Hostname: page-component-cd9895bd7-q99xh Total loading time: 0 Render date: 2024-12-18T15:14:44.018Z Has data issue: false hasContentIssue false
  • English
  • Français

Light propagation in the Solar System for astrometry on sub-micro-arcsecond level

Published online by Cambridge University Press:  07 March 2018

Sven Zschocke
Sven Zschocke*
Affiliation:
Institute of Planetary Geodesy - Lohrmann Observatory, Dresden Technical University, Helmholtzstrasse 10, D-01069, Dresden, Germany email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We report on recent advancement in the theory of light propagation in the Solar System aiming at sub-micro-arcsecond level of accuracy:

  1. (1) A solution for the light ray in 1.5PN approximation has been obtained in the field of N arbitrarily moving bodies of arbitrary shape, inner structure, oscillations, and rotational motion.

  2. (2) A solution for the light ray in 2PN approximation has been obtained in the field of one arbitrarily moving pointlike body.

Keywords

astrometryrelativitygravitation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S330: Astrometry and Astrophysics in the Gaia sky , April 2017 , pp. 106 - 107
Copyright
Copyright © International Astronomical Union 2018 

References

Zschocke, S., 2015, Phys. Rev. D, 92, 063015 CrossRefGoogle Scholar
Zschocke, S. 2016a, Phys. Rev. D, 93, 103010 CrossRefGoogle Scholar
Zschocke, S. 2016b, Phys. Rev. D, 94, 124007 CrossRefGoogle Scholar