Introduction

The special theory of relativity was proposed in 1905 by Albert Einstein (1879–1955). It describes how time, space, and physical phenomena appear in different frames of reference that are moving at constant velocity with respect to each other. This differs from Einstein’s later work on general relativity, which deals with any frame of reference, including accelerated frames.

The theory of relativity led to a profound change in the way we perceive space and time. The “common sense” rules that we use to relate space and time measurements in the Newtonian worldview differ seriously from the correct rules at speeds near the speed of light. For example, the special theory of relativity tells us that measurements of length and time intervals are not the same in reference frames moving relative to one another. A particle might be observed to have a lifetime of $1.0\times {10}^{-8}\text{s}$ in one reference frame, but a lifetime of $2.0\times {10}^{-8}\text{s}$ in another; and an object might be measured to be 2.0 m long in one frame and 3.0 m long in another frame. These effects are usually significant not only at speeds comparable to the speed of light, but even at the much lower speeds of the global positioning satellite. Every signal, satellite position, earth location, must be precisely measured, and the slightest differences in time can create significant inaccuracies. The differences in the measured lengths of the same intervals when measured in different reference frames can therefore be significant enough to render the system unusable. To overcome these issues, Gladys West, a computer scientist and mathematician, developed and programmed the algorithms capable of precisely measuring the Earth's shape, the signals, and satellite positions, and she accounted for the relativistic effects in her algorithm. The United States' GPS system that West helped develop has been the most extensively used geolocation system in the world.

Unlike Newtonian mechanics, which describes the motion of particles, or Maxwell's equations, which specify how the electromagnetic field behaves, special relativity is not restricted to a particular type of phenomenon. Instead, its rules on space and time affect all fundamental physical theories.

The modifications of Newtonian mechanics in special relativity do not invalidate classical Newtonian mechanics or require its replacement. Instead, the equations of relativistic mechanics differ meaningfully from those of classical Newtonian mechanics only for objects moving at relativistic speeds (i.e., speeds less than, but comparable to, the speed of light). In the macroscopic world that you encounter in your daily life, the relativistic equations reduce to classical equations, and the predictions of classical Newtonian mechanics agree closely enough with experimental results to disregard relativistic corrections.