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Evidence for the spinning nature of the supermassive black hole in m87, located in the virgo constellation. The black hole, which is 55 million light-years away from earth, has a mass 6.5 billion times greater than the sun. The importance of understanding the behavior of supermassive black holes in active galaxies and their impact on the universe. The use of very long baseline interferometry (vlbi) reveals a 22-year oscillation in m87's central black hole, suggesting the presence of a spinning black hole. The document also explains the significance of accretion disk misalignment, precessional motion, and spacetime curvature in confirming the black hole's spin.
Typology: Schemes and Mind Maps
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