SUMMARY
The discussion centers on the visibility limits of stars from the International Space Station (ISS) for individuals with 20/15 vision. Participants debate the magnitude of stars visible to the naked eye, concluding that while amateur astronomers during wartime could see 8th magnitude stars, visibility decreases significantly due to atmospheric extinction. Key factors affecting visibility include molecular absorption, Rayleigh scattering, and aerosol scattering, which collectively result in a total extinction effect of approximately 0.28 magnitudes per air mass at sea level. The Hubble Space Telescope (HST) can detect stars up to 30th magnitude using advanced technology, which is unattainable with the naked eye.
PREREQUISITES
- Understanding of astronomical magnitude scales
- Familiarity with atmospheric extinction concepts
- Knowledge of Rayleigh scattering and its effects on visibility
- Basic principles of telescope optics and CCD technology
NEXT STEPS
- Research the effects of atmospheric conditions on astronomical observations
- Learn about the Hubble Space Telescope's imaging capabilities and technology
- Explore the concept of sky glow and its impact on stargazing
- Investigate advanced telescope designs and their performance at different altitudes
USEFUL FOR
Astronomers, astrophysics students, and anyone interested in the effects of atmospheric conditions on stargazing and astronomical observations.