Discussion Overview
The discussion revolves around the hypothetical scenario of the Sun being frozen, specifically exploring how much smaller it would be if its hydrogen and helium were in a liquid state. Participants engage in calculations, density comparisons, and the implications of gravitational compression on the Sun's size and density.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
- Mathematical reasoning
Main Points Raised
- Some participants suggest calculating the volume of the Sun's hydrogen and helium using their respective densities to visualize its size if frozen.
- Others argue that gravitational compression would significantly affect the density and volume, complicating simple calculations.
- A participant notes that the average density of the Sun is greater than that of liquid hydrogen, implying that the Sun would compress under its own gravity if it lost its energy source.
- One participant mentions that a liquefied Sun could be 2.7 times larger in diameter based on a specific density of hydrogen.
- Another participant raises a question about the similar densities of Jupiter and the Sun, prompting further exploration of density variations within the Sun.
- Some participants reflect on misconceptions about the nature of stars, particularly regarding their composition as gas and plasma.
Areas of Agreement / Disagreement
Participants express differing views on the feasibility of calculating the size of a frozen Sun, with some asserting that gravitational effects complicate the matter. There is no consensus on the exact implications of density and compression in this hypothetical scenario.
Contextual Notes
Limitations include the dependence on assumptions about the state of matter and the effects of gravity on the Sun's structure. The discussion does not resolve the complexities involved in the calculations or the physical implications of a frozen Sun.
Who May Find This Useful
This discussion may be of interest to those exploring astrophysics, stellar dynamics, and the properties of matter under extreme conditions.