Interstellar Comets vs. Dark Matter express

Original: "Contribution of interstellar objects to local dark matter density"
arXiv:2605.04801 · 2026-05-06 · CC BY 4.0 · 1 min
Accounting for interstellar comets changes the estimated amount of dark matter around us.

Recently, astronomers spotted three interstellar comets coming from deep space. One of them, 3I/ATLAS, turned out to be unexpectedly large: its nucleus is several kilometers across. This got scientists thinking: there might be countless such icy wanderers throughout the Galaxy, with a combined mass comparable to all visible stars combined, around 50 billion solar masses.

This much ordinary matter changes the picture of mass distribution. For a long time, the fast rotation of galaxies was explained by the presence of invisible dark matter, a hypothesis proposed by Fritz Zwicky and confirmed by observations by Vera Rubin. But now there's an alternative: we simply overlook a huge amount of ordinary objects, like weighing a bag without realizing it's stuffed with thick books. The weight seems to appear from nowhere, but it's actually hidden in plain sight.

New calculations suggest that the density of dark matter near the Sun could be almost half of previous estimates. To be fair, explaining all rotation with just comets would require an absurdly large number. But the discovery itself is a reminder: we still have a poor idea of how much ordinary matter lurks in the interstellar darkness. And these comets themselves are time travelers: unchanged for billions of years, they even witnessed the birth of our Sun.

Some interstellar comets, like 3I/ATLAS, have been wandering the Galaxy almost since its birth: their age rivals that of the Milky Way itself.

This concept is reminiscent of Arthur C. Clarke's 'Rendezvous with Rama,' only with giant comets wandering for millions of years instead of an alien spaceship.

Scientists
Fritz ZwickyMichael FaradayHendrik LorentzEmile ClapeyronIsaac NewtonJohn Michell
Concepts
interstellar object solar mass matter density young stellar object interstellar medium intermediate mass black hole galactic halo galactic halo composition innermost stable circular orbit dust black hole dark matter interaction asteroid belt cold gas dust obscuration donor star host galaxy asteroid stellar objects infrared excess gas disk