SUMMARY
The discussion centers on the claim of two planets discovered in perpendicular orbits relative to the existing nine planets. Participants express skepticism regarding the stability of such orbits due to gravitational perturbations from mass in the plane of the ecliptic. The conversation also highlights the ambiguity surrounding the definition of "planet," suggesting that the objects in question may be larger-than-usual entities in the Oort Cloud rather than traditional planets. Overall, the consensus leans towards the improbability of stable perpendicular orbits in the solar system.
PREREQUISITES
- Understanding of celestial mechanics and orbital dynamics
- Familiarity with the Oort Cloud and its characteristics
- Knowledge of the current definitions and classifications of celestial bodies
- Basic grasp of gravitational interactions in multi-body systems
NEXT STEPS
- Research the stability of orbits in celestial mechanics
- Explore the current definitions of planets by the International Astronomical Union (IAU)
- Investigate the characteristics and significance of the Oort Cloud
- Study gravitational perturbations and their effects on orbital paths
USEFUL FOR
Astronomers, astrophysicists, and science enthusiasts interested in planetary formation and orbital dynamics.