Simulations of protoplanetary disks indicate the movements of newborn planets
An article published in “The Astrophysical Journal” reports a study on protoplanetary disks that offers a solution to the rarity of the discovery of newborn exoplanets near the rings that form inside them. A team of three Japanese researchers used the ATERUI II supercomputer, the most powerful used in astronomy, to create simulations of planetary systems’ evolution. The results indicate that the planets create rings as they grow but subsequently move away from them.




