SUMMARY
The average temperature of the universe is approximately 2.7 Kelvin, primarily determined by the Cosmic Microwave Background (CMB) radiation, a remnant from the Big Bang. While space itself lacks temperature as it is not a material substance, the presence of interstellar and intergalactic gas allows for the assignment of temperature and pressure to these regions. Interstellar space can reach temperatures exceeding one million Kelvins, yet due to its extremely low density, it would not warm a human body, which would instead experience rapid cooling. In contrast, intergalactic gas can reach temperatures of up to 50 million Kelvins, influenced by nearby galaxies and shock waves.
PREREQUISITES
- Understanding of Cosmic Microwave Background (CMB) radiation
- Familiarity with concepts of temperature and matter
- Knowledge of interstellar and intergalactic medium properties
- Basic principles of thermodynamics in space environments
NEXT STEPS
- Research the properties and implications of Cosmic Microwave Background radiation
- Explore the characteristics of the interstellar medium and its temperature variations
- Investigate the effects of shock waves on intergalactic gas temperatures
- Learn about the thermodynamics of space and its impact on human physiology
USEFUL FOR
Astronomers, astrophysicists, educators, and anyone interested in understanding the thermal dynamics of space and the universe.