Discussion Overview
The discussion centers on whether the Sun creates different geodesics for each planet in the context of general relativity (GR). Participants explore the implications of geodesic motion for planets, the influence of the Sun's mass, and the complexities introduced by the planets' own gravitational effects.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
Main Points Raised
- Some participants propose that the geodesics are influenced by the mass, energy, and momentum distribution of the Sun and planets, suggesting that the Sun's mass has a dominant effect.
- One participant mentions that while planets generally follow geodesics in the Sun's curved spacetime, the actual motion of planets like Earth is affected by their own gravitational influence, complicating the notion of geodesic motion.
- Another participant introduces the idea that the Earth and other planets do not follow geodesics due to interactions with other forces, such as electromagnetic forces, and that this is a question of the individual particles that make up these extended objects.
- There is a discussion about the differences between a "world line" and a "bundle of world lines," with some participants questioning whether the center of an extended object can be said to follow a geodesic.
- One participant raises the question of whether intrinsic properties like spin affect geodesic motion, suggesting that this could complicate the understanding of particle behavior in curved spacetime.
- Concerns are expressed about the complexity of the topic, with some participants suggesting that the original poster may not fully grasp the concept of geodesics.
Areas of Agreement / Disagreement
Participants express differing views on the nature of geodesics for planets, with some asserting that planets follow distinct geodesics while others argue that their paths are influenced by additional factors. The discussion remains unresolved, with multiple competing perspectives presented.
Contextual Notes
Participants note that the background geometry of spacetime is not well-defined in the presence of massive bodies like Earth, complicating the analysis of geodesic motion. There are also references to approximation schemes and alternative theories of gravity that may affect the understanding of geodesics.