A new sonification turns X-ray “light echoes” from a black hole into sound. Rings of X-rays seen by NASA’s Chandra and Swift observatories show the echoes. Material around a black hole can generate bursts of X-rays. The X-rays reflect off clouds of gas and dust like beams from headlights can in fog. Credits: NASA/CXC/A. Hobart
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.
The sonification of V404 Cygni translates the X-ray data from both Chandra
and Swift into sound. During the sonification, the cursor moves outward from
the center of the image in a circle. As it passes through the light echoes
detected in X-rays (seen as concentric rings in blue by Chandra and red by
Swift in the image), there are tick-like sounds and changes in volume to denote
the detection of X-rays and the variations in brightness. To differentiate
between the data from the two telescopes, Chandra data is represented by
higher-frequency tones while the Swift data is lower. In addition to the
X-rays, the image includes optical data from the Digitized Sky Survey that
shows background stars. Each star in optical light triggers a musical note. The
volume and pitch of the note are determined by the brightness of the star.
More sonifications of astronomical data, as well as additional information
on the process, can be found at the "A Universe of Sound"
website: https://chandra.si.edu/sound/
These sonifications were led by the Chandra X-ray Center (CXC) and included
as part of NASA's Universe of Learning (UoL) program. The collaboration was driven by visualization
scientist Kimberly Arcand (CXC), astrophysicist Matt Russo, and musician Andrew
Santaguida (both of the SYSTEM Sounds project). NASA's Marshall Space Flight
Center manages the Chandra program. The Smithsonian Astrophysical Observatory's
Chandra X-ray Center controls science from Cambridge Massachusetts and flight operations
from Burlington, Massachusetts. NASA's Universe of Learning materials are based
upon work supported by NASA under cooperative agreement award number NNX16AC65A
to the Space Telescope Science Institute, working in partnership with
Caltech/IPAC, Center for Astrophysics | Harvard & Smithsonian, and the Jet
Propulsion Laboratory.
Read more from NASA's Chandra
X-ray Observatory.
For more Chandra images, multimedia and related materials, visit: http://www.nasa.gov/chandra
Megan Watzke
Chandra X-ray Center, Cambridge, Massachusetts
Source: 'Listen' to the Light Echoes From a Black Hole | NASA