Welcome to roadsat.com on July 11 2009.
This is an internet experiment running to monitor browsing habbits of individuals through wikipedia contents.

Geodetic effect

From Wikipedia, the free encyclopedia

Jump to: navigation, search
A representation of the geodetic effect.
General relativity
G_{\mu \nu} + \Lambda g_{\mu \nu}= {8\pi G\over c^4} T_{\mu \nu}\,
Einstein field equations
Introduction to...
Mathematical formulation of...
Resources
Phenomena
Kepler problem · Lenses · Waves
Frame-dragging · Geodetic effect
Event horizon · Singularity
Black hole

The geodetic effect represents the effect of the curvature of spacetime, predicted by general relativity, on a spinning, moving body. A related effect was first predicted by Willem de Sitter in 1916, who provided relativistic corrections to the Earth-Moon system's motion. De Sitter's work was extended in 1918 by Jan Schouten and in 1920 by Adriaan Fokker.[1]

Contents

[edit] Experimental confirmation

The geodetic effect was verified to a precision of better than 1 percent by Gravity Probe B, an experiment which measures the tilting of the spin axis of gyroscopes in orbit about the Earth.[2] The first results were announced in April 14, 2007 at the meeting of the American Physical Society[3].

[edit] See also

[edit] References

  1. ^ Jean Eisenstaedt, Anne J. Kox (1988). Studies in the History of General Relativity. Birkhäuser. p. 42. ISBN 0817634797. http://books.google.com/books?id=vDHCF_3vIhUC&pg=PA42. 
  2. ^ Gravity Probe B
  3. ^ http://einstein.stanford.edu/content/press_releases/SU/pr-aps-041807.pdf

[edit] External links

This relativity-related article is a stub. You can help Wikipedia by expanding it.
Personal tools

Visit joltnews for the latest headlines
Visit bloit.com for company information
Geed Media does computer consulting on long island.
This page viewed times. See Logs