You’ve heard the creaks, cracks, and cackling noises of our universe before. Using data from our spacecraft, our scientists gathered NEW sinister sounds from the depths of space in time for Halloween.
 
Listen to our playlist filled with new “moans” and “whistles” from our universe that would scare the most ghoulish of creatures.

Sinister Sounds of the Solar System and Beyond

☆☆☆☆☆☆☆☆

ፕꏂርዘñዐ¹

gfvvzghz

NASA

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

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

Studied by scientists for decades, the black hole in Messier 87, or M87, gained celebrity status in science after the first release from the Event Horizon Telescope (EHT) project in 2019. This new sonification does not feature the EHT data, but rather looks at data from other telescopes that observed M87 on much wider scales at roughly the same time. The image in visual form contains three panels that are, from top to bottom, X-rays from NASA’s Chandra X-ray Observatory, optical light from NASA’s Hubble Space Telescope, and radio waves from the Atacama Large Millimeter Array in Chile. The sonification scans across the three-tiered image from left to right, with each wavelength mapped to a different range of audible tones. Radio waves are mapped to lowest tones, optical data to medium tones, and X-rays detected by Chandra to the highest tones. The brightest part of the image corresponds to the loudest portion of the sonification, which is where astronomers find the 6.5 billion solar mass black hole that EHT imaged.

Learn more: https://chandra.si.edu/photo/2022/sonify5/ 

Sonification Credit: NASA/CXC/SAO/K.Arcand, SYSTEM Sounds (M. Russo, A. Santaguida)

Black Hole Sonification: M87

alvedon — our last goodbye

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

Listen to the eerie sound of a boom on board ESA’s Jupiter Icy Moons Explorer (Juice) spacecraft deploying in space during commissioning of the spacecraft in May 2023.

 

Tip: use headphones or surround speakers for the best experience – the forward and backward wobbles of the boom come through the left and right channels.

 

The vibration signal used to create the sound came from the accelerometer on board the main body of the spacecraft, which was switched on to monitor the reaction of the spacecraft to the boom’s deployment.

 

The larger the vibration measured by the accelerometer, the louder the sound in the sonification. We can imagine the boom like a human arm initially folded into the body; the first higher-pitched ‘ring’ that you hear is the elbow opening and the second lower-pitched ring is the shoulder stretching up.

 

Though the accelerometer measurements were not mandatory to validate the deployment, the engineers working on Juice were happy to see that they are very accurate. Turning the vibration signal into sound may help us understand the mechanics of the deployment.

 

The boom is one of four 'Langmuir probes' that are part of Juice's Radio & Plasma Wave Investigation experiment. These probes will provide crucial information on the electric fields and plasma environment around Jupiter's moons.

 

The sonification was prepared by Johannes Z. D. Mieth (TU Braunschweig) and Willi Exner (ESA).

 

#ESAJuice #Jupiter #ESA #EuropeanSpaceAgency

Sound of a Juice boom deploying

How to pronounce the name of Rosetta's comet: Churyumov–Gerasimenko. After Klim Churyumov and Svetlana Gerasimenko, the two Ukrainian astronomers who discovered it in 1969. Courtesy of Irina Vavilova from the Main Astronomical Observatory of the National Academy of Sciences of Ukraine.

Churyumov - Gerasimenko - Audio by Irina Vavilova

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

UPDATE (20 Aug 2015): What made the comet sing? Scientists working on Rosetta's RPC instrument have found out why 67P/C-G was singing. Via http://wp.me/p46DHN-1nN
==
ORIGINAL Citation (Oct 2014): Rosetta’s Plasma Consortium (RPC) has uncovered a mysterious ‘song’ that Comet 67P/Churyumov-Gerasimenko is singing into space. The comet seems to be emitting a ‘song’ in the form of oscillations in the magnetic field in the comet’s environment. It is being sung at 40-50 millihertz, far below human hearing, which typically picks up sound between 20 Hz and 20 kHz. To make the music audible to the human ear, the frequencies have been increased in this recording. This sonification of the RPC-Mag data was compiled by German composer Manuel Senfft (www.tagirijus.de).  Read full details in ESA's Rosetta blog: http://wp.me/p46DHN-Li 

Copyright Notice

Original Data Credit: ESA/Rosetta/RPC/RPC-MAG
Sonification: TU Braunschweig/IGEP/Manuel Senfft, CC-BY-NC-SA 4.0 http://creativecommons.org/licenses/by-nc-sa/4.0/

