space blog

Ever wonder how stars and planets form? New clues have been found in the protoplanetary system Herbig-Haro 30 by the James Webb Space Telescope, Hubble and the Earth-bound telescope ALMA. The observations show, that large dust grains are more concentrated into a central disk where they can form planets. The featured image from Webb shows many attributes of the HH-30 system. Jets of particles are being expelled vertically, shown in red, while a dark dust-rich disk is seen across the center, blocking the light from the star or stars still forming there. Blue-reflecting dust is seen in an arc above and below the central disk, although why a tail appears on the lower left is currently unknown. Studying how planets form in HH 30 can help astronomers better understand how planets in our own Solar System once formed, including the Earth.