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Invisible Object Weighing a Million Suns: Gravity Acts as a Magnifying Glass ⚡ экспресс

Original: "A million-solar-mass object detected at cosmological distance using gravitational imaging"
arXiv:2510.07382 · 2025-10-08 · CC BY · ⏱ 1 min · Cosmology Galaxies
Astronomers have measured the mass of an invisible object weighing a million Suns for the first time by how it distorts light from a distant galaxy.
Abstract

Studying subgalactic-scale structures is crucial for testing galaxy formation models and the nature of dark matter, yet such objects are usually too faint for reliable mass estimates. Using Very Long Baseline Interferometry (VLBI) with milliarcsecond resolution, an extremely low-mass object has been detected perturbing a thin gravitationally lensed arc. The object was identified via non-parametric gravitational imaging and confirmed by independent parametric modeling. Its mass within a projected radius of 80 parsecs, assuming a redshift of 0.881, is (1.13±0.04)×10⁶ M☉, with a statistical significance of 26σ, a relative mass uncertainty of 3.3%, and an astrometric uncertainty of 194 microarcseconds. This is the lightest object known at cosmological distances by its gravitational influence — two orders of magnitude lighter than previous finds. The result demonstrates the practical feasibility of probing the million-solar-mass range far beyond the Local Universe through gravitational imaging methods.

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Astronomers have found an invisible object in the Universe weighing just a million Suns — for cosmic scales, that’s a mere trifle, a hundred times lighter than anything they’ve been able to “weigh” at such distances. The object itself doesn’t shine, but it gave itself away by bending the light from an even more distant galaxy. Massive bodies, as Einstein showed, warp spacetime and act like lenses: just as a transparent bead on a window distorts the outline of a streetlamp.

In this case, the invisible object became that bead.

Its position was determined with precision that could spot a coin on the Moon, and its mass with an error margin of just 3%.

It’s likely either a faint dwarf galaxy, almost devoid of stars, or a clump of dark matter — that enigmatic substance first suspected after the observations of Vera Rubin. Catching such invisible things means probing the hidden scaffolding of the Universe and understanding how giant galaxies like our Milky Way grew.

🎯 This object’s mass — roughly a million Suns — is a drop in the ocean by cosmic standards. For comparison, the Milky Way is a million times heavier, weighing in at about a trillion Suns.

Scientists
Albert EinsteinFritz ZwickyVera RubinRobert H. DickeJosef LenseWilliam Unruh
Tags
dark matter galaxy spacetime curvature
Laws
gravitational lensingequivalence principlevirial theoremLense–Thirring effectUnruh effectAdS/CFT correspondence
Original: arXiv:2510.07382 · CC BY · bridge42worlds