Galactic Sneeze: Bubbles from a Black Hole express

Original: "Southern eROSITA bubble as a forward shock and the low-metallicity CGM. South-east side story"
arXiv:2603.20740 · 2026-03-21 · CC BY 4.0 · 1 min
The eROSITA X-ray telescope captured a shock wave left behind by a 'sneeze' from the supermassive black hole at the center of the Milky Way.

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

In 2020, the eROSITA X-ray telescope discovered a pair of enormous bubbles looming above and below the disk of our Galaxy. These clouds of gas heated to millions of degrees are the aftermath of a colossal energy release from the center.

That's what a shock wave from a galactic-scale sneeze might look like: a few million years ago, the supermassive black hole 'sneezed' out matter, blowing these bubbles.

Astronomers examined the southeastern edge of one bubble, where matter slams into the sparse background. By breaking X-ray light into colors with spectroscopy, they found the shock wave racing at 700 km/s, surrounded by a near-vacuum: the gas is mostly hydrogen, with less than 10% of the heavy elements found in the Sun. Although the gas is scorching, an astronaut inside wouldn't feel the heat — the density is trillions of times lower than air, and particles zip by hardly colliding. This shock wave acts as a natural particle accelerator: it revs up particles to such speeds that they become cosmic rays bombarding Earth. Understanding these bubbles links the history of the galaxy to the mystery of the most energetic particles in the universe.

The shock wave's speed (700 km/s) is such that it could travel from Earth to the Moon in 9 minutes.

Scientists
Roger PenroseSubrahmanyan ChandrasekharMargaret BurbidgeAdam RiessJohn Archibald WheelerMaarten Schmidt
Concepts
erosita bubble gamma-ray burst age of the universe asteroid belt starburst observable universe solar corona Westerly wind burst