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The motion of Hyperion: On the accuracy of the observations

Published online by Cambridge University Press:  25 May 2016

Nikolai O. Kirsanov*
Affiliation:
Institute for Theoretical Astronomy, Kutuzova 10, St. Petersburg, Russia [email protected]

Abstract

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93 observations of the seventh satellite of Saturn, Hyperion, with 473 observations of Titan—Saturn's sixth and the most massive satellite and the one nearest to Hyperion—are considered. The observations were made in 1967–1981 at several observatories. The values of (O–C) across and along the orbits are obtained. The normality of the distributions of (O–C) is studied.

Type
Part III - Satellites: Theory and Ephemerides
Copyright
Copyright © Kluwer 1996 

References

1. Bulirsh, R., Stoer, J. (1966) “Numerical treatment of ordinary differential equations by extrapolation methods”, Numerische Mathematik, 8 1.CrossRefGoogle Scholar
2. Burns, J. A. (ed.). (1977) Planetary Satellites, University of Arizona Press, Arizona.Google Scholar
3. Kulikov, D. K., Batrakov, Yu. V. (1960) “Method for improving orbits of artificial satellites of the Earth, using observations when time is only approximately known”, Bull. ITA, 7(7), 554.Google Scholar
4. Kirsanov, N. O. (1995) The Orbits of Hyperion and Titan from the 1967–1981 Observations, Astronomy Letters, 21(2), 231.Google Scholar
5. Woltjer, J. (1928) The motion of Hyperion, Annalen van de Sterrewacht te Leiden 16(3).Google Scholar