SUMMARY
A nuclear explosion can be seen from low Earth orbit (LEO) due to its immense brightness and size. Observers in LEO can detect the initial flash of a nuclear detonation, which is significantly brighter than most manmade structures. While the average nuclear weapon yields between 100-300 kilotons in the U.S. and up to 500 kilotons in Russia, even smaller explosions can be visible under optimal conditions. The discussion highlights that atmospheric absorption may obscure some visual wavelengths, but the explosion's brightness would still be detectable from orbit.
PREREQUISITES
- Understanding of low Earth orbit (LEO) and its altitude.
- Familiarity with nuclear weapon yield measurements (kilotons and megatons).
- Knowledge of atmospheric effects on light and visibility.
- Basic concepts of visual wavelength energy and its absorption.
NEXT STEPS
- Research the visibility of nuclear explosions from different altitudes and conditions.
- Explore the effects of atmospheric absorption on light from nuclear detonations.
- Learn about the historical context and impact of the 57 megaton hydrogen bomb detonated by Russia in 1961.
- Investigate the capabilities of gamma ray and x-ray telescopes in detecting high-energy events from space.
USEFUL FOR
This discussion is beneficial for astrophysicists, military analysts, and anyone interested in the visibility of large-scale explosions from space, as well as those studying the effects of nuclear detonations on the environment.