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The Trial of Probing Gravitation with Spacecraft Doppler Tracking: (I) Modeling
Author information
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1. Purple Mountain Observatory, CAS, Nanjing 210008, China
2. Department of Astronomy, Nanjing University, Nanjing 210093, China;Shanghai Key Laboratory of Space Navigation and Position Techniques, Shanghai 200030, China
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History
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Received |
Revised |
Published |
14 Oct 2014 |
10 Feb 2015 |
20 May 2022 |
Issue Date |
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20 May 2022 |
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Currently two-way and three-way spacecraft Doppler tracking techniques are widely used and play important roles in control and navigation of deep space missions. Starting from a one-way Doppler model, we extend the theory to two-way and three-way Doppler models by making them include possible violations of the local Lorentz invariance (LLI) and the local position invariance (LPI) in order to test the Einstein equivalence principle, which is the cornerstone of general relativity and all other metric theories of gravity. After taking the finite speed of light into account, which is the so-called light time solution (LTS), we make these models depend on the time of reception of the signal only for practical convenience. We find that possible violations of LLI and LPI cannot affect two-way Doppler tracking under a linear approximation of LTS, although this approximation is sufficiently good for most cases in the solar system. We also know that, given the accuracy of measurement and control in China and no additional payload in this method, possible violations of LLI and LPI could be the scientific goals of Chinese measurement and control.
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