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The Updated Versions of Saturn`s Major Satellites Numerical Ephemerides

G. A. Kosmodamiansky

Transactions of IAA RAS, issue 46, 77–86 (2018)

DOI: 10.32876/ApplAstron.46.77-86

Keywords: producing ephemerides of satellites, optical observations, accuracy of ephemerides, numerical integration.

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Abstract

The numerical ephemerides of eight Saturn`s major satellites (Mimas, Enceladus, Tethys, Diona, Rhea, Titan, Hyperion, Iapetus) for the period 1870–2025 are prepared. The satellites motion theories are based on the method of differential correction and numerical integration. The dynamical model includes the mutual perturbations of the satellites, the Sun, the major planets, and Saturn`s oblateness. The coordinates and velosities initial values of the satellites were adjusted using a set of all available optical observational data (1874–2015). The residuals, their root-mean-square and comparison of our ephemerides with those produced by V. Lainey are given. The ephemerides are publicly available.

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G. A. Kosmodamiansky. The Updated Versions of Saturn`s Major Satellites Numerical Ephemerides // Transactions of IAA RAS. — 2018. — Issue 46. — P. 77–86. @article{kosmodamiansky2018, abstract = {The numerical ephemerides of eight Saturn`s major satellites (Mimas, Enceladus, Tethys, Diona, Rhea, Titan, Hyperion, Iapetus) for the period 1870–2025 are prepared. The satellites motion theories are based on the method of differential correction and numerical integration. The dynamical model includes the mutual perturbations of the satellites, the Sun, the major planets, and Saturn`s oblateness. The coordinates and velosities initial values of the satellites were adjusted using a set of all available optical observational data (1874–2015). The residuals, their root-mean-square and comparison of our ephemerides with those produced by V. Lainey are given. The ephemerides are publicly available.}, author = {G.~A. Kosmodamiansky}, doi = {10.32876/ApplAstron.46.77-86}, issue = {46}, journal = {Transactions of IAA RAS}, keyword = {producing ephemerides of satellites, optical observations, accuracy of ephemerides, numerical integration}, pages = {77--86}, title = {The Updated Versions of Saturn`s Major Satellites Numerical Ephemerides}, url = {http://iaaras.ru/en/library/paper/1878/}, year = {2018} } TY - JOUR TI - The Updated Versions of Saturn`s Major Satellites Numerical Ephemerides AU - Kosmodamiansky, G. A. PY - 2018 T2 - Transactions of IAA RAS IS - 46 SP - 77 AB - The numerical ephemerides of eight Saturn`s major satellites (Mimas, Enceladus, Tethys, Diona, Rhea, Titan, Hyperion, Iapetus) for the period 1870–2025 are prepared. The satellites motion theories are based on the method of differential correction and numerical integration. The dynamical model includes the mutual perturbations of the satellites, the Sun, the major planets, and Saturn`s oblateness. The coordinates and velosities initial values of the satellites were adjusted using a set of all available optical observational data (1874–2015). The residuals, their root-mean-square and comparison of our ephemerides with those produced by V. Lainey are given. The ephemerides are publicly available. DO - 10.32876/ApplAstron.46.77-86 UR - http://iaaras.ru/en/library/paper/1878/ ER -