Schwarzschild Diameter Formula:
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The Schwarzschild diameter represents the diameter of the event horizon of a non-rotating black hole. It is derived from Karl Schwarzschild's solution to Einstein's field equations and defines the boundary beyond which nothing, not even light, can escape the black hole's gravitational pull.
The calculator uses the Schwarzschild diameter formula:
Where:
Explanation: The formula calculates the diameter of the event horizon based solely on the mass of the black hole, using fundamental physical constants.
Details: Understanding the Schwarzschild diameter is crucial for studying black hole physics, gravitational theory, and astrophysical phenomena. It helps astronomers estimate the size of black holes and understand their properties.
Tips: Enter the mass of the black hole in kilograms. The mass must be a positive value. For astronomical objects, you may need to use scientific notation or very large numbers.
Q1: What is the event horizon?
A: The event horizon is the boundary around a black hole from which no matter or radiation can escape. It marks the point of no return.
Q2: Does this formula work for rotating black holes?
A: No, this formula is specifically for non-rotating (Schwarzschild) black holes. Rotating black holes (Kerr black holes) have a more complex geometry.
Q3: What are typical Schwarzschild diameters?
A: For a solar mass black hole (2 × 10³⁰ kg), the diameter is approximately 5.9 kilometers. Supermassive black holes can have diameters of astronomical units or light-days.
Q4: Can anything escape from inside the Schwarzschild radius?
A: No, once inside the event horizon, all paths lead toward the singularity, and nothing can escape, not even light.
Q5: How accurate is this calculation?
A: The calculation is theoretically exact for non-rotating, uncharged black holes in vacuum, using the most precise values for physical constants.