Physics
Textbooks
Boundless Physics
Special Relativity
Consequences of Special Relativity
Physics Textbooks Boundless Physics Special Relativity Consequences of Special Relativity
Physics Textbooks Boundless Physics Special Relativity
Physics Textbooks Boundless Physics
Physics Textbooks
Physics
Concept Version 6
Created by Boundless

Time Dilation

Time dilation is an actual difference of elapsed time between two events as measured by observers moving relative to each other.

Learning Objective

  • Explain why time dilation can be ignored in daily life


Key Points

    • Time dilation effects are extremely small for speeds below 1/10 the speed of light and can be safely ignored at daily life.
    • Time dilation effects become important when an object approaches speeds on the order of 30,000 km/s (1/10 the speed of light).
    • The formula for determining time dilation is: $\Delta t' = \frac{\Delta t}{\sqrt{1 - v^{2}/c^{2}}}$.

Terms

  • Lorentz factor

    The factor, used in special relativity, to calculate the degree of time dilation, length contraction and relativistic mass of an object moving relative to an observer.

  • speed of light

    the speed of electromagnetic radiation in a perfect vacuum: exactly 299,792,458 meters per second by definition

  • time dilation

    The slowing of the passage of time experienced by objects in motion relative to an observer; measurable only at relativistic speeds.


Full Text

Time dilation is an actual difference of elapsed time between two events as measured by observers either moving relative to each other.

For instance, two rocket ships (A and B) speeding past one another in space would experience time dilation. If they somehow had a clear view into each other's ships, each crew would see the others' clocks and movement as going too slowly. That is, inside the frame of reference of Ship A, everything is moving normally, but everything over on Ship B appears to be moving slower (and vice versa).

From a local perspective, time registered by clocks that are at rest with respect to the local frame of reference (and far from any gravitational mass) always appears to pass at the same rate. In other words, if a new ship, Ship C, travels alongside Ship A, it is "at rest" relative to Ship A. From the point of view of Ship A, new Ship C's time would appear normal too.

The formula for determining time dilation is: $\Delta t' = \gamma \Delta t = \frac{\Delta t}{\sqrt{1 - v^{2}/c^{2}}}$

where Δt is the time interval between two co-local events (i.e. happening at the same place) for an observer in some inertial frame (e.g. ticks on his clock), this is known as the proper time, Δt' is the time interval between those same events, as measured by another observer, inertially moving with velocity v with respect to the former observer, v is the relative velocity between the observer and the moving clock, c is the speed of light, and $\gamma = \frac{1}{\sqrt{1 - v^{2}/c^{2}}}$

is the Lorentz factor. Thus the duration of the clock cycle of a moving clock is found to be increased: it is measured to be "running slow". Note that for speeds below 1/10 the speed of light, Lorentz factor is approximately 1 . Thus, time dilation effects and extremely small and can be safely ignored in a daily life. They become important only when an object approaches speeds on the order of 30,000 km/s (1/10 the speed of light).

Lorentz Factor

Lorentz factor as a function of speed (in natural units where c = 1). Notice that for small speeds (less than 0.1), γ is approximately 1.

[ edit ]
Edit this content
Prev Concept
Simultaneity
Effects of Time Dilation: The Twin Paradox and the Decay of the Muon
Next Concept
Subjects
  • Accounting
  • Algebra
  • Art History
  • Biology
  • Business
  • Calculus
  • Chemistry
  • Communications
  • Economics
  • Finance
  • Management
  • Marketing
  • Microbiology
  • Physics
  • Physiology
  • Political Science
  • Psychology
  • Sociology
  • Statistics
  • U.S. History
  • World History
  • Writing

Except where noted, content and user contributions on this site are licensed under CC BY-SA 4.0 with attribution required.