Black Holes
Overview
Black holes are locations where spacetime is bent so severely that nothing can escape. They form when massive stars can no longer support themselves with the energy released in nuclear reactions. The resulting runaway collapse compresses the star's core into a region of enormous gravitational pull while ejecting most surrounding material in a massive supernova. This explosion produces elements that comprise up to 73% of the human body's mass.
The existence of black holes was predicted in 1916 by Albert Einstein's theory of gravity—general relativity—which described the universe as having an underlying fabric that curves in the presence of mass and energy. With enough of either, the warping can become so extreme that anything traveling within a certain distance of the region, including light, becomes trapped. This boundary of no return is the event horizon. With no light able to leave this region via emission or reflection, everything within it appears black.
Scientists estimate that there are 40 quintillion black holes in the universe, which are categorized into three types—supermassive, intermediate, and star-sized—based on their mass. Although not directly observable, their presence can be inferred based on their gravitational influence on nearby objects. Black holes serve as natural laboratories for testing various models in theoretical physics and are theorized to play a significant role in galactic formation and evolution.
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