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Please use this identifier to cite or link to this item: https://elib.bsu.by/handle/123456789/211337
Title: Моделирование эквипотенциальных поверхностей двойной звезды
Authors: Клищенко, Анатолий Петрович
Хвалей, Сергей Владимирович
Шуппяк, Вячеслав Иванович
Issue Date: 2003
Publisher: Минск : БГУ
Citation: Вестник Белорусского государственного университета. Сер. 1, Физика. Математика. Информатика. – 2003. - № 3. – С. 43-48.
Abstract: The method of computer simulation of a gravitational field structure of the binary star revolving around the common mass center with constant angular speed, in rotating system of coordinates, is considered in this article. The given method allows building the equipotential surfaces corresponding to any value of effective potential. The created program illustrates position of all Lagrangian libration points and Roche cavities and can calculate parameters of a gravitational field in any point of space. Besides, this method allows to model equipotential surfaces for single stars, and also for any planetary and artificial systems which are situating in gravitational interaction. It can be applied as a methodical illustration in a university course of the general astronomy and astrophysics.
URI: http://elib.bsu.by/handle/123456789/211337
ISSN: 0321-0367
Appears in Collections:2003, №3 (сентябрь)

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