How Fast Is the Black Hole at the Milky Way's Center Growing? express

Original: "Milky Way evolution on a human timescale"
· Eugene, Neige
arXiv:2603.29503 · 2026-03-31 · CC BY 4.0 · 1 min
Three key traits of our Galaxy shifted in just a few decades.

Other galaxies are just ancient snapshots, but we watch the Milky Way live. Comparing data over 30 years, scientists found that the Galaxy’s center is, like, speeding up: the supermassive black hole got heavier, swallowing the mass of a large asteroid each year; the stellar bar (a huge beam of billions of suns, like the crossbar of a merry-go-round) started spinning 5% faster; and the Sun moved closer to the axis: we’re 1,700 light-years nearer to the center than we thought.

These changes are linked. Perhaps more gas is flowing into the Galaxy’s core, or dark matter (the invisible framework that holds stars together) is altering the celestial mechanics. The whole system behaves like a mechanism come to life, with gears suddenly spinning faster. If you watched our star city from the outside, the bar’s acceleration would be noticeable within the span of a single movie: that’s how rapid it is.

The distance from the Sun to the center of the Galaxy was long thought to be 27,700 light-years, but modern measurements have refined it to 26,000 light-years: we turned out to be a couple thousand light-years closer to the heart of the Milky Way.

In *Interstellar*, Gargantua seemed eternal, but real black holes grow even while you’re watching the movie.

Scientists
Adam RiessBrian SchmidtEdwin HubbleGeorges LemaîtreMaarten SchmidtSaul Perlmutter
Concepts
galactic evolution processes milky way galaxy formation supermassive black hole formation cosmology galactic bulge galaxy distribution stellar evolution early universe galaxies age of the universe cosmic expansion starburst cosmic acceleration deceleration stellar orbit supermassive black hole growth milky way halo structure dark matter halo structure solar system three dimensional map planetary system