A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2017; you can also visit the original URL.
The file type is application/pdf.
A general solution to non-collinear equilibria in terms of largest root (κ) of confocal oblate spheroid
2016
International Journal of Advanced Astronomy
Preserved Fulltext
<p>This paper deals with the existence of non-collinear equilibria in restricted three-body problem when less massive primary is an oblate spheroid and the potential of oblate spheroid is in terms of largest root of confocal oblate spheroid. This is found that the non-collinear equilibria are the solution of the equations r<sub>1</sub> = n<sup>-2/3</sup> and κ = 1 – a<sup>2</sup>, where r<sub>1</sub> is the distance of the infinitesimal mass from more massive primary, n is mean-motion of
doi:10.14419/ijaa.v4i1.5587
fatcat:aooebhhrnfguzesunznqbapzvy