A Practical Relativistic Model of Microarcsecond Astrometry in Space
Sergei A. Klioner

TL;DR
This paper develops a comprehensive relativistic model for space astrometry achieving 1 microarcsecond accuracy, accounting for gravitational effects within the Solar system and suitable for future high-precision space missions.
Contribution
It introduces a practical relativistic model for astrometry at microarcsecond precision, compatible with existing standards and applicable to both celestial and Solar system objects.
Findings
Model accurately accounts for Solar system gravitational effects.
Compatible with IAU 2000 resolutions for general relativity.
Framework adaptable for 0.1 microarcsecond accuracy improvements.
Abstract
This paper is devoted to a practical model for relativistic reduction of positional observations with an accuracy of 1 \muas which is expected to be attained in the future space astrometry missions. All relativistic effects which are caused by the gravitational field of the Solar system and which are of practical importance for this accuracy level are thoroughly calculated and discussed. The model includes relativistic modeling of the motion of observer, modeling of relativistic aberration and gravitational light deflection as well as a relativistic treatment of parallax and proper motion suitable for the accuracy of 1 \muas. The model is formulated both for remote sources (stars, quasars, etc.) and for Solar system objects (asteroids, etc.). The suggested model is formulated within the framework of Parametrized Post-Newtonian Formalism with parameters and . However, for…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Geophysics and Gravity Measurements
