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

Thierry Appourchaux, Raymond Burston, Yanbei Chen, Michael Cruise, Hansjörg Dittus, Bernard Foulon, Patrick Gill, Laurent Gizon, Hugh Klein, Sergei Klioner, Sergei Kopeikin, Hans Krüger, Claus Lämmerzahl, Alberto Lobo, Xinlian Luo, Helen Margolis, Wei Tou Ni, Antonio Pulido Patón, Qiuhe Peng, Achim PetersErnst Rasel, Albrecht Rüdiger, Étienne Samain, Hanns Selig, Diana Shaul, Timothy Sumner, Stephan Theil, Pierre Touboul, Slava Turyshev, Haitao Wang, Li Wang, Linqing Wen, Andreas Wicht, Ji Wu, Xiaomin Zhang, Cheng Zhao

Research output: Contribution to journalArticlepeer-review

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 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 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 (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 effect 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.

Original languageEnglish (US)
Pages (from-to)491-527
Number of pages37
JournalExperimental Astronomy
Volume23
Issue number2
DOIs
StatePublished - Feb 2009

Keywords

  • ASTROD
  • ASTROD I
  • Exploring the microscopic origin of gravity
  • Gravitational-wave detection
  • Mapping solar-system gravity
  • Probing the fundamental laws of spacetime
  • Solar g-mode detection
  • Testing relativistic gravity

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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