SUMMARY
The average annual accumulation of cosmic dust on Earth is approximately 4 x 107 kg/year, translating to a deposition rate of about 10-7 kg/m2/year across the Earth's surface area of roughly 5 x 1014 m2. This accumulation consists of materials such as meteors and stardust, specifically in dust form, excluding gases and liquids. The typical density of rock is estimated between 3-5 x 103 kg/m3, resulting in a negligible depth of less than 10-10 m/year.
PREREQUISITES
- Understanding of cosmic dust composition and sources
- Familiarity with basic physics concepts regarding mass and density
- Knowledge of Earth's surface area calculations
- Ability to interpret scientific papers and data
NEXT STEPS
- Research the methods for measuring cosmic dust accumulation
- Explore the implications of cosmic dust on Earth's geology
- Investigate the relationship between cosmic dust and climate change
- Learn about the composition and origin of meteoric materials
USEFUL FOR
Astronomers, geologists, environmental scientists, and anyone interested in the impact of cosmic materials on Earth’s surface and atmosphere.