
Artist's conception of HD142527 system: Gas streamers cross gap in protoplanetary disk.
As young stars gather material from their surrounding clouds of gas and dust, the incoming material forms a flat, spinning disk around the star. Planets begin as small clumps within that disk that, through their gravitational pull, add to their mass. As the planets pull in more material, they also leave a wake in their trail that clears out a gap in the disk. Such gaps have been observed in the dust disks surrounding a number of still-forming solar systems.
During this process, the star also continues to grow more massive, leading to the question of how material can get through the gap cleared by the protoplanets and onto the star.
"This has been a bit of a mystery, but now we have found a process that allows the star to continue to grow despite the gap," said Simon Casassus, of the University of Chile and the Millennium Nucleus for Protoplanetary Disks, who led an international research team.
First, the scientists found that the gap is not empty, but is filled by thin, tenuous gas, as shown by ALMA detection of carbon monoxide. "Whereas dust is severely depleted within the gap, some residual gas remains," said Gerrit van der Plas, of the University of Chile. "This agrees with predictions for gap clearing by a planetary-mass body," he added.













