Discussion Overview
The discussion explores the hypothetical scenario of uranium gathering in sufficient quantities to form a star-like structure, specifically focusing on the implications of fission versus fusion processes in such a configuration. Participants examine the feasibility of a "fissioning star" and the conditions required for uranium to condense into a stable form, touching on theoretical and conceptual aspects of astrophysics.
Discussion Character
- Exploratory
- Debate/contested
- Conceptual clarification
Main Points Raised
- Some participants question whether uranium could gather in enough quantities to prevent a chain reaction from occurring, which would disrupt the formation of a stable structure.
- Others argue that the critical concentration of Uranium-235 necessary for a chain reaction likely cannot be achieved in a natural gas cloud, making the formation of a "weapons-grade uranium star" improbable.
- One participant notes that the natural fusion process in stars ceases at iron, suggesting that a "fissioning star" is self-contradictory and cannot exist.
- Another participant introduces the idea of redefining what constitutes a "star" if such a fissioning body were to exist, proposing a new term "rats" for a reverse star.
- Concerns are raised about the energy released during fission potentially blowing apart any condensing uranium cloud before it could form a stable structure.
- Some participants express skepticism about the existence of a Goldilocks zone around a fission-type star, likening it to a "bungee bomb" due to the violent reactions involved.
- A participant suggests that the concept could serve as a basis for a math/physics/computer science simulation homework problem.
Areas of Agreement / Disagreement
Participants generally agree that the term "star" is traditionally associated with fusion processes, leading to a consensus that a "fissioning star" is a problematic concept. However, multiple competing views remain regarding the feasibility and implications of uranium gathering in sufficient quantities, and the discussion remains unresolved.
Contextual Notes
Limitations include the lack of calculations to support claims about the conditions necessary for fission versus fusion, as well as the dependence on definitions of what constitutes a star.