330 likes | 450 Vues
Explore the complexities of Earth's atmosphere through its evolution from a primary to a secondary atmosphere, with key components such as hydrogen, helium, and carbon dioxide. Delve into geological features shaped by tectonic activity, including mountains, volcanoes, and craters. Discover the structure of Earth's interior, from the crust and mantle to the outer and inner core, along with the conditions necessary for generating the planet's magnetic field. Learn how these elements interconnect to shape our dynamic planet.
E N D
Primary Atmosphere: - H, He Secondary Atmosphere: - CO2 (90%), N, Sulfur Dioxide, H2O vapor
Primary Atmosphere: - H, He Secondary Atmosphere: - CO2 (90%), N, Sulfur Dioxide, H2O vapor Current Atmosphere: - N2 (78%), O2 (21%), CO2 (0.03%), H2O vapor
Geologic Features: - Mountains, Volcanoes, Craters - Erosional Features - Plate tectonics
The Earth’s Interior Crust, Silicate rock, 5-50 km, Solid
The Earth’s Interior Mantle- Basaltic Rock, 2850 km thick, Plastic
The Earth’s Interior Outer Core- Iron/Nickel, 2200 km thick, Liquid
The Earth’s Interior Inner Core- Iron/Nickel, 1300 km radius, Solid
Conditions for a Planetary Magnetic Field 1. Liquid/Molten core 2. Core is electrically conducting 3. Rapid rotation