Local Landmarks & General Relativity

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SUMMARY

General relativity establishes that no object can exceed the speed of light when measured against local landmarks. Local landmarks are defined by their proximity and the curvature of spacetime around them. As spacetime curvature increases, the effective distance between local landmarks decreases, particularly in strong gravitational fields like those near the sun. The boundary between local and distant landmarks is determined by the deviation from flat spacetime exceeding the limits of instrumental error.

PREREQUISITES
  • Understanding of general relativity principles
  • Familiarity with spacetime curvature concepts
  • Knowledge of local versus distant reference frames
  • Basic grasp of instrumental error in measurements
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  • Study the implications of spacetime curvature on local measurements
  • Explore the concept of local versus distant landmarks in physics
  • Research the effects of gravity on light speed and measurements
  • Examine instrumental error and its impact on scientific observations
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Physicists, students of general relativity, and anyone interested in the implications of spacetime curvature on measurements and the speed of light.

codeman_nz
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General relativity says that nothing can go faster than the speed of light when measured against local landmarks.

What counts as a local landmark? What is the boundary between a local and distant landmark?
 
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The distance between such local landmarks gets smaller as the spacetime curvature around them, or between them increases. So in flat spacetime it can be any distance, but close to the sun it would be smaller. I suppose the boundary is where the nearby spacetime deviates from flatness by an amount greater than the instrumental error.
 

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