English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

In a synodic-pulsating dimensionless coordinate, with a luminous primary and an oblate secondary, we examine the effects of radiation pressure, oblateness (quadruple and octupolar i.e. 2 4 J and J ) and eccentricity of the orbits of the primaries on the triangular points 4,5 L in the ER3BP. 2 4 J and J have been shown to disturb the motion of an infinitesimal body and 4 J particularly has significant effects on a satellite’s secular perturbation and orbital precessions. The influence of these parameters on the triangular points of Zeta Cygni, 54 Piscium and Procyon A/B are highlighted in this study. Triangular points are stable in the range 0 C μ μ < < and their stability is affected by said parameters.

international journal of advanced research in mathematics

Effect of Oblateness of the Secondary up to &lt;i&gt;J&lt;sub&gt;4&lt;/sub&gt; &lt;/i&gt;on &lt;i&gt;L&lt;sub&gt;4,5&lt;/sub&gt;&lt;/i&gt; in the Photogravitaional ER3BP