One of these objects that rotates is named for Roy Kerr. These objects have only three measurable properties, mass, charge and angular momentum, according to the No Hair Theorem.
One of these objects that rotates is named for Roy Kerr. These objects have only three measurable properties, mass, charge and angular momentum, according to the No Hair Theorem. These objects are formed by stars above the Tolman-Oppenheimer-Volkoff limit, and these objects were theorized to emit blackbody radiation by Hawking. The Schwarzschild radius is defined as the distance from the singularity at the center of one of these objects to its event horizon. For 10 points, name these deformations in spacetime where gravity is so strong that not even light can escape.
One of these objects that rotates is named for Roy Kerr. These objects have only three measurable properties, mass, charge and angular momentum, according to the No Hair Theorem.
{black hole}s