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Black holes are invisible regions with immense gravity, shaping galaxies and testing physics at the universe’s most extreme limits.
Black holes shape galaxies by regulating star formation, driving jets, and merging during collisions, playing a key role in cosmic evolution and galaxy growth.
Black hole mergers unleash powerful gravitational waves, revealing key insights into stellar evolution, gravity, and the universe’s deepest mysteries.
Event horizons are the defining boundaries of black holes, marking the point of no return for matter and light. This article explores their nature, detection, and significance in modern physics.
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