Overview
- The structure lies about 140 million light-years away and hosts roughly 280–300 galaxies within a thread about 117,000 light-years wide.
- Kinematic modeling shows galaxies on opposite sides move in opposing directions, implying bulk rotation at about 110 km/s.
- Within the filament, astronomers traced a razor-thin line of 14 hydrogen-rich galaxies stretching about 5.5 million light-years.
- The system appears young and relatively undisturbed, with coherent spin alignments and abundant neutral hydrogen pointing to ongoing gas inflow and star formation.
- The findings, reported in MNRAS by a team led by Lyla Jung and Madalina Tudorache, rely on MeerKAT MIGHTEE radio data combined with DESI and SDSS spectroscopy and motivate deeper multi-wavelength surveys to test how common such rotation is.