
Milky Way Enveloped in a Vast Dark Matter Plane That Shapes Local Motion
A new Nature Astronomy study using constrained, Lambda-CDM–based simulations finds the Local Group’s unseen mass is arranged not in a spherical halo but in a flattened dark matter plane tens of millions of light-years across. This geometry better reproduces the observed motions of nearby galaxies and the local Hubble flow, reducing discrepancies seen in spherical models while remaining consistent with overall cosmology. The result highlights how the dark matter around us likely forms sheets and filaments in the cosmic web, though more data is needed to pin down the plane’s thickness and orientation.





