Galaxies on the Scale express

Original: "Fast rotations in galaxies at cosmic noon indicate central concentration of stars, dark matter or massive black holes"
arXiv:2601.03338 · 2026-01-06 · CC BY 4.0 · 1 min
Astronomers weighed three distant galaxies and found something unexpectedly heavy at their cores.

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Three distant galaxies spin like giant carousels. Their stars and gas move along spiral arms, and from the speed of this motion you can calculate how much total matter the galaxy contains — visible and invisible.

Astronomers combined two views: radio telescopes revealed cold gas, while the James Webb Space Telescope showed the stars. This allowed them to precisely measure how these three galaxies rotate. The outer parts spin as expected. But right at the center, the speed turned out to be higher than calculated. As if the carousel were spinning faster near its axis than it should be for its mass.

This discrepancy could mean that extra mass is hiding in the galactic cores: either black holes heavier than usual, or dark matter packed into a dense clump.

It is not yet clear which explanation is correct. But the very fact that we can peer into the center of a galaxy billions of light-years away and notice such a 'shortfall' in our calculations is a step toward understanding how the invisible part of the Universe is structured.

The James Webb Space Telescope sees in infrared light, so dust that hides the galactic center from ordinary telescopes does not bother it.

Scientists
Fritz ZwickyVera RubinSubrahmanyan ChandrasekharChristian DopplerAdam RiessJohn Archibald Wheeler
Concepts
galactic kinematics mass distribution galactic disk modified gravity vs dark matter vera rubin galaxy rotation galaxy rotation curve dark matter halo structure stellar motion gas disk density profile halo stellar orbit dust ring black hole dynamics gravitational lensing analysis cosmic dust black hole mass gap three dimensional map milky way