SPECIFICATION OF LIMITS OF POSSIBLE EXISTENCE OF SATELLITES IN THE GRAVITATIONAL FIELD OF PLANETS

Journal Title: Odessa Astronomical Publications - Year 2016, Vol 29, Issue

Abstract

It is known that the satellites of the planets may exist in the area, which is bounded on one side by Rocha limit, on the other – Hill sphere. The article deals with the determination of the Rocha limits and Hill sphere of satellites of some planets in the solar system. This analysis revealed some features and identified the main factors influencing the setting of these parameters. Roche limits and Hill sphere parameters of the largest satellites of the planets of the solar system have been specified.

Authors and Affiliations

S. O. Yasenev, K. O. Radchenko

Keywords

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  • EP ID EP379841
  • DOI 10.18524/1810-4215.2016.29.85237
  • Views 72
  • Downloads 0

How To Cite

S. O. Yasenev, K. O. Radchenko (2016). SPECIFICATION OF LIMITS OF POSSIBLE EXISTENCE OF SATELLITES IN THE GRAVITATIONAL FIELD OF PLANETS. Odessa Astronomical Publications, 29(), 226-228. https://europub.co.uk./articles/-A-379841