Thumbnail image credit: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0

A Singing Comet

For the first time, NASA released a sonification simultaneously with news results associated with two of its telescopes, the Imaging X-ray Polarimetry Explorer (IXPE) and the Chandra X-ray Observatory. The data cover the region near the supermassive black hole at the center of the Milky Way galaxy. The black hole, known as Sagittarius A*, is barely seen in the lower right-hand of the visual image that contains X-ray data from IXPE (red-orange) and Chandra (purple). In the sonification of these data, the cursor begins at Sagittarius A* and moves out as a growing circle toward the center of the image. As it encounters IXPE data, the volume of the notes changes according to the brightness of the X-rays. The brighter the Chandra data, the higher the musical pitch and vice versa. When the cursor travels over a large patch of X-rays both from Chandra and IXPE in the center of the image, a rushing sound is heard. This region is where scientists find a “light echo,” a high-energy relic left behind from an eruption from Sagittarius A* about 200 years ago.

Sagittarius A* Light Echo Sonification

One of the surprising features of black holes is that although light (such as radio, visible, and X-rays) cannot escape from them, surrounding material can produce intense bursts of electromagnetic radiation. As they travel outward, these blasts of light can bounce off clouds of gas and dust in space, similar to how light beams from a car’s headlight will scatter off fog.
A new sonification turns these “light echoes” from the black hole called V404 Cygni into sound. Located about 7,800 light-years from Earth, V404 Cygni is a system that contains a black hole, with a mass between five and 10 times the Sun’s, that is pulling material from a companion star in orbit around it. The material is funneled into a disk that encircles the stellar-mass black hole.
This material periodically generates bursts of radiation, including X-rays. As the X-rays travel outward they encounter clouds of gas and dust in between V404 Cygni and Earth and are scattered at various angles. NASA’s Chandra X-ray Observatory and Neil Gehrels Swift Observatory have imaged the X-ray light echoes around V404 Cygni. Because astronomers know exactly how fast light travels and have determined an accurate distance to this system, they can calculate when these eruptions occurred. This data, plus other information, helps astronomers learn more about the dust clouds, including their composition and distances.

V404 Cygni Sonification

This image shows the region around the Milky Way's central supermassive black hole, known as Sagittarius A* (Sgr A*), in infrared (orange and purple) and X-ray light (blue). The image is scanned from left to right and the data are transformed into sound. The brightness of the objects is represented by the volume, while the vertical positions of the sources in the image are mapped to musical pitches. X-rays are played with a soft synthesizer and the infrared data are heard as bass notes and plucked sounds. The brightest region in the middle of the image (and hence the loudest) is where Sgr A* the black hole, resides. It is within this area that the Event Horizon Telescope was able to peer to obtain the first image of Sgr A* itself.

Sagittarius A* Sonification

MSH 15-52 is a cloud of energized particles blown away from a dead, collapsed star. This image includes X-rays from NASA’s Chandra X-ray Observatory (orange, green and blue) as well as the Imaging X-ray Polarimetry Explorer, or IXPE (purple). X-ray data have been combined with infrared data from the Dark Energy Plane Survey 2 (red and blue). In sound, the scan goes from the bottom to the top. The brightness of the Chandra data of the cloud has been converted into rough string-like sounds, while the blast wave is represented by a range of pitches of firework-type noises. The IXPE data are heard as wind-like sounds. The infrared data are mapped to musical pitches of a synthesizer sound. The light curve, or brightness over time, from the dead star’s collapsed core is heard in pulses that occur almost 7 times every second as it does in the original data.

Credits: Images: X-ray: NASA/CXC/Stanford Univ./R. Romani et al. (Chandra); NASA/MSFC (IXPE); Infrared: NOIRLab/DECam; Image Processing: NASA/CXC/SAO/J. Schmidt; Sonification: NASA/CXC/SAO/K.Arcand, SYSTEM Sounds (M. Russo, A. Santaguida)


Chandra/IXPE/DEPS2 B1509 (MSH 15-52) Sonification

IC 443 is a supernova remnant, or the debris of an exploded star, which astronomers have nicknamed the Jellyfish Nebula. A visual composite image of IC 443 includes X-rays from NASA’s Chandra X-ray Observatory (cyan) and German ROSAT X-ray telescope (blue) along with radio data from the NSF’s Very Large Array (green) and optical data from the Digitized Sky Survey (red). The sonification of IC 443 begins with a top-down scan as the brightness of the data is correlated to the volume of the sound. The sounds are mapped to colors in the image with red light being heard as lower pitches, the green as medium, and the blue light as the higher pitches. This creates notes that sweep up and down in pitch continuously. Several colors are isolated and control the volume of sustained tones with red controlling the lowest note and white controlling the highest note. The background stars in the optical image have been converted to water drop sounds in the sonification.

