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A Method of Integrating the Equations of Motion in Special Coordinates and the Elimination of a Discontinuity in the Theory of the Motion of Periodic Comet Wolf

Published online by Cambridge University Press:  14 August 2015

E. I. Kazimirchak-Polonskaya
E. I. Kazimirchak-Polonskaya*
Affiliation:
Institute for Theoretical Astronomy, Leningrad, U.S.S.R.

Abstract

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From the integration formulae of Numerov and Subbotin we have developed and programmed for an electronic computer a particular method for integrating the differential equations of cometary motion in special rectangular coordinates, with a variable step and allowing for all planetary perturbations and nongravitational effects over a time interval of 400 yr. Application of this method and our set of programmes to the investigation of the motion of P/Wolf permits us to eliminate the discontinuity that has hitherto existed in the theory on account of the comet's close approach to Jupiter in 1922.

Type
Part II/General Methods of Orbit Theory
Information
Symposium - International Astronomical Union , Volume 45: The Motion, Evolution of Orbits and Origin of Comets , 1972 , pp. 95 - 102
Copyright
Copyright © Reidel 1972 

References

Belyaev, N. A: 1972, this Symposium, p. 90.Google Scholar
Bokhan, N. A: 1972, this Symposium, p. 86.Google Scholar
Clemence, G. M.: 1943, Astron. Pap. Washington 11, part 1.Google Scholar
Clemence, G. M.: 1949, Astron. Pap. Washington 11, part 2.Google Scholar
Clemence, G. M.: 1954, Astron. Pap. Washington 13, part 5.Google Scholar
Clemence, G. M.: 1961, Astron. Pap. Washington 16, part 2.Google Scholar
Duncombe, R. L.: 1958, Astron. Pap. Washington 16, part 1.Google Scholar
Eckert, W. J., Brouwer, D., and Clemence, G. M.: 1951, Astron. Pap. Washington 12.Google Scholar
Kamieński, M.: 1933, Acta Astron. Ser. a. 3, 1.Google Scholar
Kamieński, M.: 1948, Bull. Acad. Polon. Sci. Lettres Ser. A 1.Google Scholar
Kamieński, M.: 1959, Acta Astron. 9, 53.Google Scholar
Kamieński, M. and Bielicki, M.: 1935, Repr. Astron. Obs. Warsaw Univ. 30, 270.Google Scholar
Kamieński, M. and Bielicki, M.: 1936, Repr. Astron. Obs. Warsaw Univ. 32, 1.Google Scholar
Kazimirchak-Polonskaya, E. I.: 1961, Trudy Inst. Teor. Astron. 7, 191.Google Scholar
Kazimirchak-Polonskaya, E. I.: 1967, Trudy Inst. Teor. Astron. 12, 24.Google Scholar
Kazimirchak-Polonskaya, E. I.: 1972a, this Symposium, p. 227.Google Scholar
Kazimirchak-Polonskaya, E. I.: 1972b, this Symposium, p. 373.Google Scholar
Kazimirchak-Polonskaya, E. I., Belyaev, N. A., and Terent'eva, A. K.: 1972, this Symposium, p. 462.Google Scholar
Morgan, H. R.: 1945, Astron. J. 51, 127.Google Scholar
Myachin, V. F.: 1962, Byull. Inst. Teor. Astron. 8, 537.Google Scholar
Newcomb, S.: 1895a, Astron. Pap. Washington 6, part 1, part 3.Google Scholar
Newcomb, S.: 1895b, The Elements of the Four Inner Planets and the Fundamental Constants of Astronomy , Washington.CrossRefGoogle Scholar
Numerov, B. V.: 1923, Trudy Gl. Ross. Astrofiz. Obs. 2, 188.Google Scholar
Subbotin, M. F.: 1927, Byull. Sredne-Aziat. Univ. Tashkent 16, 273.Google Scholar
Subbotin, M. F.: 1928, Byull. Sredne-Aziat. Univ. Tashkent 17, 21.Google Scholar
Subbotina, N. S.: 1965, Byull. Inst. Teor. Astron. 10, 143.Google Scholar