A stellar black hole is a type of black hole that is formed from the remnants of a massive star after it undergoes a supernova explosion. These black holes are known for their incredibly strong gravitational pull, which is so intense that not even light can escape from it. Here's a study guide to help you understand the concept of stellar black holes:
When a massive star exhausts its nuclear fuel, it can no longer support its own mass against gravitational collapse. The core of the star collapses under its own gravity, leading to a supernova explosion. If the core's mass is greater than about three times the mass of the Sun, it collapses into a black hole, forming a stellar black hole.
Black holes are characterized by several key properties, including:
Stellar black holes cannot be observed directly, as they do not emit light. However, their presence can be inferred through the effects they have on nearby stars and other celestial objects. Astronomers look for specific phenomena, such as the gravitational influence of a stellar black hole on its surrounding environment, to indirectly detect their presence.
Stellar black holes are fascinating astronomical objects that have captured the imagination of scientists and the public alike. Their mysterious nature and extreme gravitational pull make them a subject of ongoing research and exploration in the field of astrophysics.
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