Carbon monoxide is ultra-bright and extremely common in protoplanetary disks, making it a prime target for astronomers. But a huge chunk of carbon monoxide is missing in all observations of such disks, if the current predictions of its abundance are correct. According to new research led by the Harvard & Smithsonian’s Center for Astrophysics, carbon monoxide has been hiding in ice formations within the protoplanetary disks. An artist’s illustration...
