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Oxford-Led Team Finds Rotating, Razor-Thin Cosmic Filament in the Nearby Universe

The peer-reviewed analysis infers a 110 km/s twist, offering a rare test of how the cosmic web feeds galaxies.

Overview

  • Researchers report one of the longest rotating filaments yet detected, with coherent spin alignment across a razor-thin core of 14 hydrogen-rich galaxies.
  • MeerKAT’s MIGHTEE radio survey, paired with DESI and SDSS data, mapped a 5.5-million–light-year core embedded within an extended structure of more than 280 galaxies spanning roughly 50 million light-years.
  • Galaxy redshifts show opposite motions on either side of the filament’s spine, consistent with bulk rotation modeled at about 110 km/s.
  • The filament appears hydrogen-rich and dynamically cold, indicating a relatively young, undisturbed environment that can channel gas to fuel star formation.
  • The finding bears on theories of angular-momentum transfer and intrinsic-alignment modeling for future weak-lensing surveys, while coverage differs on its distance estimate (about 140 vs 440 million light-years).