Skip to main content
NAV
SCAN
COMM

Welcome to Earth 2025

Let's take a Journey to the center of the Earth

Scroll to begin your journey

The Exosphere

Welcome to the outermost layer of Earth's atmosphere, extending from about 700 km to 10,000 km above the surface.

  • The air is extremely thin here, with particles rarely colliding with each other
  • Many satellites orbit Earth within this region
  • The exosphere gradually fades into the emptiness of space
  • Temperatures can reach up to 1700°C during the day
Fun fact: The International Space Station orbits in the thermosphere, just below the exosphere
Scroll to continue your journey

The Thermosphere

Extending from 80 km to 700 km above Earth's surface, the thermosphere is where temperatures can reach up to 2,000°C, yet would feel cold to human skin due to the extremely thin air.

  • Home to the spectacular aurora borealis (Northern Lights) and aurora australis (Southern Lights)
  • The International Space Station orbits in the lower thermosphere
  • Contains the ionosphere, which reflects radio waves, enabling long-distance radio communication
  • Solar radiation causes air molecules to ionize, creating charged particles that interact with Earth's magnetic field

Did you know?

The thermosphere expands during periods of high solar activity, causing more drag on satellites and altering their orbits!

Continue your journey

The Mesosphere

The mesosphere extends from about 50 to 85 kilometers above the Earth's surface. It's the layer where temperatures decrease with height, reaching the coldest temperatures in Earth's atmosphere.

  • Most meteors burn up in this layer, creating "shooting stars"
  • Home to beautiful noctilucent clouds (night-shining clouds)
  • Temperatures can drop to -90°C (-130°F) at the mesopause
  • Too high for aircraft but too low for satellites to orbit

Did you know?

Noctilucent clouds are the highest clouds in Earth's atmosphere and can only be seen during twilight when the Sun is below the horizon.

Continue your journey

The Stratosphere

The stratosphere is the second major layer of Earth's atmosphere, extending from about 10-50 kilometers (6-31 miles) above Earth's surface. Here, the temperature increases with height due to absorption of ultraviolet radiation from the Sun.

  • Contains the ozone layer that absorbs and scatters harmful solar ultraviolet radiation
  • Commercial airplanes typically fly in the lower stratosphere to avoid turbulence
  • Very dry with almost no water vapor or weather
  • Strong horizontal winds that flow in bands around the globe

Ozone Shield in Action!

The ozone layer absorbs 97-99% of the Sun's medium-frequency ultraviolet radiation, protecting life on Earth from genetic damage.

Continue your journey

The Troposphere

The troposphere is the lowest layer of Earth's atmosphere, extending from the surface to about 8-15 kilometers high. This is where we live and where most weather occurs.

  • Contains about 75% of the atmosphere's mass and almost all water vapor
  • Temperature decreases with altitude - approximately 6.5°C per kilometer
  • Home to all our weather phenomena - clouds, rain, snow, and storms
  • The boundary where air pollution is trapped and can't easily escape

Click the buttons on the right to change weather conditions!

Entering Earth's interior next...
Crust thickness
(not to scale)

The Earth's Crust

The crust is Earth's outermost layer, a thin shell comprising less than 1% of Earth's volume. It's the layer we live on and where all familiar surface features are found.

  • Oceanic crust: 5-10 km thick, made primarily of basalt
  • Continental crust: 30-50 km thick, composed mainly of granite
  • Contains all known life and surface features - mountains, valleys, and ocean floors
  • Divided into tectonic plates that move on the semi-fluid mantle below

Did you know?

If Earth were the size of an apple, the crust would be as thin as the apple's skin!

Heading deeper...

The Upper Mantle

The upper mantle extends from the base of the crust (Mohorovičić discontinuity) to about 670 km deep. This region is characterized by partially molten rock that flows over geological time.

  • Contains the asthenosphere, a partially molten layer where rocks flow like a very slow-moving liquid
  • Temperatures range from about 500°C to 1,500°C
  • Convection currents in this layer drive plate tectonics and continental drift
  • Composed mainly of iron and magnesium-rich silicate rocks like peridotite and olivine

Did you know?

The upper mantle's asthenosphere allows the tectonic plates to move like a conveyor belt, at speeds of 2-10 cm per year!

