Description
Transcript: Black holes have few observable properties; after all, there’s nothing to see. Mass is a fundamental property, and it can be measured in principle by the gravitational interactions of a black hole with a nearby star. Angular momentum is another property. As with neutron stars, black holes have collapsed by a large factor from a normal stellar state, so they must be rotating very rapidly. A black hole also has a measurable surface area at its event horizon, and it has an amount of electric charge. We cannot say what a black hole is made of because information of the material that went in to make it is lost as soon as that material passes the event horizon. The idea of information being lost is connected to the fact that the entropy of black holes is very large, about 100 million times larger than the equivalent entropy of a star like the Sun.
Transcript: A fundamental prediction of General Relativity is the fact that time slows down in strong gravitational fields. The ultimate test of this idea would be to observe someone falling into a black hole carrying a clock. In theory, the clock would slow down and come to a complete halt as...
Published 07/25/11
Transcript: Any change in a gravitational field or gravitational configuration causes ripples in space time to be emitted. These disturbances which travel at the speed of light are called gravity waves or gravitational radiation. Pulsars slow down slightly in their periods, and this corresponds...
Published 07/25/11
Transcript: If you throw an object up into the air it will eventually slow down and fall back to Earth. The object is losing kinetic energy by trying to climb out through the gravitational field of the Earth. Photons also lose energy as they climb out of the pit of gravity. This effect is...
Published 07/25/11