A black hole is a region in space where the gravitational pull is so strong that nothing, not even light, can escape from it. This phenomenon occurs when a massive star collapses under its own gravity at the end of its life cycle. Black holes are characterized by their event horizon, which is the boundary beyond which nothing can escape.
There are several types of black holes:
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Stellar Black Holes: Formed when massive stars exhaust their nuclear fuel and collapse. They typically have masses ranging from a few to several tens of solar masses.
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Supermassive Black Holes: Found at the centers of galaxies, including our Milky Way, these black holes contain millions to billions of solar masses. Their formation is still an area of research, but they may form from the merging of smaller black holes and the accumulation of gas and stars over time.
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Intermediate Black Holes: These are less common and have masses between stellar and supermassive black holes, typically ranging from a few hundred to a few thousand solar masses. Their formation mechanisms are still not well understood.
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Primordial Black Holes: Hypothetical black holes that may have formed in the early universe within the first few moments after the Big Bang.
Black holes can be detected indirectly through their interactions with surrounding matter; for instance, when they pull in gas from nearby stars or accrete matter from a companion star, this process can emit X-rays and other forms of radiation that can be observed. Despite their name, black holes are not "holes" in the traditional sense; rather, they are incredibly dense objects with extremely strong gravitational fields.