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Predictions of occultations by minor planets as a test of accuracy

Published online by Cambridge University Press:  04 August 2017

Leif Kahl Kristensen*
Affiliation:
Institute of Physics, University of Aarhus DK - 8000 Aarhus C, Denmark

Abstract

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Predictions of tracks of occultations of stars by minor planets give a strong test of the accuracy of observations, star places, and dynamical theories. A critical discussion of the 1983 September 11 occultation of 14 Piscium by (51) Nemausa shows that the systematic regional errors of fundamental stars introduce errors in the long-term predictions of occultations that are larger than relativistic effects.

Type
Motions of Natural Bodies in the Solar System
Copyright
Copyright © Reidel 1986 

References

Bien, R., 1984: (Astron. Rechen Inst., private communication).Google Scholar
Bien, R. and Schwan, H., 1983: Astron. Astrophys. 124, L7L9.Google Scholar
Dunham, D.W., 1983 (private communication).Google Scholar
Fricke, W., 1963: Veröff. Astron. Rechen Inst., Heidelberg, 10, 8.Google Scholar
Hughes, J.A., 1979: (US Naval Obs., private communication).Google Scholar
Klemola, A.R. and Harlan, E.A., 1984: Astron. Journal 89, 879.Google Scholar
Kristensen, L.K., 1980: Mitt. d. Astron. Gesellschaft 48, 50.Google Scholar
Kristensen, L.K., 1981: Astron. Astrophys. Suppl. Ser. 44, 375.Google Scholar
Kristensen, L.K., 1983: I.A.U. Circular 3834.Google Scholar
Requième, Y. and Rapaport, M., 1985: Minor Planet Circular 9747.Google Scholar
Strömgren, B., 1950: Transactions of the I.A.U. VII, Cambridge, 220.Google Scholar