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Clock at Lagrange point L4 or L5

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Abstract and 1. Introduction

  1. Clock in Orbit

    2.1 Coordinate Time

    2.2 Local Frame for the Moon

  2. Clock Rate Differences Between Earth and Moon

  3. Clocks at Earth-Moon Lagrance Points

    4.1 Clock at Lagrange point L1

    4.2. Clock at Lagrange point L2

    4.3. Clock at Lagrange point L4 or L5

  4. Conclusions


Appendix 1: Fermi Coordinates with Origin at the Center of the Moon

Appendix 2: Construction of Freely Falling Center of Mass Frame

Appendix 3: Equations of Motion of Earth and Moon

Appendix 4: Comparing Results in Rotating and Non-Rotating Coordinate Systems

Acknowledgments and References

4.3. Clock at Lagrange point L4 or L5

The clock is equidistant from Earth and the Moon. The total velocity squared is the sum of the radial velocity squared and the transverse velocity squared:



TABLE II. Results: computed rates for various points of interest.



Authors:

(1) Neil Ashby, National Institute of Standards and Technology, Boulder, CO 80305 ([email protected]);

(2) Bijunath R. Patla, National Institute of Standards and Technology, Boulder, CO 80305 ([email protected]).


This paper is available on arxiv under CC0 1.0 license.


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