Content deleted Content added
m →Special Relativity (SR): It's "its", not "it's" |
m →Relativity: copy edit |
||
Line 116:
== Relativity ==
The [[
(as measured by the frame's clocks). [[General relativity]] takes into account also the effects that gravity has on the passage of time. In the context of GPS the most prominent correction introduced by general relativity is [[gravitational time dilation]]: the clocks located deeper in the gravitational potential well (i.e. closer to the attracting body) appear to tick slower.
[[File:Orbit times.svg|thumb|Satellite clocks are slowed by their orbital speed but sped up by their distance out of the Earth's gravitational well.]]
=== [[Special
=== [[General
=== Combined kinetic and gravitational time dilations ===
Combined, these sources of time dilation cause the clocks on the satellites
To compensate for the discrepancy, the frequency standard on board each satellite is given a rate offset prior to launch, making it run slightly slower than the desired frequency on Earth; specifically, at 10.22999999543 MHz instead of 10.23 MHz.<ref name="Nelson">[http://www.aticourses.com/global_positioning_system.htm The Global Positioning System by Robert A. Nelson Via Satellite] {{Webarchive|url=https://web.archive.org/web/20100718150217/http://www.aticourses.com/global_positioning_system.htm |date=2010-07-18 }}, November 1999</ref> Since the atomic clocks on board the GPS satellites are precisely tuned, it makes the system a practical engineering application of the scientific theory of relativity in a real-world environment.<ref>
▲To compensate for the discrepancy, the frequency standard on board each satellite is given a rate offset prior to launch, making it run slightly slower than the desired frequency on Earth; specifically, at 10.22999999543 MHz instead of 10.23 MHz.<ref name="Nelson">[http://www.aticourses.com/global_positioning_system.htm The Global Positioning System by Robert A. Nelson Via Satellite] {{Webarchive|url=https://web.archive.org/web/20100718150217/http://www.aticourses.com/global_positioning_system.htm |date=2010-07-18 }}, November 1999</ref> Since the atomic clocks on board the GPS satellites are precisely tuned, it makes the system a practical engineering application of the scientific theory of relativity in a real-world environment.<ref>Pogge, Richard W.; [http://www.astronomy.ohio-state.edu/~pogge/Ast162/Unit5/gps.html "Real-World Relativity: The GPS Navigation System"]. Retrieved 25 January 2008.</ref> Placing atomic clocks on artificial satellites to test Einstein's general theory was proposed by [[Friedwardt Winterberg]] in 1955.<ref>{{Cite web |date=1956-08-10 |title=Astronautica Acta II, 25 (1956). |url=http://bourabai.kz/winter/satelliten.htm |access-date=2009-10-23 |archive-date=2014-07-03 |archive-url=https://web.archive.org/web/20140703080406/http://bourabai.kz/winter/satelliten.htm |url-status=dead }}</ref>
=== Calculations ===
To calculate the amount of daily time dilation experienced by GPS satellites relative to Earth we need to separately determine the amounts due to the satellite's velocity and altitude, and add them together.
==== Kinetic time dilation ====
The amount due to velocity
: <math> \frac{1}{\gamma } = \sqrt{1-\frac{v^2}{c^2}} </math>
For small values of ''v/c'' this approximates to:
Line 159 ⟶ 147:
: <math> -8.349\times 10^{-11}\times 60\times 60\times 24\times 10^9\approx -7214 \text{ ns} </math>
That is the satellites' clocks
: Note that this speed of {{val|3874|u=m/s}} is measured relative to Earth's center rather than its surface where the GPS receivers (and users) are. This is because Earth's equipotential makes net time dilation equal across its geodesic surface.<ref>{{Cite web |last=S. P. Drake |date=January 2006 |title=The equivalence principle as a stepping stone from special to general relativity |url=http://www.phys.unsw.edu.au/einsteinlight/jw/2006AJP.pdf |website=Am. J. Phys., Vol. 74, No. 1 |pages=22–25}}</ref> That is, the combination of Special and General effects make the net time dilation at the equator equal to that of the poles, which in turn are at rest relative to the center. Hence we use the center as a reference point to represent the entire surface.
==== Gravitational time dilation ====
The amount of dilation due to gravity
: <math> \frac{t_r}{t_\infty} =\sqrt{1-\frac{2G M}{r c^2}} </math>
where <math>t_r</math> is the time passed at a distance <math>r</math> from the center of the Earth and <math>t_\infty</math> is the time passed for a far away observer.
Line 186 ⟶ 174:
: 45850 – 7210 = 38640 ns
Hence the satellites' clocks gain approximately 38,640 nanoseconds a day or 38.6 μs per day due to
In order to compensate for this gain, a GPS clock's frequency needs to be slowed by the fraction:
|