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Geodetic effect 

A representation of the geodetic effect.
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
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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.

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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].

See also

References

  1. ^ Gravity Probe B
  2. ^ http://einstein.stanford.edu/content/press_releases/SU/pr-aps-041807.pdf

External links

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