BLACK HOLE SIMULATION

A black hole with the Sun's mass would have an event horizon of just 2.95 km in radius, small enough to sit inside a town. Mass and spin a* decide the rest: the innermost stable circular orbit shrinks from 3 Rs towards 0.5 Rs for a maximally spinning hole, while the dark shadow keeps an apparent diameter near 5.2 Rs. Around such a hole play out the tidal disruption of a star, mergers, relativistic jet flares and Hawking evaporation.

▸ Loading Schwarzschild / Kerr metric…
▸ Building the event horizon & photon sphere
▸ Heating the accretion disk — Doppler beaming
▸ Bending background light (gravitational lensing)
▸ Spinning up the accretion flow…
▸ Ready — Online. ✅
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⌂ Space

Simulation room Black Hole

Black Hole
Online
Schwarzschild · Kerr metric
Selected black hole
🌌 Sagittarius A*
gravity well (Flamm)
Mass—
Schwarzschild radius—
ISCO (inner disk edge)—
Disk temperature—
Time dilation—
Shadow diameter—
Clock & status
0 yr
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Left-drag = rotate · right-drag = pan · scroll = zoom · click the BLACK REGION = cross-section
WebGL is not enabled in your browser — the 3D black hole cannot be rendered.
Disk brightness & clock rate over time brightnessclock rate
About Black Hole

A black hole with the Sun's mass would have an event horizon of just 2.95 km in radius, small enough to sit inside a town. Mass and spin a* decide the rest: the innermost stable circular orbit shrinks from 3 Rs towards 0.5 Rs for a maximally spinning hole, while the dark shadow keeps an apparent diameter near 5.2 Rs. Around such a hole play out the tidal disruption of a star, mergers, relativistic jet flares and Hawking evaporation.

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