Hostname: page-component-cd9895bd7-dk4vv Total loading time: 0 Render date: 2024-12-28T17:43:45.979Z Has data issue: false hasContentIssue false
  • English
  • Français

Astrometry by asteroid occultations

Published online by Cambridge University Press:  25 May 2016

L. Kahl Kristensen
L. Kahl Kristensen*
Affiliation:
Institute of Physics and Astronomy University of Aarhus, DK-8000 Aarhus, Denmark

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.

For the determination of the dynamical equinox in fundamental star catalogues observed by astrometric satellites it is proposed to observe occultations of stars by selected asteroids. Being a long term programme now is the time for planning. Quadrature observations and photometric back-up are essential.

Type
Part X - Solar System Astrometry
Information
Symposium - International Astronomical Union , Volume 172: Dynamics, Ephemerides and Astrometry of the Solar System , 1996 , pp. 443 - 446
Copyright
Copyright © Kluwer 1996 

References

Brouwer, D.: 1935, Astron. Journ. 44, 57–63.Google Scholar
Dyson, F.: 1929, Trans. I.A.U. 3, 227.Google Scholar
Kristensen, L.K.: 1980, Mitt. d. Astron. Ges. 48, 50–55.Google Scholar
Kristensen, L.K.: 1981, Astron. Astrophys. Suppl. Ser. 44, 375.Google Scholar
Newcomb, S.: 1878, Motion of the Moon. Washington Observations for 1875. Washington, Appendix II.Google Scholar
Numerov, M.B.: 1932, Bull. l'Inst. Astron. (Leningrad) 32, 139–147.Google Scholar
Strömgren, B.: 1950, Trans. I.A.U. 7, 220.Google Scholar