Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-12-01T10:56:56.837Z Has data issue: false hasContentIssue false
  • English
  • Français

Ecliptical Coordinate System as the Basis of Regatta–Astro Space Astrometry Program

Published online by Cambridge University Press:  12 April 2016

Irina S. Guseva ,
Alexandr Ju. Kogan  and
Vladimir N. Heifets
Irina S. Guseva
Affiliation:
Central Astronomical Observatory USSR Academy of Sciences Pulkovo 196140 LeningradUSSR
Alexandr Ju. Kogan
Affiliation:
Space Research InstituteUSSR Academy of Sciences Profsojusnaja, 84/32 117810 MoscowUSSR
Vladimir N. Heifets
Affiliation:
Space Research InstituteUSSR Academy of Sciences Profsojusnaja, 84/32 117810 MoscowUSSR

Extract

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.

One of the most important problems of modern astrometry is constructing of an ideal inertial coordinate system. A bulk of up–to–date star catalogues is referenced to an equatorial frame, which is far from being really inertial, Some attempts were made to remove this defect by excluding both nutation and precession in right ascention [Guinet 1979, Murray, 1990]. This proposal seams to be a compromise between the existing tradition and the new requirements met by the modern astrometry.

Type
Part 2. Poster Papers
Information
International Astronomical Union Colloquium , Volume 127: Reference Systems , 1991 , pp. 276 - 279
Copyright
Copyright © United States Naval Observatory 1991

References

1. Guinot, B; 1979, Time and Earth’s rotation, 1AU Symp. 82 Google Scholar
2. Murray, C.A.: 1790, Inertial Coordinate system on the sky, IAU Symp. 141 Google Scholar
3. Avanesov, G. et al: 1990, Inertial Coordinate system on the sky, IAU Symp. 141 Google Scholar