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Earth

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Earth is the third planet from the Sun and the only known astronomical object that harbors life. This unique status is largely due to Earth being an ocean world. It is the only planet in our Solar System that sustains liquid surface water. The global ocean covers 70.8% of Earth's crust, leaving only 29.2% as land. Most of this land exists as continental landmasses within the land hemisphere.

Meteosat-12-fci-march-equinox-2025-noon
Meteosat-12-fci-march-equinox-2025-noon

Much of this land is humid and covered by vegetation. However, massive ice sheets in polar deserts actually hold more water than all groundwater, lakes, rivers, and atmospheric water combined.

Our planet functions through complex, interconnected physical mechanisms. The Earth's crust is divided into slowly moving tectonic plates. These plates interact with one another to produce mountain ranges, volcanoes, and earthquakes.

Deep beneath the surface, a liquid outer core generates a magnetosphere. This magnetic field acts as a shield, deflecting destructive solar winds and cosmic radiation.

Magnetosphere Levels-en
Magnetosphere Levels-en

Additionally, the atmosphere protects the surface from most meteoroids and ultraviolet light. This atmosphere is composed primarily of nitrogen and oxygen gases.

A vital process called the greenhouse effect helps maintain habitable temperatures. Water vapor and carbon dioxide (CO2) act as greenhouse gases in the atmosphere. These gases capture energy from the Sun's light to keep the planet warm. This process maintains a current average surface temperature of 14.76 °C (58.57 °F). At this temperature, water can remain in a liquid state under normal atmospheric pressure. Differences in solar energy absorption between the equator and the poles drive atmospheric and ocean currents. These currents create a global climate system that allows elements like carbon and nitrogen to cycle.

Earth's physical structure is an ellipsoid with a circumference of about 40,000 kilometers. It is the densest planet in the Solar System and the largest of the four rocky planets. Earth orbits the Sun at a distance of about one astronomical unit (1 AU). It takes approximately 365.25 days to complete one full revolution around the Sun. The planet also rotates on its own axis every 23 hours and 56 minutes. Because the axis of rotation is tilted, Earth experiences different seasons throughout the year.

Seasons1
Seasons1

Earth is also orbited by the Moon, a natural satellite roughly one-quarter the width of Earth.

Earth From the Perspective of Artemis II
Earth From the Perspective of Artemis II

The Moon orbits at 384,400 km and helps stabilize Earth's axis while causing tides.

The history of Earth began about 4.5 billion years ago. Like other bodies in the Solar System, Earth formed from gas and dust in a solar nebula. The Moon likely formed when a Mars-sized object named Theia collided with the early Earth. This glancing blow released material that eventually accreted into the Moon. Between 4.0 and 3.8 billion years ago, the Late Heavy Bombardment brought many asteroid impacts to Earth.

Solar system
Solar system

During the first billion years, oceans formed through volcanic outgassing and impacts from comets. By 3.5 billion years ago, the magnetic field was established to protect the atmosphere.

Over long periods, the movement of tectonic plates has reshaped the surface. These forces have caused continental crust to group into supercontinents and then break apart. For example, the supercontinent Rodinia began to break apart about 750 million years ago. Later, the supercontinent Pangaea formed and eventually began to break up around 180 million years ago.

Tectonic plates (empty)
Tectonic plates (empty)

Earth has also experienced cycles of glaciation. The Last Glacial Period, or the last ice age, ended roughly 11,700 years ago. These geological and climatic shifts show how dynamic our planet truly is.

Humanity has a significant relationship with the Earth's biosphere. Humans emerged approximately 300,000 years ago in Africa and have since spread to every continent. We depend entirely on Earth's natural resources and biological systems for our survival. However, human activities are currently impacting the climate and the biosphere in unsustainable ways. These changes are causing widespread extinctions and threatening the livelihoods of many life forms.

Global land use for food production, OWID statistic
Global land use for food production, OWID statistic

Looking much further ahead, the Sun will eventually evolve into a red giant. This will change Earth's environment forever, demonstrating the deep connection between our planet and its star.

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🖼️ Images & Media (42)
File:Seasons1.svg
Seasons1.svg
File:Flag of the United Nations.svg
Flag of the United Nations.svg
File:Global Temperature And Forces With Fahrenheit.svg
Global Temperature And Forces With Fahrenheit.svg
File:Tectonic plates (empty).svg
Tectonic plates (empty).svg
File:Spaccato vulcano.svg
Spaccato vulcano.svg
File:Axial tilt vs tropical and polar circles.svg
Axial tilt vs tropical and polar circles.svg
File:Earth-cutaway-schematic-english.svg
Earth-cutaway-schematic-english.svg
File:Earth cutaway schematic-en.svg
Earth cutaway schematic-en.svg
File:Magnetosphere Levels-en.svg
Magnetosphere Levels-en.svg
File:Earth symbol (bold).svg
Earth symbol (bold).svg
File:Earth symbol (fixed width).svg
Earth symbol (fixed width).svg
File:Globus cruciger (bold).svg
Globus cruciger (bold).svg

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