Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-26T04:39:50.159Z Has data issue: false hasContentIssue false

Investigation of the Motion of Periodic Comet Stephan-Oterma

Published online by Cambridge University Press:  14 August 2015

M. Ya. Shmakova*
Affiliation:
Institute for Theoretical Astronomy, Leningrad, U.S.S.R.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The orbit of P/Stephan-Oterma has been determined using 128 observations at the two apparitions (1867 and 1942) and taking into account perturbations by Venus to Neptune. The evolution of the comet's orbit has been studied over the interval 1660–2060.

Type
Part III/Motions of the Short-Period Comets
Copyright
Copyright © Reidel 1972 

References

Becker, L.: 1891, Monthly Notices Roy. Astron. Soc. 51, 475.CrossRefGoogle Scholar
Dubyago, A. D.: 1943, Astron. Tsirk . No. 17.Google Scholar