Appourchaux, T. and Burston, R. and Chen, Y. and Cruise, M. and Dittus, H. and Foulon, B. and Gill, P. and Gizon, L. and Klein, H. and Klioner, S. and Kopeikin, S. and Krüger, Hans and Lämmerzahl, C. and Lobo, A. and Luo, X.-L. and Margolis, H. and Ni, W.-T. and Pulido Patón, A. and Peng, Q. and Peters, A. and Rasel, E. and Rüdiger, A. and Samain, E. and Selig, H. and Shaul, D. and Sumner, T. and Theil, S. and Touboul, P. and Turyshev, S.G. and Wang, H. and Wang, L. and Wen, L. and Wicht, A. and Wu, J. and Zhang, W. and Zhao, C. (2009) Astrodynamical Space Test of Relativity Using Optical Devices I (ASTRO I)- A class-M fundamental physics mission proposal for Cosmic Vision 2015-2025. Experimental Astronomy, 23 (2), pp. 491-527. Springer. DOI: DOI 10.1007/s10686-008-9131-8. ISSN 0922-6435.
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ASTROD I isx a planned interplanetary space mission with multiple goals. The primary aims sre: to test general relativity with an improvement in sensitivity of over three orders of magnitude, improving our understanding of gravity and aiding the development of a new quantum gravity theory; to measure key solar system parameters with increased accuracy, advancing solar physics and our knowledge of the solar system; and to measure the time rate of change of the gravitational constant with an order of magnitude improvement and the anomalous Pioneer acceleration, thereby probing dark matter and dark energy gravitationally. It is an international project, with major contributions from Europe and China and is envisaged as the first in a series of ASTROD missions. ASTROD I will consist of on spacecraft carrying a laser telescope, four lasers, two event timers and a clock. Two-way, two-wavelengths laser pulse ranging will be used between the spacecraft in a solar orbit and deep space laser stations on Earth, to achieve the ASTROD I goals. A second mission, ASTROD (ASTROD II) is envisaged as a three-spacecraft mission which would test General Relativity to 1 ppb, enable detection of solar g-modes, measure the solar Lense-Thirring effec to 10 ppm, and probe gravitational waves at frequencies below the LISA bandwidth. In the third phase (ASTROD III or Super-ASTROD), larger orbits could be implemented to map the outer solar system and to probe primordial gravitational waves at frequencies below the ASTROD II bandwidth.
|Title:||Astrodynamical Space Test of Relativity Using Optical Devices I (ASTRO I)- A class-M fundamental physics mission proposal for Cosmic Vision 2015-2025|
|Journal or Publication Title:||Experimental Astronomy|
|In ISI Web of Science:||Yes|
|Page Range:||pp. 491-527|
|Keywords:||Probing the fundamental laws mof spacetime, Exploring the microscopic origin of gravity, Testing relativistic gravity, Mapping solar-system gravity, Solar g-mode detection, Gravitational wave detection, ASTROD, ASTROD I|
|HGF - Research field:||Aeronautics, Space and Transport (old)|
|HGF - Program:||Space (old)|
|HGF - Program Themes:||W - no assignment|
|DLR - Research area:||Space|
|DLR - Program:||W - no assignment|
|DLR - Research theme (Project):||W - no assignment (old)|
|Location:||Berlin-Adlershof , Bremen|
|Institutes and Institutions:||Institute of Space Systems|
|Deposited By:||Prof.Dr. Hansjörg Dittus|
|Deposited On:||09 Mar 2010 10:03|
|Last Modified:||22 Jan 2015 12:41|
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