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Astronomers Spot an Unusual Set of X-ray Light Echoes Around a Black Hole

Posted by Guy Pirro   08/06/2021 03:39PM

Astronomers Spot an Unusual Set of X-ray Light Echoes Around a Black Hole

This image features a spectacular set of rings around a black hole, captured using NASA's Chandra X-ray Observatory and Neil Gehrels Swift Observatory. The X-ray images of the giant rings reveal information about dust located in our galaxy, using a similar principle to the X-rays performed in doctor's offices and airports. In this composite image, X-rays from Chandra (light blue) were combined with optical data from the Pan-STARRS telescope in Hawaii that show the stars in the field of view. The image contains eight separate concentric rings. Each ring is created by X-rays from V404 Cygni flares observed in 2015 that reflect off different dust clouds. (Image Credit: X-ray: NASA/CXC/University of Wisconsin-Madison/S. Heinz et al.; Optical/IR: Pan-STARRS)

 


Astronomers Spot an Unusual Set of X-ray Light Echoes Around a Black Hole

V404 Cygni is a black hole binary system located about 7800 light years away from Earth. The black hole is actively pulling material away from a companion star — with about half the mass of the Sun — into a disk around the invisible object. This material glows in X-rays, so astronomers refer to these systems as "X-ray binaries." On June 5, 2015, Swift discovered a burst of X-rays from V404 Cygni. The burst created high-energy rings from a phenomenon known as light echoes. Instead of sound waves bouncing off a canyon wall, the light echoes around V404 Cygni were produced when a burst of X-rays from the black hole system bounced off of dust clouds between V404 Cygni and Earth. Cosmic dust is not like household dust but is more like smoke, and consists of tiny, solid particles.

 

 

 

A team of researchers led by Sebastian Heinz of the University of Wisconsin in Madison analyzed 50 Swift observations of the system made in 2015 between June 30 and August 25, and Chandra observations made on July 11 and 25, 2015. It was such a bright event that the operators of Chandra purposely placed V404 Cygni in between the detectors so that another bright burst would not damage the instrument.

The rings tell astronomers not only about the black hole's behavior, but also about the landscape between V404 Cygni and Earth. For example, the diameter of the rings in X-rays reveals the distances to the intervening dust clouds the light ricocheted off. If the cloud is closer to Earth, the ring appears to be larger, and vice versa. The light echoes appear as narrow rings rather than wide rings or haloes because the X-ray burst lasted only a relatively short period of time.

The researchers also used the rings to probe the properties of the dust clouds themselves. They compared the X-ray spectra — that is, the brightness of X-rays over a range of wavelengths — to computer models of dust with different compositions. Different compositions of dust will result in different amounts of the lower energy X-rays being absorbed and prevented from being detected with Chandra. This is a similar principle to how different parts of our body or our luggage absorb different amounts of X-rays, giving information about their structure and composition.

 

 

 

The team determined that the dust most likely contains mixtures of graphite and silicate grains. In addition, by analyzing the inner rings with Chandra, they found that the densities of the dust clouds are not uniform in all directions. Previous studies have assumed that they did not.

There have been multiple papers published every year reporting studies of the V404 Cygni outburst in 2015 that caused these rings. Previous outbursts were recorded in 1938, 1956 and 1989, so astronomers may still have many years to continue analyzing the 2015 one.

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.

 

 

For more information:

 

https://chandra.si.edu/photo/2021/v404cyg/

 

https://astromart.com/news/show/extreme-power-of-a-black-hole-is-revealed

 

https://astromart.com/news/show/space-telescopes-reveal-secrets-of-a-turbulent-black-hole

 

https://astromart.com/news/show/black-hole-rips-apart-a-star-that-wandered-too-close

 

https://astromart.com/news/show/chandra-finds-a-30-year-old-black-hole

 

https://astromart.com/news/show/nasas-chandra-designed-for-five-year-mission-still-going-strong-at-ten

 

https://astromart.com/news/show/how-does-one-weigh-a-supermassive-black-hole-very-carefully

 

 

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