How it works
Karl Schwarzschild found this solution of Einstein's equations in 1916. Compress the Sun into a sphere about 2.95 km in radius and not even light could escape. The Event Horizon Telescope imaged the shadows of M87* (2019) and Sagittarius A* (2022).
Variables
r_s— Schwarzschild radiusM— mass
Assumptions and limits
- Non-rotating, uncharged black hole (Schwarzschild solution)
- Rotating (Kerr) black holes have a smaller horizon, down to r_s/2 for maximal spin
For education only. These models are simplified and are not suitable for spacecraft navigation or safety-critical engineering. See our scientific accuracy policy.