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

Автор(и)

  • S. O. Yasenev Department "Aerospace Surveying", National Aviation University, Ukraine
  • K. O. Radchenko 2Department of Computer Engineering, National Technical University of Ukraine “Kyiv Polytechnic Institute”,

DOI:

https://doi.org/10.18524/1810-4215.2016.29.85237

Ключові слова:

satellites of planets, gravitational field, Roche limit, Hill sphere, mass

Анотація

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.

 

Посилання

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Vidmachenko A.P., Morozhenko O.V., 2012, The study of the satellites surfaces and the rings of the giant planets Kyiv, DIA, 255 pp. (in Ukrainian).

Vidmachenko A. P., Morozhenko O. V.: 2014, K. The physical characteristics of surface Earth-like planets, dwarf planets and small, and their companions, according to distance studies. Kyiv, Profi, 388 pp. (in Ukrainian).

Yasenev S.O., 2015: Od. Astron. Publ., 28(1), 88.

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Опубліковано

2016-12-02

Номер

Том 29 (2016)

Розділ

Сонце та Сонячна система

Ліцензія

Авторське право (c) 2016 Odessa Astronomical Publications

Creative Commons License

Ця робота ліцензується відповідно до Creative Commons Attribution-NonCommercial 4.0 International License.

Відповідно Закону України про авторське право і суміжні права N 3792-XII від 23 грудня 1993 року