Astronomers using the Atacama Large Millimeter/sub-millimetre Array (ALMA) have observed the emission from dust grains in the protoplanetary disk around the infant star IRS 63. Their observations revealed two ring-like and two gap-like substructures in IRS 63’s disk. This ALMA image shows young planet-forming dust rings around IRS 63. Image credit: D. Segura-Cox, Max Planck Institute for Extraterrestrial Physics. IRS 63, also known as IRAS 16285-2355,...
