
This image shows the protoplanetary disc surrounding the young star HL Tauri, revealing substructures within the disc that have never been seen before. It even shows the possible positions of planets forming in the dark patches within the system. Image credit: ALMA (ESO/NAOJ/NRAO).
For a long time the formation of protostellar disks has defied theoretical astrophysicists. In a dense, collapsing cloud of gas and dust, the magnetic field would be dragged to the centre as well resulting in a braking effect. Hardly any rotationally supported disk can form this way, unless tiny grains are removed from the cloud by growing or coagulating into bigger grains. This is the result from a new study at Max Planck Institute for Extraterrestrial Physics and other intuitions...
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