Discussion Overview
The discussion explores the potential effects of photons emitted by stars on the motion of other stars and star systems, particularly focusing on concepts like radiation pressure and its implications for cosmic expansion. Participants also touch on the relationship between these effects and dark matter and dark energy, considering both theoretical and observational aspects.
Discussion Character
- Exploratory
- Technical explanation
- Conceptual clarification
- Debate/contested
Main Points Raised
- One participant questions whether photons from the sun can affect the flight path of asteroids and extends this inquiry to nearby star systems, suggesting a possible slight push between star systems.
- Another participant asserts that while photons do not significantly modify the orbits of other stars, they acknowledge that there could be a slight push due to radiation pressure, although it is negligible.
- A participant clarifies that dark matter and dark energy are relevant only on very large scales, which do not pertain to the interactions between nearby stars.
- One participant references a lecture by Susskind discussing radiation pressure's effects on cosmological expansion, noting its significance in the early universe but not in the current context of star interactions.
- Another participant confirms that the photons affecting cosmological expansion during the radiation era originated from the cosmic microwave background rather than from stars.
Areas of Agreement / Disagreement
Participants express varying views on the extent to which photons can influence star systems, with some suggesting a negligible effect while others emphasize the lack of significant impact on star orbits. There is no consensus on the relevance of these effects to dark matter and dark energy calculations.
Contextual Notes
Participants acknowledge the low intensity of light from one star affecting another and the massive nature of stars, which contribute to the negligible measurable effects of radiation pressure. The discussion also highlights the distinction between the effects of stellar photons and those from the cosmic microwave background.