Schwarzschild Radius Formula:
From: | To: |
The Schwarzschild radius is the radius of the event horizon of a non-rotating black hole. It represents the boundary beyond which nothing, not even light, can escape the black hole's gravitational pull.
The calculator uses the Schwarzschild radius formula:
Where:
Explanation: The formula shows the relationship between an object's mass and the radius at which its escape velocity equals the speed of light.
Details: The Schwarzschild radius is fundamental in general relativity and black hole physics. It helps determine whether an object of a given mass could theoretically become a black hole if compressed within this radius.
Tips: Enter the mass of the object in kilograms. The result will show the Schwarzschild radius in meters. For example, the Sun's mass would be 1.989 × 1030 kg.
Q1: What's the Schwarzschild radius of Earth?
A: For Earth's mass (5.972 × 1024 kg), the Schwarzschild radius is about 8.87 millimeters.
Q2: What's the Schwarzschild radius of the Sun?
A: For the Sun's mass (1.989 × 1030 kg), it's approximately 2.95 kilometers.
Q3: Does anything have a natural Schwarzschild radius?
A: Only objects that have collapsed into black holes naturally have sizes smaller than their Schwarzschild radii.
Q4: Can a human have a Schwarzschild radius?
A: Yes, but it's extremely small (about 10-25 meters for a 70 kg person) - far smaller than any known elementary particle.
Q5: Does rotation affect the Schwarzschild radius?
A: The original formula is for non-rotating black holes. Rotating black holes (Kerr black holes) have more complex event horizons.