Discussion Overview
The discussion revolves around the concept of time dilation in the context of galactic gravitational mass and its implications for the observed acceleration of stars in galaxies. Participants explore the relationship between rotational speeds, gravitational potential, and relativistic effects, questioning whether time dilation could account for discrepancies in galaxy rotation curves.
Discussion Character
- Exploratory
- Debate/contested
- Technical explanation
Main Points Raised
- Some participants propose that time dilation could explain the observed acceleration of stars at varying distances from galactic centers, questioning what "time" is used in calculations.
- Others argue that the relativistic effects due to tangential speeds and changes in gravitational potential are too small to account for the discrepancies observed in galaxy rotation curves.
- A participant notes that while relativistic effects exist at any speed, they are negligible at the speeds typical of stars in galaxies.
- There is a discussion about the need for research or papers that quantify the time dilation effects between the center and the outskirts of galaxies, with some participants expressing skepticism about the significance of these effects.
- Some participants emphasize the complexity of galaxy dynamics and suggest that astrophysicists have already considered gravitational time dilation in their models.
- Concerns are raised about the lack of simple estimates or formulas to explain the insignificance of time dilation effects in layman's terms.
Areas of Agreement / Disagreement
Participants generally disagree on the significance of time dilation in explaining galaxy rotation curves. While some acknowledge the existence of relativistic effects, they contend that these effects are too small to be relevant, whereas others question the adequacy of existing explanations and seek further evidence.
Contextual Notes
Participants note that the calculations of time dilation and relativistic effects depend on specific parameters such as the mass of the galaxy and the distance from the galactic center, which may not yield significant results. There is also mention of the complexity of galaxy dynamics and the potential for overlooked factors in existing models.