Astronomers spot one of the largest spinning structures ever found in the Universe

UNDER EMBARGO UNTIL 00:01 GMT THURSDAY 04 DECEMBER 2025 / 19:01 ET WEDNESDAY 3 DECEMBER 2025

An international team led by the University of Oxford has identified one of the largest rotating structures ever reported: a “razor-thin” string of galaxies embedded in a giant spinning cosmic filament, 140 million light-years away. The findings, published today (4 December) in Monthly Notices of the Royal Astronomical Society, could offer valuable new insights into how galaxies formed in the early Universe.

Cosmic filaments are the largest known structures in the Universe: vast, thread-like formations of galaxies and dark matter that form a cosmic scaffolding. They also act as ‘highways’ along which matter and momentum flow into galaxies. Nearby filaments containing many galaxies spinning in the same direction- and where the whole structure appears to be rotating – are ideal systems to explore how galaxies gained the spin and gas they have today. They can also provide a way to test theories about how cosmic rotation builds up over tens of millions of light-years.

In the new study, the researchers found 14 nearby galaxies rich in hydrogen gas, arranged in a thin, stretched-out line about 5.5 million light-years long and 117,000 light-years wide. This structure sits inside a much larger cosmic filament containing over 280 other galaxies, and roughly 50 million light-years long. Remarkably, many of these galaxies appear to be spinning in the same direction as the filament itself- far more than if the pattern of galaxy spins was random. This challenges current models and suggests that cosmic structures may influence galaxy rotation more strongly or for longer than previously thought.

The researchers found that the galaxies on either side of the filament's spine are moving in opposite directions, suggesting that the entire structure is rotating. Using models of filament dynamics, they inferred the rotation velocity of 110 km/s and estimated the radius of the filament’s dense central region at approximately 50 kiloparsecs (about 163,000 light-years).

Co-lead author Dr Lyla Jung (Department of Physics, University of Oxford) said: "What makes this structure exceptional is not just its size, but the combination of spin alignment and rotational motion. You can liken it to the teacups ride at a theme park. Each galaxy is like a spinning teacup, but the whole platform- the cosmic filament -is rotating too. This dual motion gives us rare insight into how galaxies gain their spin from the larger structures they live in.”

The filament appears to be a young, relatively undisturbed structure. Its large number of gas-rich galaxies and low internal motion - a so-called “dynamically cold” state - suggest it’s still in an early stage of development. Since hydrogen is the raw material for star formation, galaxies that contain much hydrogen gas are actively gathering or retaining fuel to form stars. Studying these galaxies can therefore give a window into early or ongoing stages of galaxy evolution.

Hydrogen-rich galaxies are also excellent tracers of gas flow along cosmic filaments. Because atomic hydrogen is more easily disturbed by motion, its presence helps reveal how gas is funnelled through filaments into galaxies -offering clues about how angular momentum flows through the cosmic web to influence galaxy morphology, spin, and star formation.

The discovery could also inform future efforts to model intrinsic alignments of galaxies, a potential contaminant in upcoming weak lensing cosmology surveys with European Space Agency's Euclid mission and the Vera C. Rubin Observatory in Chile.

Co-lead author Dr Madalina Tudorache (Institute of Astronomy, University of Cambridge / Department of Physics, University of Oxford) added: "This filament is a fossil record of cosmic flows. It helps us piece together how galaxies acquire their spin and grow over time."

The international team used data from South Africa’s MeerKAT radio telescope, one of the world’s most powerful telescopes, comprising an array of 64 interlinked satellite dishes. This spinning filament was discovered using a deep survey of the sky called MIGHTEE, which is led by Professor of Astrophysics Matt Jarvis (Department of Physics, University of Oxford). This was combined with optical observations from the Dark Energy Spectroscopic Instrument (DESI) and Sloan Digital Sky Survey (SDSS) to reveal a cosmic filament exhibiting both coherent galaxy spin alignment and bulk rotation.

Professor Jarvis said: “This really demonstrates the power of combining data from different observatories to obtain greater insights into how large structures and galaxies form in the Universe. Such studies can only be achieved by large groups with diverse skillsets, and in this case, it was really made possible by winning an ERC Advanced Grant/UKIR Frontiers Research Grant, which funded the co-lead authors.”

The study also involved researchers from University of Cambridge University of the Western Cape Rhodes University, South African Radio Astronomy Observatory, University of Hertfordshire, University of Bristol, University of Edinburgh, and University of Cape Town.

Notes to editors:

For media enquiries and interview request, contact:

• Madalina N. Tudorache (University of Cambridge/Oxford) — madalina.tudorache@ast.cam.ac.uk
• Lyla S. Jung (University of Oxford) —lyla.jung@physics.ox.ac.uk
• Matt Jarvis (University of Oxford/University of the Western Cape) matt.jarvis@physics.ox.ac.uk

The paper ‘A 15 Mpc rotating galaxy filament at redshift 𝑧 = 0.032’ will be published in Monthly Notices of the Royal Astronomical Society at 00:01 GMT Thursday 4 December / 19:01 ET Wednesday 3 December 2025 at https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/staf2005 . To view a copy of the paper before this under embargo, please contact the researchers listed above. 

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