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

TL;DR
The LATOR mission aims to perform highly precise measurements of gravitational effects near the Sun to test and refine theories of relativity and gravity with unprecedented accuracy.
Contribution
This paper introduces the optical design and mission concept of LATOR, a novel experiment to measure relativistic gravity effects with significantly improved precision.
Findings
Projected measurement of the Eddington parameter γ to 1 part in 10^9
First measurement of gravity's non-linear light effects at 0.01% accuracy
Direct measurement of solar quadrupole moment J2 and frame-dragging effects
Abstract
This paper discusses the Laser Astrometric Test Of Relativity (LATOR) mission. By using a combination of independent time-series of highly accurate gravitational deflection of light in the immediate proximity to the Sun along with measurements of the Shapiro time delay on the interplanetary scales (to a precision respectively better than radians and 1 cm), LATOR will significantly improve our knowledge of relativistic gravity. The primary mission objective is to i) measure the key post-Newtonian Eddington parameter with accuracy of a part in 10. is a direct measure for presence of a new interaction in gravitational theory, and, in its search, LATOR goes a factor 30,000 beyond the present best result, Cassini's 2003 test. Other mission objectives include: ii) first measurement of gravity's non-linear effects on light to 0.01% accuracy; including…
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Taxonomy
TopicsHistory and Developments in Astronomy · Planetary Science and Exploration · Relativity and Gravitational Theory