Credits: Images: Chandra X-ray: NASA/CXC/B.Gaensler et al; ROSAT X-ray: NASA/ROSAT/Asaoka & Aschenbach; Radio: NRC/DRAO/D.Leahy; Optical: DSS; Sonification: NASA/CXC/SAO/K.Arcand, SYSTEM Sounds (M. Russo, A. Santaguida)

Chandra/ROSAT/VLA/DSS IC 443 (Jellyfish) Sonification

The Vela Pulsar data has also been converted to sound through a process called data sonification. In this sonification, listen to a radar-like scan, clockwise from 12:00 of the image. Brightness is mapped to volume. Distance from the center is mapped to pitch (farther away is higher pitch). For the Chandra X-ray data, the bright inner region (violet) is mapped to a low synth sound, with 11 Hz oscillations matching the period of the pulsar. The dimmer outer region (blue) and jet are mapped to a wind-like sound. A long upper jet can be heard around 4 seconds in, and a bright, but much shorter lower jet can be heard around 20 seconds. For the Hubble optical data, the stars are mapped to notes on a plucked-type synth (where brighter stars are louder, and stars farther from the center are higher pitched).
Credits: Images: X-ray: NASA/CXC/SAO; Optical: NASA/ESA/STScI; Image processing: NASA/CXC/SAO/J. Schmidt, K. Arcand; Sonification: NASA/CXC/SAO/K.Arcand, SYSTEM Sounds (M. Russo, A. Santaguida)

Chandra/Hubble Vela Pulsar Sonification

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Rikki Moore. PKA Trampa has taken 2016 by the scruff of the neck. His earth shattering signature sound has drawn attention from some of the industries leading figures. Flux Pavilion, MUST DIE! and Snails to name a few. 
 
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Two of the most earnest techno acts in the scene, ARTBAT links up with Matador and his RUKUS imprint for their debut collaboration 'Apollo 11' - a direct and out of this world two-tracker named after the first successful moon landing.

The Kiev-based duo and the Irish DJ-producer have handed the title-track over to Mixmag ahead of the record's release on March 15. With its driving rhythmic elements, vigorous pads and lively arpeggiator breakdown, 'Apollo 11' is a tune that has gotten nothing but an ebullient reaction from dancefloors all around the globe.

'Apollo 11' drops on March 15 via RUKUS.

Pre-order: https://bit.ly/2XK5SAu

More exclusive music

Premiere: Matador & ARTBAT 'Apollo 11'

Get it here: http://smarturl.it/DH25Xn

Denis Horvat returns to Afterlife Recordings for a second EP of distinctive, dancefloor productions.

A year after ‘Modelo’ comes ‘Miracle Of The Rose’, an evocative and authentic development of Horvat’s sound. On ‘Noise’, the vocals of Lelah give way to a stripped-down, reverberant groove. The title track rises with a free-flowing melody before dropping a tough, angular beat. ‘Divin’ is the EP’s deepest cut, before digital only track ‘Royale’ rounds off this diverse release with flair.

Denis Horvat - Miracle Of The Rose EP (AL025)

A1 Noise feat. Lelah
B1 Miracle Of The Rose
B2 Divin
Digital only: Royale

Denis Horvat - Noise feat. Lelah

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Ableton 9 Full Project Remake (Cover)

Full Ableton 9 Instrumental Cover Template !!! (without vocals) 11 exclusive Serum Presets !!! Drums , using Simpler (Ableton Native) easy to replace . Harmonics instrument using MIDI (easy to replace) Perfect to Learn ! ALso Included Ableton Native Mastering Rack.

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11 Serum Exclusive Presets
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(Ableton REMAKE) CamelPhat, ARTBAT - For A Feeling

Adele - Rolling In The Deep (Fabrication Edit)

Credit: UC Berkeley Space Sciences Laboratory

STEREO: Solar Winds Passing by NASA Satellites

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Aphex Twin - Stone in Focus

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.