The Laser Astrometric Test of Relativity Mission
Slava G. Turyshev, Michael Shao, Kenneth L. Nordtvedt Jr

TL;DR
The LATOR mission aims to perform highly precise tests of relativistic gravity by measuring light deflection near the Sun using laser interferometry, potentially revealing new physics beyond general relativity.
Contribution
LATOR introduces a novel space-based laser interferometry experiment with geometric redundancy to measure relativistic effects at unprecedented accuracy.
Findings
Expected measurement of PPN gamma to 1 part in 10^8
Ability to detect next-order post-Newtonian effects (1/c^4)
High-precision measurement of solar quadrupole moment J2
Abstract
This paper discusses new fundamental physics experiment to test relativistic gravity at the accuracy better than the effects of the 2nd order in the gravitational field strength. The Laser Astrometric Test Of Relativity (LATOR) mission uses laser interferometry between two micro-spacecraft whose lines of sight pass close by the Sun to accurately measure deflection of light in the solar gravity. The key element of the experimental design is a redundant geometry optical truss provided by a long-baseline (100 m) multi-channel stellar optical interferometer placed on the International Space Station. The geometric redundancy enables LATOR to measure the departure from Euclidean geometry caused by the solar gravity field to a very high accuracy. LATOR will not only improve the value of the parameterized post-Newtonian (PPN) parameter gamma to unprecedented levels of accuracy of 1 part in 1e8,…
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