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Everything about Geodetic effect

Precession of satellite orbits due to a celestial body's presence affecting spacetime

The geodetic effect is a consequence of the curvature of spacetime, predicted by general relativity, on a vector carried along with an orbiting body. For example, the vector could be the angular momentum of a gyroscope orbiting the Earth, as carried out by the Gravity Probe B experiment. The geodetic 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. It can also be applied to a particular secular precession of astronomical orbits, equivalent to the rotation of the Laplace–Runge–Lenz vector. Wikipedia →

🧭 Start here: a 6-step reading path

  1. Read the overview: Geodetic effectA 5-minute orientation
  2. Pick up a classic book: Doppler handbook for Magnavox MX 1502The most-reprinted book on the subject
  3. Read the landmark paper: Effect of annual signals on geodetic velocityCited 481 times
  4. Go sideways: Spherically symmetric spacetimeA closely related topic
  5. Go sideways: Theoretical motivation for general relativityA closely related topic

📖 Definitions

Noun the change in the spin of a gyroscope as it moves through curved spacetime

🏆 Landmark papers (most cited)

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