Fundamental Physics with the Laser Astrometric Test Of Relativity
LATOR Collaboration: S.G. Turyshev, H. Dittus, M. Shao, K.L., Nordtvedt, Jr., C. Laemmerzahl, S. Theil, W. Ertmer, E. Rasel, R. Foerstner,, U. Johann, S. Klioner, M. Soffel, B. Dachwald, W. Seboldt, V. Perlick, M.C.W., Sandford, R. Bingham, B. Kent, T.J. Sumner, O. Bertolami

TL;DR
LATOR is a highly precise experiment designed to test Einstein's general relativity by measuring light deflection, time delay, and other gravitational effects near the Sun, significantly improving current measurement accuracy.
Contribution
The paper introduces the LATOR mission, a novel experiment that aims to measure key relativistic parameters with unprecedented precision, surpassing previous tests like Cassini's.
Findings
Measurement of the PPN parameter to 1 part in 10^9
First measurement of gravity's non-linear effects on light
Direct measurement of solar quadrupole moment J2
Abstract
The Laser Astrometric Test Of Relativity (LATOR) is a joint European-U.S. Michelson-Morley-type experiment designed to test the pure tensor metric nature of gravitation - a fundamental postulate of Einstein's theory of general relativity. 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 interplanetary scales (to a precision respectively better than 0.1 picoradians 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 \gamma with accuracy of a part in 10^9. (1-\gamma) 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,…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Geophysics and Gravity Measurements · History and Developments in Astronomy
