The Size Spectrum of Black Holes
Channel: SpaceSphereFacts
Date: 2024-02-23

From microscopic to galactic behemoths, black holes come in varying sizes. Their unique properties offer insights into stellar evolution, cosmic history, and the limits of physical laws.
Micro black holes: Theoretically, they existed during the early universe's rapid expansion phase.
Stellar black holes: Resulting from collapsed massive stars, they hint at stellar evolution and gravitational wave emissions.
Intermediate-mass black holes (IMBH): Challenging current theories about black hole formation and evolution, they range from hundreds to millions of solar masses.
Supermassive black holes: They dominate galaxy centers and impact their hosts' behaviors.
Tools like EHT and JWST allow scientists to investigate black holes' event horizons, accretion disks, and interactions with neighbors, pushing boundaries of knowledge.
Understanding the entire black hole size spectrum promises to shed light on the cosmos's past, present, and future while challenging established theories and inspiring novel solutions.
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