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. The closer to a massive object, the slower time passes.
The calculator uses the gravitational time dilation formula:
Where:
Explanation: This formula describes how time is affected by gravity, with time passing slower in stronger gravitational fields.
Details: Understanding gravitational time dilation is crucial for GPS satellite systems, astrophysics research, and testing fundamental principles of general relativity. Even small time differences become significant over large distances or long periods.
Tips: Enter proper time in seconds, mass in kilograms, and radius in meters. All values must be positive numbers. The calculator uses standard physical constants for gravitational constant and speed of light.
Q1: What is the significance of the term under the square root?
A: The term \( \frac{2GM}{rc^2} \) represents the gravitational potential. When this approaches 1 (at the Schwarzschild radius), time dilation becomes infinite, indicating an event horizon.
Q2: How significant is time dilation in everyday life?
A: For Earth's gravity, the effect is very small (about 1 second difference every 30 years between sea level and space), but it's crucial for precision systems like GPS.
Q3: Does this formula work for all gravitational fields?
A: This is the exact solution for a non-rotating, uncharged spherical mass. For other configurations, more complex formulas are needed.
Q4: What happens when 2GM/rc² equals or exceeds 1?
A: This represents the Schwarzschild radius or event horizon of a black hole. Beyond this point, the formula gives imaginary results, indicating no information can escape.
Q5: How is this different from velocity time dilation?
A: Gravitational time dilation is caused by differences in gravitational potential, while velocity time dilation (from special relativity) is caused by relative motion between reference frames.