Satellite orbital dynamics in binary stellar systems

Authors

Mariam I. Idica ⋅ PH Institute of Mathematical Sciences and Physics, University of the Philippines Los Baños
Teodorick Barry R. Manguerra ⋅ PH Institute of Mathematical Sciences and Physics, University of the Philippines Los Baños
Alexandra B. Santos ⋅ PH Institute of Mathematical Sciences and Physics, University of the Philippines Los Baños
Rogel Mari D. Sese ⋅ PH Institute of Mathematical Sciences and Physics, University of the Philippines Los Baños

Abstract

The orbital dynamics of a satellite in a bipolar gravitational field was obtained using a computer simulation. The theoretical orbital dynamics calculations were done using the "Restricted 3-Body Problem" approach (analytic) and the "Summation of Gravitational Forces" Approach (numerical). The trajectories of a single satellite moving in several binary configurations were obtained and the energy content of system was also described.

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Issue

2004: Proceedings of the 22nd Samahang Pisika ng Pilipinas Physics Congress

Twenty five years of promoting diversity in physics
25-27 October 2004, Tagbilaran City, Bohol

Article ID

SPP-2004-3C-03

Section

Theoretical and Computational Physics

Published

2004-10-25

How to Cite

[1]

MI Idica, TBR Manguerra, AB Santos, and RMD Sese, Satellite orbital dynamics in binary stellar systems, Proceedings of the Samahang Pisika ng Pilipinas 22, SPP-2004-3C-03 (2004). URL: https://proceedings.spp-online.org/article/view/SPP-2004-3C-03.