SUMMARY
The discussion centers on calculating the size of the Sun if it were composed of liquid hydrogen and helium instead of gas. Participants emphasize that the average density of the Sun is 1410 kg/m³, while liquid hydrogen has a density of only 70 kg/m³, indicating that the Sun is denser than liquid hydrogen. The conversation highlights that if the Sun were to lose its energy source, it would compress to a state comparable to a white dwarf, resulting in a radius similar to that of Earth. Ultimately, a liquefied Sun would be approximately 2.7 times larger in diameter than its current state.
PREREQUISITES
- Understanding of stellar composition and density
- Knowledge of the properties of hydrogen and helium
- Familiarity with concepts of gravity and compression in astrophysics
- Basic comprehension of white dwarf characteristics
NEXT STEPS
- Research the properties of liquid hydrogen and helium, including their densities
- Explore the concept of electron degeneracy in white dwarfs
- Study the average density variations within stars
- Read about stellar evolution and the lifecycle of stars
USEFUL FOR
Astronomers, astrophysics students, and anyone interested in stellar dynamics and the physical properties of celestial bodies will benefit from this discussion.