Radio observatories detect hidden gas shielding record-breaking space blast

The study explains the absence of expected chemical signatures in the brightest known LFBOT.
PUBLISHED JAN 13, 2026
A new, extremely LFBOT AT2024wpp, flares as a bright blue point of light in the left panel, while the right panel shows the same region of sky after the outburst faded (Cover Image Source: Astrophysics Research Institute)
A new, extremely LFBOT AT2024wpp, flares as a bright blue point of light in the left panel, while the right panel shows the same region of sky after the outburst faded (Cover Image Source: Astrophysics Research Institute)

With a network of high-powered radio telescopes, scientists have discovered a giant "cocoon" of gas surrounding one of the most explosive events ever recorded in space. This cocoon was making one of the brightest events in the universe appear to be missing key chemical signatures, according to the National Radio Astronomy Observatory



The object, now officially known as AT2024wpp and unofficially dubbed "the Whippet," is a member of the rare and not-so-well-understood class of space explosions termed Luminous Fast Blue Optical Transients, or LFBOTs. They are bright enough to outshine about 100 billion Suns but vanish in a matter of days before most telescopes can react. The Whippet is especially significant among these since it is the brightest known LFBOT discovered yet. 

This is an artist's concept of one of brightest explosions ever seen in space. Called a Luminous Fast Blue Optical Transient (LFBOT) (Image Source: NASA, ESA, NSF's NOIRLab, Mark Garlick , Mahdi Zamani)
This is an artist's concept of one of brightest explosions ever seen in space. Called a Luminous Fast Blue Optical Transient (LFBOT) (Image Source: NASA, ESA, NSF's NOIRLab, Mark Garlick, Mahdi Zamani)

The Whippet was first spotted in September 2024 by the Zwicky Transient Facility. Initial follow-up data from NASA’s Swift satellite and the Liverpool Telescope revealed that the blast was scorching hot and churning out intense X-rays, but scientists were scratching their heads about what they weren’t seeing. During an LFBOT explosion, the debris should slam into surrounding gas, creating distinctive chemical "fingerprints" in ultraviolet and optical light.

In the Whippet's case, those signatures could not be detected even with the Hubble Space Telescope. The space around the explosion looked empty, even though theory said that it should be crowded with stellar debris. Ultimately, the mystery was solved by the National Science Foundation's Very Large Array (VLA) and Atacama Large Millimeter/submillimeter Array (ALMA). These radio telescopes do not depend on light signatures; instead, they can follow shock waves.

Like a celestial blanket the Milky Way forms an arc high above the antennas of the Atacama Large Millimeter/submillimeter Array (Image Source: ALMA Observatory)
Like a celestial blanket the Milky Way forms an arc high above the antennas of the Atacama Large Millimeter/submillimeter Array (Image Source: ALMA Observatory)

The radio data revealed a shock wave that charged outward at 20% of the speed of light, which had then struck a dense pocket of gas located very close to the explosion. Immediately, the scientists realized that the gas had never disappeared—the explosion's own power had simply cloaked it. The X-rays produced by the blast were so intense that they stripped electrons off the nearby gas. This ionization effectively erased the chemical fingerprints that optical and ultraviolet telescopes usually detect.

The researchers recreated the Whippet's last moments by merging data from various light spectrums. They think a nearby star was consumed by a massive black hole, which is what caused the explosion. The star started to lose its outer layers as the black hole spiraled toward its victim, producing a dense gas bubble. After the core was torn apart, its debris arranged itself into a hot disk that acted as the black hole's food. This feeding frenzy produced a strong wind that collided with the gas that had previously been shed, lighting it up from radio to X-rays. Later observations from Keck, Magellan, and even the Very Large Telescope revealed faint traces of hydrogen and helium traveling at 6,000 km/s. This suggests that a dense structure survived the initial blast. 

More on Starlust

Record-breaking, wobbling black hole jets are starving a nearby galaxy of stars

Astronomers surprised to witness a young star's jet backfire, triggering dramatic cosmic explosion

MORE STORIES

Relying on 50 years of data, the study has identified two potential danger windows till mid-2027.
19 hours ago
The study observed the activity of tardigrades, or 'water bears,' in Martian soil simulations.
19 hours ago
The revelations from the image will help understand how stars are born and die in the most extreme region of the galaxy.
4 days ago
Future Artemis missions could test the hypothesis proposed by the new study.
4 days ago
NASA's Chandra X-ray Observatory has captured images of the astrosphere around the young star HD 61005 for the first time.
5 days ago
New close-ups reveal mineral ridges and nodules that point to a wet past on the Red Planet.
5 days ago
It is a stunning discovery since the planet and the moon have different atmospheric conditions.
6 days ago
Future human missions can target the vicinity of the volcano to set foot on the Red Planet.
7 days ago
Researchers explore cool flames, spherical fires, and new methods aimed at making spacecraft safer.
7 days ago
The light from the rare galaxy has challenged conceptions of what the universe would have been like in the early stages.
Feb 20, 2026