Astronomers using the Center for High Angular Resolution Astronomy (CHARA) Array interferometer at the Mount Wilson Observatory have observed the long-sought, innermost dusty ring around a supermassive black hole in NGC 4151, an active spiral galaxy located 62 million light-years away in the constellation of Canes Venatici. Kishimoto et al. captured a long-sought-after view of the dusty inner region in NGC 4151. Image credit: Georgia State University...
