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Schwarzschild Radius — When Gravity Traps Light - Printable Version +- The Lumin Archive (https://theluminarchive.co.uk) +-- Forum: The Lumin Archive — Core Forums (https://theluminarchive.co.uk/forumdisplay.php?fid=3) +--- Forum: Equations Archive (https://theluminarchive.co.uk/forumdisplay.php?fid=83) +--- Thread: Schwarzschild Radius — When Gravity Traps Light (/showthread.php?tid=440) |
Schwarzschild Radius — When Gravity Traps Light - Leejohnston - 01-08-2026 Schwarzschild Radius — When Gravity Traps Light The Schwarzschild radius defines the size of a black hole’s event horizon — the point beyond which nothing, not even light, can escape. Equation: rₛ = 2GM / c² Where: rₛ = Schwarzschild radius G = gravitational constant M = mass of the object c = speed of light What this means: If an object’s mass is compressed inside its Schwarzschild radius, gravity becomes so strong that escape is impossible. Key insight: • Earth has a Schwarzschild radius of about 9 mm • The Sun’s is about 3 km • Black holes are not “dense objects” — they are regions where spacetime is curved beyond escape Why this matters: This equation tells us when gravity wins completely, creating an event horizon and defining what a black hole actually is. |