Ancient Explosion Left a Bubble in Space express

Original: "An unusual pair of interstellar HI features and a related white dwarf star inside the HI cavity surrounding the Upper Sco-Cen OB2 Association"
· Gerrit L. Verschuur
arXiv:2602.08756 · 2026-02-09 · CC0 1.0 · 1 min
Two mysterious gas structures found near a dim star — possibly the cooled remnant of a planetary nebula.

📄 Showing the "Simple" version — "Popular" is not ready yet. Add it to favorites to help prioritize it.

In radio sky data, like on old photographic film, two bright gas streaks have emerged. They move at different speeds but hang near the same dim star. The star and the streaks turned out to be inside a huge empty bubble in the interstellar gas. This bubble is like a blown soap bubble left over from an ancient supernova explosion.

A bubble in interstellar gas is a region where there is almost no gas: the supernova blast swept it aside, like a shock wave pushing leaves.

The gas streaks are most likely remnants of a planetary nebula — the shell shed by a dying star. Usually such shells quickly dissipate into the surrounding gas. Here they survived because they expanded into the nearly empty space of the bubble. Over 300,000 years, the gas cooled, became neutral, and began emitting radio waves at a wavelength of 21 centimeters.

An age of 300,000 years is about 15 times longer than the entire history of human civilization.

So an ancient explosion inadvertently preserved for us the traces of another, more modest stellar death. The bubble acted as a museum display case: without it, the gas would have long since mixed with the interstellar medium.

Radio waves at a wavelength of 21 centimeters are emitted by neutral hydrogen — the most abundant element in the universe. It is through this radiation that astronomers see cold gas invisible to ordinary telescopes.

Scientists
Alan GuthAlexander FriedmannAndrei LindeGeorges LemaîtreJames PeeblesAdam Riess
Concepts
cold gas interstellar object galactic halo composition galactic halo interstellar space young stellar object nebula open cluster star formation regions hills mechanism white dwarf helium star pair instability supernova stellar nursery intermediate mass black hole asteroid belt supernova remnant formation pulsar wind nebula quasistar super earth