larger scales at regarding the same time.
The visual format image contains three panels that are, from top to bottom, X-rays from Chandra, optical light from NASA’s Hubble Space Telescope, and radio waves from the Atacama Large Millimeter Array in Chile. The brightest region on the left of the image is where the black hole is located, and the structure in the upper right is a jet produced by the black hole. The jet is produced by material falling onto the black hole.
Sonification scans the image of three levels from left to right, with each length wave assigned to a different range of audible tones.
Radio waves are assigned to lower tones, optical data to midtones, and X-rays detected by Chandra to higher tones. The brightest part of the image corresponds to the noisiest part of the sonificationwhich is where astronomers find the 6.5 billion solar mass black hole that the EHT captured.
PJG
