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Astrodynamical Space Test of Relativity using Optical Devices I (ASTROD I) - A class-M fundamental physics mission proposal for Cosmic Vision 2015-2025

Authors :
Appourchaux, Thierry
Burston, Raymond
Chen, Yanbei
Cruise, Michael
Dittus, Hansjoerg
Foulon, Bernard
Gill, Patrick
Gizon, Laurent
Klein, Hugh
Klioner, Sergei
Kopeikin, Sergei
Krueger, Hans
Laemmerzahl, Claus
Lobo, Alberto
Luo, Xinlian
Margolis, Helen
Ni, Wei-Tou
Paton, Antonio Pulido
Peng, Qiuhe
Peters, Achim
Rasel, Ernst
Ruediger, Albrecht
Samain, Etienne
Selig, Hanns
Shaul, Diana
Sumner, Timothy
Theil, Stephan
Touboul, Pierre
Turyshev, Slava
Wang, Haitao
Wang, Li
Wen, Linqing
Wicht, Andreas
Wu, Ji
Zhang, Xiaomin
Zhao, Cheng
Source :
Exper.Astron.23:491-527,2009
Publication Year :
2008

Abstract

ASTROD I is a planned interplanetary space mission with multiple goals. The primary aims are: to test General Relativity with an improvement in sensitivity of over 3 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 one spacecraft carrying a telescope, four lasers, two event timers and a clock. Two-way, two-wavelength 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 II is envisaged as a three-spacecraft mission which would test General Relativity to one part per billion, enable detection of solar g-modes, measure the solar Lense-Thirring effect to 10 parts per million, 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.<br />Comment: 26 pages, 11 figures, shortened from the original cosmic vision proposal, submitted to Experimental Astronomy; this version, shortened to 25 pages, re-organized and added references, is accepted for publication in Experimental Astronomy

Details

Database :
arXiv
Journal :
Exper.Astron.23:491-527,2009
Publication Type :
Report
Accession number :
edsarx.0802.0582
Document Type :
Working Paper
Full Text :
https://doi.org/10.1007/s10686-008-9131-8