Deep in space, young stars are surrounded by enormous swirling disks of gas and dust. Inside these disks, new planets slowly begin to form. For years, astronomers have observed mysterious bright rings inside these dusty disks, believing they could be signs of hidden newborn planets. Now, a team of astronomers has discovered a powerful new method to estimate the masses of these invisible worlds simply by studying the dust rings around them. The breakthrough research, led by scientists from the University of Warwick in collaboration with researchers from MIT and McMaster University, has been published in The Astrophysical Journal . Their findings could transform the way astronomers search for and study planets that are still buried deep inside their birth environments. The Mystery of Planet-Forming Disks When stars are born, they are surrounded by giant rotating disks made of gas, dust, and tiny rocky particles. These are known as protoplanetary disks. Over millions of years, material in...