Black Holes, Explained Clearly: It’s Not a Vacuum (Richard Feynman)
Автор: Quantum Horizon
Загружено: 2026-02-07
Просмотров: 46
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Most people picture a black hole as a cosmic vacuum cleaner. That’s the wrong mental image. From far away, a black hole doesn’t pull harder than any object with the same mass—so the real mystery is not “stronger gravity,” but what happens to the paths you’re allowed to take in spacetime.
In this episode, I break black holes down in plain physical terms: what an event horizon really is (a limit on information, not a wall), why “escape” stops (not because light gets tired, but because outward paths disappear), and why time near a black hole can look frozen to a distant observer while still feeling normal to the one falling in.
Black holes aren’t science fiction—they’re measured through orbits, hot gas, bent light, and extreme energy near the boundary. With new Webb results and ongoing observations of powerful black-hole activity, the same core ideas keep showing up: gravity shapes space and time, and the rules stay precise even where intuition collapses.
#BlackHole #Space #Science #NASA #RichardFeynman
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