As you travel from the Earth's surface to its center, you would experience significant increases in both temperature and pressure. The temperature can rise from about 15°C at the surface to over 4,000°C at the center, while pressure escalates from 1 atmosphere to approximately 3.6 million atmospheres. The materials also change, moving from solid crust to liquid outer core and then to solid inner core.
;
When traveling from the Earth's surface to its center, we observe significant changes in temperature, pressure, and material. Here's a breakdown of two changes you would see in each aspect:
Temperature:
Increase in Temperature: As you descend deeper into the Earth, the temperature steadily increases. This increase is due to heat produced by radioactive decay and residual heat from the Earth's formation. For instance, in the crust, the temperature rises about 25–30 degrees Celsius for every kilometer descended.
Near the Core: As you approach the Earth's core, the temperature can rise to about 5,000 to 7,000 degrees Celsius. The inner core, composed mainly of iron and nickel, is as hot as the surface of the sun.
Pressure:
Increase in Pressure: The pressure also increases significantly as you travel inward. This is due to the weight of the overlying rocks pressing down. At times, this increase is approximately 1 giga-pascal per 33 kilometers.
Core Pressure: At the Earth's core, pressures are extreme, reaching about 360 gigapascals. This immense pressure is why the inner core is solid despite the high temperatures.
Material:
Crust and Mantle Composition: Near the surface, the Earth is composed of silicate rocks. The crust is primarily made of lighter elements like silicon and aluminum, whereas the mantle below is richer in magnesium and iron.
Core Composition: As you move towards the core, the material changes from rocky compositions to metallic ones. The outer core is liquid iron and nickel, while the inner core is solid due to its high pressure.
These changes in temperature, pressure, and material composition are crucial for understanding the Earth's internal processes, including plate tectonics and the generation of its magnetic field.