'Dark' and Powerful Space Explosions May Be Cloaked by Cosmic Dust (Video, Images)

Gamma-Ray Burst Buried in Dust
Artist's impression of a gamma-ray burst buried in dust. (Image credit: NAOJ)

Astronomers using a giant radio telescope to investigate the most violent explosions in the universe, known as gamma-ray bursts (GRBs), found something surprising in two distant galaxies: more dust and less gas than they expected.

So-called "dark GRBs" may explain a curious phenomenon for astronomers mapping out these powerful explosions in space. While most gamma-ray bursts have an afterglow, sometimes scientists don't see that luminescence. It is possible that thick interstellar dust may mask the light from dark GRBs.

The new gamma-ray burst observations were collected by the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile, which revealed substantial amounts of molecular gas in the centers of two target galaxies. The observed GRBs took places in galactic zones that had little gas, but a lot of dust. [See a video about the dark gamma-ray bursts]

"We didn't expect that GRBs would occur in such a dusty environment with a low ratio of molecular gas to dust. This indicates that the GRB occurred in an environment quite different from a typical star-forming region," Bunyo Hatsukade, the lead scientist who performed the research with the National Astronomical Observatory of Japan, said in a statement.

Observations of galaxy GRB 020819B of molecular gas (left) and dust (middle) done by the Atacama Large Millimeter/submillimeter Array (ALMA). At right is a visible-light image from the Frederick C. Gillett Gemini North Telescope. The cross indicates the site of a gamma-ray burst in the region. (Image credit: Bunyo Hatsukade(NAOJ), ALMA (ESO/NAOJ/NRAO))

Brief bursts of energy

While telescopes have observed gamma rays for decades, less is known about gamma-ray bursts. Brief GRBs (they last less than two seconds) may be produced as two neutron stars collide. Longer bursts might happen when massive stars go supernova, collapse into black holes, and send out a surge of energy.

Usually, a burst will send out as much energy as the sun will during its 10 billion-year lifetime. The accompanying afterglow is believed to happen after the thrown-off material crashes into the gas surrounding the explosion.

Artist's conception of the environment around GRB 020819B. (Image credit: NAOJ)

ALMA's results add to a growing stream of observations astronomers are making of the galaxies where these bursts originate. They believed the huge stars could be lurking in star-forming areas within the galaxies, which these latest results appear to contradict.

The bursts might alter the environment, though. Dust would remain after the explosion because it's more robust than the gas, the astronomers suggested. Ultraviolet radiation from the explosion would break apart the bonds in the molecular gas.

ALMA also made the first detection of carbon monoxide gas in a host galaxy. The array's dozens of telescopes are providing higher-resolution observations in radio and submillimeter wavelengths than ever seen before, its backers say.

The astronomers added that more observations will be needed to better generalize what a GRB site looks like. Results were published this week in the journal Nature.

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Elizabeth Howell
Staff Writer, Spaceflight

Elizabeth Howell (she/her), Ph.D., is a staff writer in the spaceflight channel since 2022 covering diversity, education and gaming as well. She was contributing writer for Space.com for 10 years before joining full-time. Elizabeth's reporting includes multiple exclusives with the White House and Office of the Vice-President of the United States, an exclusive conversation with aspiring space tourist (and NSYNC bassist) Lance Bass, speaking several times with the International Space Station, witnessing five human spaceflight launches on two continents, flying parabolic, working inside a spacesuit, and participating in a simulated Mars mission. Her latest book, "Why Am I Taller?", is co-written with astronaut Dave Williams. Elizabeth holds a Ph.D. and M.Sc. in Space Studies from the University of North Dakota, a Bachelor of Journalism from Canada's Carleton University and a Bachelor of History from Canada's Athabasca University. Elizabeth is also a post-secondary instructor in communications and science at several institutions since 2015; her experience includes developing and teaching an astronomy course at Canada's Algonquin College (with Indigenous content as well) to more than 1,000 students since 2020. Elizabeth first got interested in space after watching the movie Apollo 13 in 1996, and still wants to be an astronaut someday. Mastodon: https://qoto.org/@howellspace