Elliptic Restricted Three-Body Problem - Ashagwu, Blessing Samuel
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This study examines the triangular points in the elliptic restricted three-body problem when both primaries are sources of radiation as well as oblate spheroids with oblateness up to zonal harmonic J4. The positions of triangular points and their critical mass ratio are seen to be affected by the eccentricity, semi major axis, radiation and oblateness of both primaries up to zonal harmonic J4. The effects of the said parameters on the locations of the triangular points of 61 CYGNI and STRUVE 2398 was highlighted. The triangular points of these systems are found to be unstable.

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Produktbeschreibung
This study examines the triangular points in the elliptic restricted three-body problem when both primaries are sources of radiation as well as oblate spheroids with oblateness up to zonal harmonic J4. The positions of triangular points and their critical mass ratio are seen to be affected by the eccentricity, semi major axis, radiation and oblateness of both primaries up to zonal harmonic J4. The effects of the said parameters on the locations of the triangular points of 61 CYGNI and STRUVE 2398 was highlighted. The triangular points of these systems are found to be unstable.
Autorenporträt
Blessing Samuel Ashagwu is a PhD research student at the Department of Mathematics, Ahmadu Bello University, Zaria, Nigeria. Her research interest area is Applied Mathematics (Space Dynamics). She has co-authored four international journal articles. She is a visiting-lecturer with Elite International College of Health and Technology, Zaria.