Discussion Overview
The discussion revolves around the possibility of the existence of thousands of chemical elements under extreme conditions in space, such as high temperatures and pressures. Participants explore whether these conditions could lead to the formation of stable elements, particularly those that are currently unstable or have not been observed.
Discussion Character
- Exploratory
- Debate/contested
- Conceptual clarification
Main Points Raised
- Some participants propose that under extreme conditions, such as a trillion degrees Celsius, there could be more than the currently known 118 elements.
- There is a question about whether super high temperatures would facilitate the formation of stable elements or any elements at all.
- One participant mentions that in conditions like a supernova, higher atomic number elements could be created as they decay, but doubts that this would lead to a thousand elements.
- Another participant questions the possibility of a stability area for higher nuclei numbers, specifically around 150 protons.
- Concerns are raised about the absence of evidence for super-heavy elements, questioning why they have not been found on Earth or in stellar spectra despite billions of years of cosmic history.
- There is a suggestion that super-heavy elements might be produced in heavy ion colliders, and a discussion on whether the rapid decay of transactinides is due to their production in excited states.
- One participant notes a limit on the number of electrons in atomic shells, relating it to the fine structure constant.
Areas of Agreement / Disagreement
The discussion remains unresolved, with multiple competing views on the existence and stability of elements under extreme conditions. Participants express differing opinions on the feasibility of forming stable super-heavy elements and the implications of current scientific observations.
Contextual Notes
Participants acknowledge limitations in current understanding, including the dependence on specific conditions for element formation and the unresolved nature of isotopes that have not yet been produced.