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Black Holes: Physics, Structure, and Theory

1Introduction to Black Holes and Historical Context2Foundations of General Relativity3The Schwarzschild Solution4Geometry of Spacetime and Tidal Forces5Rotating Black Holes: The Kerr Metric6Black Hole Thermodynamics7Hawking Radiation and Quantum Effects8The Information Paradox9Formation and Astrophysical Evidence10Direct Imaging and Future Horizons
Direct Imaging and Future Horizons

The Anatomy of a Black Hole Shadow

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Before we look at the actual photos, we must understand what we are seeing. The dark center in these images is called the 'shadow.' It is not the event horizon itself. Because gravity bends light so severely, any photon that gets too close falls in. This creates a 'photon sphere.' The shadow we see is actually about 2.6 times wider than the event horizon. Let's trace some light rays to see how this happens.
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An interactive visualization demonstrating how light rays bend around a black hole, defining the photon sphere and the resulting shadow observed by distant observers.

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