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This newfound fast radio burst challenges what astronomers know about the powerful astronomical phenomena

Fast radio burst: Radio telescope in New Mexico
Researchers used a radio telescope in New Mexico to study a particularly interesting fast radio burst. (Image credit: Diana Robinson/Flickr, CC BY-NC-ND)

This article was originally published at The Conversation (opens in new tab). The publication contributed the article to Space.com's Expert Voices: Op-Ed & Insights.

Kshitij Aggarwal (opens in new tab), Affiliate Researcher in Astronomy and Astrophysics, West Virginia University

A newly discovered fast radio burst has some unique properties that are simultaneously giving astronomers important clues into what may cause these mysterious astronomical phenomena while also calling into question one of the few things scientists thought they knew about these powerful flares, as my colleagues and I describe in a new study (opens in new tab) in Nature on June 8, 2022.

Fast radio bursts, or FRBs, are extremely bright pulses of radio waves that come from faraway galaxies. They release as much energy in a millisecond as the sun does over many days (opens in new tab). Researchers here at West Virginia University detected the first FRB back in 2007 (opens in new tab). In the past 15 years, astronomers have detected around 800 FRBs, with more being discovered every day (opens in new tab).

Related: 'Weird signal' hails from the Milky Way. What's causing it?

When a telescope captures an FRB, one of the most important features researchers look at is something called dispersion. Dispersion is basically a measure of how stretched out an FRB is when it reaches Earth.

The plasma that lies between stars and galaxies causes all light — including radio waves — to slow down, but lower frequencies feel this effect more strongly and slow down more than higher frequencies. FRBs contain a range of frequencies, so the higher frequency light in the burst hits Earth before the lower frequencies, causing the dispersion. This allows researchers to use dispersion to estimate how far from Earth an FRB originated (opens in new tab). The more stretched out an FRB is, the more plasma the signal must have passed through, the farther away the source must be.

Why it matters

The new FRB my colleagues and I discovered is named FRB190520 (opens in new tab). We found it using the Five-hundred-meter Aperture Spherical Telescope (opens in new tab) in China. An immediately apparent interesting thing about FRB190520 was that it is one of the only 24 repeating FRBs and repeats much more frequently than others — producing 75 bursts over a span of six months in 2020.

Our team then used the Very Large Array (opens in new tab), a radio telescope in New Mexico, to further study this FRB and successfully pinpointed the location of its source — a dwarf galaxy roughly 3 billion light years from Earth. It was then that we started to realize how truly unique and important this FRB is.

First, we found that there is a persistent, though much fainter, radio signal being emitted (opens in new tab) by something from the same place that FRB190520 came from. Of the more than 800 FRBs discovered to date (opens in new tab), only one other has a similar persistent radio signal.

Second, since we were able to pinpoint that the FRB came from a dwarf galaxy, we were able to determine exactly how far away that galaxy is from Earth. But this result didn't make sense. Much to our surprise, the distance estimate we made using the dispersion of the FRB was 30 billion light years from Earth, a distance 10 times larger than the actual 3 billion light years to the galaxy (opens in new tab).

Astronomers have only been able to pinpoint the exact location — and therefore distance from Earth — of 19 other FRB sources (opens in new tab). For the rest of the roughly 800 known FRBs, astronomers have to rely on dispersion alone to estimate their distance from Earth. For the other 19 FRBs with known locations, the distances estimated from dispersion are very similar to the real distances to their source galaxies. But this new FRB shows that estimates using dispersion can sometimes be incorrect and throws many assumptions out the window.

The top of this diagram show six spikes in radio wave brightness that are six bursts from FRB190520. The bottom half shows the frequency range for each individual burst. (Image credit: Niu, CH., Aggarwal, K., Li, D. et al., CC BY)

What still isn't known

Astronomers in this new field (opens in new tab) still don't know what exactly produces FRBs (opens in new tab), so every new discovery or piece of information is important.

Our new discovery raises specific questions, including whether persistent radio signals are common, what conditions produce them and whether the same phenomenon that produces FRBs is responsible for emitting the persistent radio signal.

And a huge mystery is why the dispersion of FRB190520 was so much greater than it should be. Was it due to something near the FRB? Was it related to the persistent radio source? Does it have to do with the matter in the galaxy where this FRB comes from? All of these questions are unanswered.

What's next

My colleagues are going to focus in on studying FRB190520 using a host of different telescopes around the world. By studying the FRB, its galaxy and the space environment surrounding its source, we are hoping to find answers to many of the mysteries it revealed.

More answers will come from other FRB discoveries in the coming years, too. The more FRBs astronomers catalog, the greater the chances of discovering FRBs with interesting properties that can help complete the puzzle of these fascinating astronomical phenomena.

This article is republished from The Conversation (opens in new tab) under a Creative Commons license. Read the original article (opens in new tab).

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Kshitij is an Affiliate Researcher in Astronomy and Astrophysics at West Virginia University. His research focuses on the study of Fast Radio Bursts (FRBs). He uses machine learning to efficiently search for and classify FRBs from noise. Kshitij is part of the Realfast collaboration, which performs real-time FRB search and localization using Very Large Array in New Mexico. He also contributes towards many open source softwares for FRB data analysis.