The actual shape of a black hole depends on how you’re looking at it:
🔵 1. Non-Rotating Black Hole (Schwarzschild Black Hole)
- Shape: Perfectly spherical.
- It’s a symmetric sphere of space where gravity pulls equally in all directions.
- Nothing can escape beyond the event horizon — a spherical boundary.
🌀 2. Rotating Black Hole (Kerr Black Hole)
- Shape: Flattened sphere or oblate spheroid.
- Due to its spin, the black hole bulges slightly at the equator (like Earth).
- It also has:
- A flattened event horizon.
- An ergosphere — a region outside the event horizon where space is dragged by rotation.
👁️🗨️ What We See (Shadow of a Black Hole)
- When astronomers image a black hole (like in the famous M87 black hole photo), they don’t see the black hole itself, but its shadow.
- The shape of that shadow is circular, even for spinning black holes — due to how light bends around it.
📷 First Real Image (M87, 2019 – Event Horizon Telescope)
- The dark shadow is nearly circular.
- Surrounded by a glowing ring of hot plasma falling into the black hole.
- This supports general relativity’s prediction of a roughly spherical or slightly oblate shape.
Would you like a visual showing both types — spherical vs rotating black hole — side by side?

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