Modelling of motion of bodies near triangular lagrangian points

Скорочена інформація про документ
dc.contributor.authorBobrov, O. A.
dc.date.accessioned2015-02-24T08:53:58Z
dc.date.available2015-02-24T08:53:58Z
dc.date.issued2014
dc.descriptionOdessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2014 . – Vol.27, I. 1.uk
dc.description.abstractIn this paper, we consider a system of three bodies connected by gravity, two of which are of comparable mass (the Sun and Jupiter), and the third is negligible and it is located in one of the triangular Lagrange points (restricted 3 – body problem). We used the equations of motion in a planar coordinate system that rotates together with massive bodies. Several programs have been written in the programming environment Pascal ABC, in order to build the trajectory of a small body, to indicate the osculating orbit around a massive body, to display equipotential surfaces.uk
dc.identifier.citationOdessa Astronomical Publicationsuk
dc.identifier.urihttps://dspace.onu.edu.ua/handle/123456789/5907
dc.language.isoenuk
dc.publisherAstroprintuk
dc.relation.ispartofseries;V. 27, I. 1, P. 41-42.
dc.subjectstarsuk
dc.subjectbinaryuk
dc.subjectcelestial mechanicsuk
dc.subjectSolar systemuk
dc.subjectasteroidsuk
dc.titleModelling of motion of bodies near triangular lagrangian pointsuk
dc.typeArticleuk
Файли
Контейнер файлів
Зараз показуємо 1 - 1 з 1
Ескіз
Назва:
18.pdf
Розмір:
462.04 KB
Формат:
Adobe Portable Document Format
Завантажити
Ліцензійна угода
Зараз показуємо 1 - 1 з 1
Ескіз недоступний
Назва:
license.txt
Розмір:
1.71 KB
Формат:
Item-specific license agreed upon to submission
Опис:
Завантажити
Зібрання
Odesa Astronomical Publications