What Is a Black Hole?

Black holes are, in their simplest terms, cosmic structures that swallow everything that is so near-distant because of their massive gravity and their very powerful gravitational forces.

The most important feature that distinguishes the black holes that are predicted by general relativity theory from other objects is the occurrence of an event horizon. The rate of escape on the event horizon, which is a global surface surrounding the sea, is equal to the speed of light. Inside the event horizon, the speed of escape is greater than the speed of light. According to the theory of relativity, it is not possible to move faster than any cismin light with or without mass, so that any object that has once passed the event horizon and falls into the darkness can not get rid of the gravity again. Therefore, a black hole can not be directly observed with its own light. But that does not mean that we can not get any information about the properties of a shaft. It is possible to determine the properties such as mass, angular momentum and electric charge by looking at the changes that are caused in places other than the event horizon.

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Black holes are very simple objects. All properties can be determined when electrical loads, masses and angular momentum are known. Since black holes often occur with the collapse of unloaded objects, it is expected that the total electric charge of the straw is zero. Therefore, it defines the size of an electrically unloaded river mass and angular momentum. Physicist J. A. Wheeler stated that "the black holes are not hair" by all three physical properties of the black holes, as compared to the difficulty of expressing or even determining the physical state of stars and planets. This statement is perfectly suited because the event is a perfect global surface. It can be said that the black holes are similar to the basic particles in that the properties of the black holes can be expressed by a few numbers.