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Geodetic effect - Wikipedia, the free encyclopedia

Geodetic effect

From Wikipedia, the free encyclopedia

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...
Phenomena
Kepler problem · Lenses · Waves
Frame-dragging · Geodetic effect
Event horizon · Singularity
Black hole
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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.

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.[1] The first results were announced in April 14, 2007 at the meeting of the American Physical Society[2].

[edit] See also

[edit] References

  1. ^ Gravity Probe B
  2. ^ 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.


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