Discussion Overview
The discussion revolves around the possibility of astronomical objects, particularly moons, having their own satellites. Participants explore the physical limitations, dynamic stability, and hierarchical structures of orbits within celestial systems, touching on theoretical and observational aspects.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
Main Points Raised
- Some participants propose that while planets orbit stars and satellites orbit planets, there may be physical limitations preventing moons from having their own satellites.
- Others discuss the concept of gravitational hierarchies, suggesting that while theoretically possible, dynamic stability issues complicate the existence of satellites around moons.
- A participant notes that for a moon to have a satellite, it must be sufficiently far from its planet and relatively massive to maintain a stable Hill sphere.
- Concerns are raised about the stability of orbits due to gravitational anomalies and the lumpiness of smaller celestial bodies.
- Some participants mention that while Apollo missions orbited the Moon, these were not stable long-term orbits, indicating that short-term orbits may be possible but not sustainable over astronomical timescales.
- There are references to natural examples, such as Saturn's moon Rhea potentially having a ring, although this remains unconfirmed.
- Participants highlight instances of smaller celestial bodies, like asteroids, having their own moons, suggesting that the dynamics may differ from those of larger bodies.
- Discussion includes the LaGrange relationships of certain objects, which complicate the classification of these bodies as independent satellites.
Areas of Agreement / Disagreement
Participants express multiple competing views on the feasibility of moons having satellites, with no consensus reached on the topic. Some acknowledge the theoretical possibility while others emphasize the practical limitations and dynamic stability issues.
Contextual Notes
Limitations include the complexity of the N-body problem, the lack of stable orbits for smaller bodies, and the specific conditions required for a moon to capture a satellite. The discussion also reflects on the varying definitions of what constitutes a satellite in different gravitational contexts.
Who May Find This Useful
This discussion may be of interest to those studying celestial mechanics, gravitational dynamics, or the formation of celestial bodies in astrophysics.