Mission Design for the Laser Astrometric Test Of Relativity
Slava G. Turyshev, Michael Shao, Kenneth L. Nordtvedt

TL;DR
The LATOR mission aims to precisely measure light deflection near the Sun using laser interferometry between spacecraft and a space-based interferometer, testing general relativity with unprecedented accuracy.
Contribution
This paper presents a novel mission design employing a space-based optical interferometer on the ISS for high-precision tests of relativistic gravity.
Findings
Achieves measurement of the PPN parameter γ to 1 part in 10^8
Plans to measure solar quadrupole moment J2 with high precision
Will test effects like Lense-Thirring precession and non-linear gravity contributions
Abstract
This paper focuses on the mission design for the Laser Astrometric Test Of Relativity (LATOR). This 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 (ISS). The spatial interferometer is used for measuring the angles between the two spacecraft and for orbit determination purposes. The geometric redundancy enables LATOR to measure the departure from Euclidean geometry caused by the solar gravity field to a very high accuracy. Such a design enables LATOR to improve the value of the parameterized post-Newtonian (PPN) parameter to unprecedented levels of accuracy…
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