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Numerical theory of movement of the major Saturnian satellites

Transactions of IAA RAS, issue 21, 162–166 (2010)

Keywords: радиоинтерферометрия со сверхдлинными базами, спутники Сатурна, численная теория движения спутника, эфемерида TASS1.7

Abstract

The numerical theory of the major Saturnian satellites movement was con-structed by numerical integration of satellites movement equation. Integration was done by Everhart's method. 5254 absolute observatiobns were used. Perturbations of Sun, Saturn and satellites mutual attraction were taken into account. As result coefficients of Chebyshev polynomials for period 1965-2015 were obtained. Initial coordinates and velocities, Saturn and satellites masses and J2 of Saturn potential were improved. Obtained ephemerides were compared with ephemerides TASS1.7.

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G. Kosmodamiansky. Numerical theory of movement of the major Saturnian satellites // Transactions of IAA RAS. — 2010. — Issue 21. — P. 162–166.

@article{kosmodamiansky2010,
  abstract = {The numerical theory of the major Saturnian satellites movement was con-structed by numerical integration of satellites movement equation. Integration was done by Everhart's method. 5254 absolute observatiobns were used. Perturbations of Sun, Saturn and satellites mutual attraction were taken into account. As result coefficients of Chebyshev polynomials for period 1965-2015 were obtained. 
Initial coordinates and velocities, Saturn and satellites masses and J2 of Saturn potential were improved. 
Obtained ephemerides were compared with ephemerides TASS1.7.},
  author = {G. Kosmodamiansky},
  issue = {21},
  journal = {Transactions of IAA RAS},
  keyword = {радиоинтерферометрия со сверхдлинными базами, спутники Сатурна, численная теория движения спутника, эфемерида TASS1.7},
  pages = {162--166},
  title = {Numerical theory of movement of the major Saturnian satellites},
  url = {http://iaaras.ru/en/library/paper/715/},
  year = {2010}
}

TY  - JOUR
TI  - Numerical theory of movement of the major Saturnian satellites
AU  - Kosmodamiansky, G.
PY  - 2010
T2  - Transactions of IAA RAS
IS  - 21
SP  - 162
AB  - The numerical theory of the major Saturnian satellites movement was
con-structed by numerical integration of satellites movement
equation. Integration was done by Everhart's method. 5254 absolute
observatiobns were used. Perturbations of Sun, Saturn and satellites
mutual attraction were taken into account. As result coefficients of
Chebyshev polynomials for period 1965-2015 were obtained.   Initial
coordinates and velocities, Saturn and satellites masses and J2 of
Saturn potential were improved.   Obtained ephemerides were compared
with ephemerides TASS1.7.
UR  - http://iaaras.ru/en/library/paper/715/
ER  -