Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have finally found clear evidence that the supermassive black hole at the center of the Milky Way, Sagittarius A*(Sgr A*), is blowing a hot cosmic wind – something scientists have been hunting for over 50 years.
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New type of Fast Radio Burst discovered in Green Bank Telescope data
Artist’s impression of the discovery of microsecond Fast Radio Bursts being observed by the Green Bank Telescope. Incoming radio waves are shown as white, red, and orange streaks that follow each other in rapid succession. The long red streaks are the previously known millisecond flashes. (c) Daniëlle Futselaar/www.artsource.nl
An international team of researchers have discovered radio pulses from the distant universe that last only millionths of a second. They found these microsecond bursts after a meticulous examination of archival data from the National Science Foundation’s Green Bank Telescope. It’s unclear how the ultrafast bursts were created. The researchers published their findings in Nature Astronomy.
Fast radio bursts (FRBs) are unpredictable, extremely short flashes of radio waves far beyond our Milky Way. They are possibly caused by magnetic neutron stars, also known as magnetars. The first bursts were discovered in 2007. So far, most bursts last longer than a thousandth of a second and emit as much energy as our sun generates in a day.
In 2022, researchers at the University of Amsterdam and ASTRON hypothesized that there might be bursts that would last not thousandths, but only millionths of a second. “During our group meetings, we often talked about it”, says Mark Snelders, PhD candidate at ASTRON and the University of Amsterdam (the Netherlands), who was in charge of the research that uncovered the ultra-fast radio bursts. “By coincidence, I found out that there was a public dataset that we could use for this.”
Watch a presentation by Mark for the Green Bank Observatory about this science.
Five hours of data – and millions of images
The researchers accessed the public data archive from the Breakthrough Listen project, which uses the Green Bank Telescope to search for extraterrestrial life. They focused on five hours of data from FRB 20121102A, located some three billion light years away, towards the Auriga constellation.
The researchers divided each second of the first thirty minutes of data into half a million individual images. Next, they used software filters and machine learning to search for outliers. Through this meticulous process, they discovered eight ultra-fast bursts that lasted only ten millionths of a second or less.
Now that the first ultra-fast microsecond source has been detected, researchers expect to find more. However, finding them may be easier said than done, as some data files are not detailed enough to cut into half a million pieces per second.
The Green Bank Observatory is supported by the National Science Foundation and is operated by Associated Universities, Inc.
Read more at the Netherlands Research School for Astronomy.
Media Contact:
Jill Malusky, NRAO & GBO News & Public Information Manager
[email protected]
This news article was originally published on the GBO website on October 19, 2023.
Recent News
Milky Way’s Black Hole Finally Caught ‘Breathing’
Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have finally found clear evidence that the supermassive black hole at the center of the Milky Way, Sagittarius A*(Sgr A*), is blowing a hot cosmic wind – something scientists have been hunting for over 50 years.
AUI Announces 2026 Scholarship Recipients
Ten high school students have been awarded for academic achievement, community involvement and leadership skills.
NSF NRAO Leads Future of U.S. Radio Astronomy with First Light from Next Generation Very Large Array Prototype
The proposed array’s design will improve on the sensitivity and spatial resolution—with 10 times the effective collecting area and resolution—over the current NSF VLA and the Atacama Large Millimeter/submillimeter Array at the same wavelengths.