Out-of-plane equilibrium points in the rotating mass dipole model with non-spherical radiating bodies

Key Points

• Unique equilibrium points emerge from the rotating mass dipole model with non-spherical bodies, indicating complex gravitational interactions.
• These points vary significantly when analyzing non-spherical radiating bodies, with shifts in stability under specific conditions.
• Observational analysis highlights out-of-plane dynamics as crucial, enriching understanding of gravitational systems and their behaviors.
• Such findings may enable advancements in models predicting celestial mechanics and gravitational phenomena for complex shapes.