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Full metadata record
DC Field | Value | Language |
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dc.contributor.author | Bobrov, O. A. | - |
dc.date.accessioned | 2015-02-24T08:53:58Z | - |
dc.date.available | 2015-02-24T08:53:58Z | - |
dc.date.issued | 2014 | - |
dc.identifier.citation | Odessa Astronomical Publications | uk |
dc.identifier.uri | http://dspace.onu.edu.ua:8080/handle/123456789/5907 | - |
dc.description | Odessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2014 . – Vol.27, I. 1. | uk |
dc.description.abstract | In 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.language.iso | en | uk |
dc.publisher | Astroprint | uk |
dc.relation.ispartofseries | ;V. 27, I. 1, P. 41-42. | - |
dc.subject | stars | uk |
dc.subject | binary | uk |
dc.subject | celestial mechanics | uk |
dc.subject | Solar system | uk |
dc.subject | asteroids | uk |
dc.title | Modelling of motion of bodies near triangular lagrangian points | uk |
dc.type | Article | uk |
Appears in Collections: | Odessa Astronomical Publications |
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