A Spinning Top at the Galaxy’s Core Snuffs Out Stars ✎ express

Original: "A precessing jet from an active galactic nucleus drives gas outflow from a disk galaxy"
arXiv:2601.08791v1 · 2026-01-13 · arXiv non-exclusive · independent analysis · 1 min
A wobbling black hole ejects gas, robbing the galaxy of new stars.

At the center of the galaxy VV 340a lurks a supermassive black hole. It spews a jet of matter that doesn’t fly straight but wobbles, like the axis of a slowing spinning top. One full wobble takes about 820,000 years. The reason: the material falling onto the black hole is unevenly twisted, so it rotates in jerks.

This swaying whirlwind pushes superheated gas out of the galaxy: each year, roughly 19 solar masses escape. The hydrogen in it is so hot that it glows, and that glow lets spectral analysis measure the gas speed. It turns out the gas travels thousands of light-years away.

The most surprising part: this black hole is far from a power record-holder. Its jet is dozens of times weaker than those of quasars, but even this gentle “breath” is enough to freeze star formation in an entire galaxy.

The gas swept out by the jet is the raw material for stars. Without it, star formation sputters out. So a relatively modest black hole governs the life of a huge stellar system.

In one full wobble cycle, the jet ejects about 16 million solar masses — more than the mass of many globular star clusters.

Scientists
Stephen HawkingJacob BekensteinFritz ZwickyBernhard RiemannJoseph WeberKarl Schwarzschild
Concepts
galactic outflow active galaxy relativistic jets starburst jet ultra fast outflow galactic winds star formation gas quasar feedback black hole feedback gas accretion supernova jets seyfert galaxy microquasar star black hole wind accretion disk wind m87 protoplanetary disk blazar