Venus, as Earth’s nearest planetary neighbor and of similar size, presents unique opportunities for scientific and defense missions. These missions may include helio-physics studies, space weather monitoring, or tracking meteoroid threats to Earth’s orbital path. Despite this, there has been limited exploration of periodic orbits in the Sun–Venus system.
This research identifies 90 resonant periodic orbits and their associated families within the Circular Restricted Three-Body Problem (CR3BP) framework, incorporating solar radiation pressure as a perturbation. By utilizing Poincaré maps and a continuation method with varying Jacobi constants, a catalog of resonant orbits is created.
Additionally, stability analyses are performed for each orbit family, examining eigenvalue structures to identify bifurcation points. The results offer critical insights into the stability and usability of these orbits, contributing to mission planning and celestial mechanics studies.
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