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Fundamental reference systems; Past, present, and future

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Abstract

The present fundamental reference system is defined by the FK5 Fundamental Reference Catalog and the associated IAU Resolutions of 1976 through 1982. The past is defined to be what preceded the present fundamental reference system and future is defined to be what ever will come after it. The resulting characteristics of the different fundamental reference systems are considered from the aspects of the observational data, the computational methods, and the underlying theories. Having developed an understanding of these operational fundamental reference systems, the desired properties of the ideal fundamental reference system are presented. Finally, some questions concerning the future fundamental reference system are presented.

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References

  • Astronomical Almanac 1984

  • Capitaine, N., Willians, J. G. and Seidelmann, P. K. 1985 ‘Clarification concerning the Definition and Determination of the Celestial Ephemer is Pole’Astronomy and Astrophysics,146, 381.

    Google Scholar 

  • Eichhorn, H., 1984 ‘Comprehensive Star Catalogs’ Bull. Inform C. D. S. No.27.

  • Eichhorn, H., 1974 ‘Astronomy of Star Positions’, Frederick Ungar Publishing Co., New York.

    Google Scholar 

  • Explanatory Supplement to the Astronomical Ephemeris and the American Ephemer is and Nautical Almanac.

  • Fricke, W., 1985 ‘Fundamental Catalogues, Past, Present and Future’ Celestial Mechanics, in press.

  • Fricke, W. 1979 ‘Methods of Compiling a Fundamental Reference System’ Colloquium on European Satellite Astrometry, Padova.

  • Fricke, W. 1972 ‘Fundamental System of Positions and Proper Motions,’Annual Review of Astronomy and Astrophysics,10.

  • Markowitz, W. M. 1985 Private communication.

  • Mueller, I. I. 1969Spherical and Practical Astronomy as applied to Geodesy. Frederick Ungar Publishing Co., New York.

    Google Scholar 

  • Newcomb, S. 1906 ‘A Compendium of Spherical Astronomy’, Dover Publications Inc., New York, New York.

    Google Scholar 

  • Proceedings of the Sixteenth General Assembly, Grenoble 1976, Transactions of the I.A.U., VolumeXV1B, 1977.

  • Williams, J. G. and Melbourne, W. G. 1982 ‘Comments on the Effect of Adopting New Precession and Equinox Corrections’ inHigh-Precision Earth Rotation and Earth-Moon Dynamics, ed. by O. Calame, D. Reidel Publishing Co., Pages 293–303.

  • Woolard, E. W. and Clemence, G. M. (1966)Spherical Astronomy, Academic Press, New York and London.

    Google Scholar 

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Seidelmann, P.K. Fundamental reference systems; Past, present, and future. Celestial Mechanics 37, 199–207 (1985). https://doi.org/10.1007/BF02285046

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  • DOI: https://doi.org/10.1007/BF02285046

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