A stellar black hole is a type of black hole that is formed from the remnants of a massive star after it has exhausted its nuclear fuel and undergoes a supernova explosion. These black holes are relatively small in size compared to supermassive black holes, with masses ranging from about 3 to 20 times that of the Sun.
When a massive star reaches the end of its life cycle, it undergoes a supernova explosion, during which the outer layers of the star are ejected into space, while the core collapses under its own gravity. If the core's mass is above a certain threshold, known as the Chandrasekhar limit, it will continue collapsing into a black hole, forming a stellar black hole.
Stellar black holes are characterized by their immense gravitational pull, which is so strong that not even light can escape from them, giving them their name. This makes them invisible to traditional telescopes and can only be detected through their interaction with nearby matter or through the gravitational waves they emit.
By understanding the formation and characteristics of stellar black holes, as well as their implications for our understanding of the cosmos, we can gain valuable insights into the nature of these enigmatic objects and their role in shaping the universe.
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