Calculates the Schwarzschild radius, the boundary beyond which nothing, not even light, can escape, for any mass using R = 2GM/c². Enter a mass in solar masses, Earth masses, or kilograms to find its event horizon radius instantly. Press Add spin to include the spin of a rotating black hole: its event horizon is smaller than the Schwarzschild radius, r₊ = (GM/c²)(1 + √(1 − a²)).