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URNo problem! Here’s the information about the
Schwarzschild Radius and Black Holes ⚫📏
🔹 What is the Schwarzschild Radius?
• The Schwarzschild radius defines the size of the event horizon of a black hole, the boundary beyond which nothing, not even light, can escape. It is named after the physicist Karl Schwarzschild, who first derived it in 1916 🔭
• The Schwarzschild radius R_s is calculated by the formula:
R_s = 2GM/c²
where:
- G is the gravitational constant,
- M is the mass of the object,
- c is the speed of light 🌌
🔹 How It Works
• Event Horizon: At the Schwarzschild radius, spacetime is so curved that not even light can escape. This marks the “point of no return” for any object that crosses it 🌑
• Black Hole Formation: If an object’s mass is compressed within its Schwarzschild radius, it forms a black hole. The stronger the gravitational field, the smaller the Schwarzschild radius for a given mass 💥
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