What are the different types of black holes?

diamonds are not forever. They can be very hard, but they are quite rigid and break like glass if they are hard enough. At high temperatures, steel tools can be used regularly and jewelers can regularly use diamonds. The rest of the collapse of giant stars, black holes are basically inviolable. They have the same matter as their parent star, put into an area that is usually considered to be a zero dimensional point. Stars can die of supernova or collisions with other stars - black holes can't.

black holes very slowly evaporate due to a phenomenon called hawking radiation, named after Stephen Hawking, who first postulated it. The length of the time that would require a black hole with a mass equal to the sun is about 10 years ^{67 , which is about as close to forever as anything can get in this universe. Supermasive black holes last a lot, for a long time to evaporate. They will be around more centuries thanare particles in space. To simplify, we can spin and charge these materials.}

In the mass variables are two main categories of black holes: solar black holes, between about 2.5 and 20 solar materials and supermassive black holes, between one hundred thousand and tens of billions of solar materials. The black holes of sun mass are formed when giant stars collapse after supernova, supermassive black holes are formed in the center of the size of the size of the galaxy size. Astronomers believe that almost all galaxies have central black holes, including the Milky Railway, our galaxy whose central black hole has already been intended.

angular momentum or spin so that it does not confuse with variable rotation in quantum mechanics, has to do with how quickly the black hole turns. Most black holes rotate very quickly because they retain all the angular momentum of their superior star, but condense into a much smaller space.It is similar to the way the skater speeds up the speed of rotation when it brings hands closer. The swivel black holes are called Kerr Black Holes.

The last variable used to describe black holes is a charge. Very few black holes have any noticeable charge, because the electromagnetic force is many times stronger than gravity, which prevents the collapse of any charged object as a result of self -apparatus. Imagine trying to press two star magnets on the sides with the same magnetic orientation, and not use anything but gravity as a pressure force. It can't be done. Charmed black holes are known as Reissner-Nordström or Kerr-Newman Black Hole, which are not annual and rotating, respect.

Inadvertent, unchanged black holes are known as Schwarzschild Black Holes.