A study led by Naman Bajaj of the University of Arizona examined 72 young, Sun-like stars and their protoplanetary disks using NASA's James Webb Space Telescope ^[1]. As planetary systems mature, the flow of material onto the star declines, causing jets to weaken and allowing high energy radiation from the young star to heat gas in the disk until it escapes via photoevaporation ^[2]. Cauê Borlina, a planetary scientist at Purdue University, stated that calcium and aluminum rich inclusions in meteorites solidified over 4.5 billion years ago before the sun and planets formed ^[3]. Lead author Alexander Berne, a planetary scientist at the University of Arizona, stated that scientists usually assume planetary interiors are spherically symmetric, but this is not necessarily true ^[4].