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Experimental Astronomy

, 27:27 | Cite as

Advancing fundamental physics with the Laser Astrometric Test of Relativity

The LATOR mission
  • S. G. Turyshev
  • M. Shao
  • K. L. Nordtvedt
  • H. DittusEmail author
  • C. Laemmerzahl
  • S. Theil
  • C. Salomon
  • S. Reynaud
  • T. Damour
  • U. Johann
  • P. Bouyer
  • P. Touboul
  • B. Foulon
  • O. Bertolami
  • J. Páramos
Original Article

Abstract

The Laser Astrometric Test of Relativity (LATOR) is an experiment designed to test the metric nature of gravitation—a fundamental postulate of the Einstein’s general theory of relativity. The key element of LATOR is a geometric redundancy provided by the long-baseline optical interferometry and interplanetary laser ranging. By using a combination of independent time-series of 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 and cosmology. The primary mission objective is i) to measure the key post-Newtonian Eddington parameter γ with accuracy of a part in 109. \(\frac{1}{2}(1-\gamma)\) 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, Cassini’s 2003 test. Other mission objectives include: ii) first measurement of gravity’s non-linear effects on light to ∼0.01% accuracy; including both the traditional Eddington β parameter and also the spatial metric’s 2nd order potential contribution (never measured before); iii) direct measurement of the solar quadrupole moment J 2 (currently unavailable) to accuracy of a part in 200 of its expected size of ≃ 10 − 7; iv) direct measurement of the “frame-dragging” effect on light due to the Sun’s rotational gravitomagnetic field, to 0.1% accuracy. LATOR’s primary measurement pushes to unprecedented accuracy the search for cosmologically relevant scalar-tensor theories of gravity by looking for a remnant scalar field in today’s solar system. We discuss the science objectives of the mission, its technology, mission and optical designs, as well as expected performance of this experiment. LATOR will lead to very robust advances in the tests of fundamental physics: this mission could discover a violation or extension of general relativity and/or reveal the presence of an additional long range interaction in the physical law. There are no analogs to LATOR; it is unique and is a natural culmination of solar system gravity experiments.

Keywords

Fundamental physics Tests of general relativity Scalar-tensor theories Modified gravity Interplanetary laser ranging Optical interferometry Picometer-class metrology LATOR 

PACS

04.80.-y 95.10.Eg 95.55.Pe 

Notes

Acknowledgements

The work described here was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.

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Copyright information

© Springer Science+Business Media B.V. 2009

Authors and Affiliations

  • S. G. Turyshev
    • 1
  • M. Shao
    • 1
  • K. L. Nordtvedt
    • 2
  • H. Dittus
    • 3
    • 4
    Email author
  • C. Laemmerzahl
    • 3
  • S. Theil
    • 4
  • C. Salomon
    • 5
  • S. Reynaud
    • 5
  • T. Damour
    • 6
  • U. Johann
    • 7
  • P. Bouyer
    • 8
  • P. Touboul
    • 9
  • B. Foulon
    • 9
  • O. Bertolami
    • 10
  • J. Páramos
    • 10
  1. 1.Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadenaUSA
  2. 2.Northwest AnalysisBozemanUSA
  3. 3.Centre of Applied Space Technology & Microgravity (ZARM)University of BremenBremenGermany
  4. 4.Institute of Space SystemsGerman Aerospace CenterBremenGermany
  5. 5.Laboratoire Kastler BrosselUniversité Pierre et Marie CurieParisFrance
  6. 6.Institut des Hautes Etudes ScientifiquesBures-sur-YvetteFrance
  7. 7.Department of Science ProgramsEarth Observation and ScienceFriedrichshafenGermany
  8. 8.Laboratoire Charles Fabry de l’Institut d’OptiqueOrsay CEDEXFrance
  9. 9.Physics and Instrumentation DepartmentONERAChatillonFrance
  10. 10.Instituto Superior TécnicoDepartamento de FísicaLisboaPortugal

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