Gravitational Time Dilation Formula:
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Gravitational time dilation is a phenomenon predicted by Einstein's theory of general relativity where time passes at different rates in regions of different gravitational potential. Clocks closer to a massive object (where gravity is stronger) run slower than clocks further away.
The calculator uses the gravitational time dilation equation:
Where:
Explanation: The equation shows how time slows down near massive objects. The effect becomes significant only in extremely strong gravitational fields, like those near black holes or neutron stars.
Details: Gravitational time dilation has practical implications for GPS satellite systems, where clocks in orbit must be regularly adjusted to account for both gravitational and velocity time dilation effects.
Tips: Enter proper time in seconds, mass in kilograms, and radial coordinate in meters. All values must be positive. The radial coordinate must be greater than the Schwarzschild radius (2GM/c²) to avoid imaginary results.
Q1: How significant is time dilation on Earth?
A: On Earth's surface, the effect is minimal (~0.02 seconds per year compared to space), but crucial for GPS accuracy.
Q2: What happens at the Schwarzschild radius?
A: At r = 2GM/c² (the event horizon of a black hole), time dilation becomes infinite - time appears to stop from an outside observer's perspective.
Q3: Does this formula work for any mass?
A: Yes, but the effect is only noticeable near extremely massive objects like neutron stars or black holes.
Q4: How does this relate to velocity time dilation?
A: Both are relativistic effects, but gravitational dilation depends on gravitational potential while velocity dilation depends on relative speed.
Q5: Has gravitational time dilation been proven?
A: Yes, through numerous experiments including the Pound-Rebka experiment and GPS system corrections.