Olivine Crystal Formation
Getting closer to the core...

The Lower Mantle

The lower mantle extends from 670 km to about 2,900 km depth, comprising over half of Earth's volume. This vast region experiences extreme pressures and temperatures that transform the physical properties of rock.

  • Temperatures reach 2,200°C to over 4,000°C near the core boundary
  • Pressures increase dramatically, reaching 1.3 million times atmospheric pressure
  • Composed primarily of bridgmanite (formerly called silicate perovskite)
  • The mysterious D" (D double-prime) layer forms the boundary with the outer core

Pressure Gauge

0 GPa
Earth's surface: 0 GPa
Core-mantle boundary: ~135 GPa

Did you know?

The mysterious D" (D double-prime) layer at the base of the lower mantle is one of Earth's most exotic regions, where seismic waves change behavior dramatically!

Approaching the outer core...

The Outer Core

The outer core is a 2,200 km thick layer of liquid metal, primarily iron and nickel, that surrounds the inner core. It's the only liquid layer within Earth's interior.

  • Temperature ranges from 4,400°C to 6,100°C
  • Rapid rotation and convection generate Earth's magnetic field
  • This "geodynamo" shields Earth from harmful solar radiation
  • Despite intense heat, the core's immense pressure prevents boiling
N
S

Did you know?

Earth's magnetic poles have completely reversed hundreds of times throughout Earth's history. The last reversal occurred about 780,000 years ago!

Inner core boundary: 6,100°C
Mid outer core: 5,250°C
Core-mantle boundary: 4,400°C
Almost at the center...

The Inner Core

The inner core is Earth's deepest layer, a solid sphere of iron and nickel approximately 1,220 km in radius. Despite extreme temperatures of up to 6,700°C, the core remains solid due to immense pressure.

  • Formed about 1-1.5 billion years ago as Earth cooled
  • Rotates slightly faster than the rest of Earth (superrotation)
  • Growing slowly at about 1mm in radius per year
  • Has a distinct east-west crystalline structure

Iron Crystal Lattice

The inner core's iron is crystallized in a hexagonal close-packed structure under extreme pressure.

Inner Core Growth

As the Earth cools, the inner core solidifies from the liquid outer core at a rate of approximately 1mm per year.

Journey complete! You've reached Earth's center.

Educational Resources

Expand your knowledge about Earth's layers with these carefully curated resources, activities, and learning materials.

Video

Earth's Layers Explained

A comprehensive explanation of Earth's atmospheric and internal layers with stunning visualizations.

Duration: 15 min
Activity

Build Earth Layers Model

Step-by-step guide to create your own model of Earth's layers using household materials.

Difficulty: Medium
Quiz

Earth Layers Challenge

Test your knowledge with this interactive quiz about Earth's atmospheric and internal structures.

20 Questions
Guide

Complete Earth Layers Guide

A comprehensive study guide with diagrams, facts, and explanations about all Earth layers.

PDF • 24 pages
Video

Plate Tectonics and Earth's Structure

Understand how plate tectonics relate to Earth's interior structure and crust movement.

Duration: 18 min
Activity

Virtual Earthquake Lab

Interactive simulation to understand how seismic waves travel through Earth's layers.

Difficulty: Advanced

Sign Up for Educator Resources

Get access to curriculum materials, lesson plans, and printable worksheets designed for teaching about Earth's structure.

  • Complete lesson plans for all grade levels
  • Printable worksheets and activities
  • Interactive presentation slides

You Might Also Like

Volcanoes and Earth's Interior

Explore the connection between volcanic activity and Earth's internal structure.

Learn more →

Earth's Magnetic Field

Learn how Earth's core generates the magnetic field that protects our planet.

Learn more →

Climate and Atmosphere

Discover how Earth's atmosphere influences our climate and weather patterns.

Learn more →

Get in Touch

Have questions about Earth's layers? Want to collaborate on educational projects? We'd love to hear from you!

Contact Information

Phone

+1 (555) 123-4567

Monday-Friday, 9AM-5PM

Email

info@earthjourney2025.edu

We'll respond within 24 hours

Location

123 Science Center Drive

Earth Learning Campus

San Francisco, CA 94103

Follow Us

Send Us a Message

Frequently Asked Questions