Our blue planet pictured by the U.S. Suomi NPP weather satellite © NASA

Earth

Earth is the only planet in the solar system with water in its three forms—liquid, solid and gaseous—and in large amounts. And the only planet we know of to sustain life. But what exactly is this large rock like no other in the universe like?

Chiffres clés

Distance from Sun149,597,870 km
Volume1.083 21 × 1012 km3
Mass6 X 1024 kg
Diameter12,756 km
GravityEarth’s gravity (g), measured at 9.81 m/s2, is the reference value when comparing
the gravity of planets
Axial tilt23.4°
Revolution period365.25 days
Rotation period23 hours, 56 minutes and 4 seconds
Temperature15°C on average at surface (but trending upwards due to global warming)
Moons1

A very large, very hard peach

Earth is one of the four rocky—or telluric—planets with MercuryVenus and Mars. It’s the largest of the four, with a diameter of 12,700 kilometres. The Earth’s structure is like a peach, with a core (stone) in the middle, surrounded by a thick layer called the mantle (flesh), itself covered by a thin crust (skin).

  • Core

The core is composed of a solid inner core of iron and nickel at a temperature of 6,000°C and an outer core of 89% liquid iron at around 3,500°C. This outer core works like a gigantic bicycle dynamo in which the motions of the electrically conductive liquid iron generate electrical energy, giving rise to a magnetic field.

  • Mantle

The mantle is a viscous mixture of molten rock where slow creep processes carry heat from the core to the surface. Like water boiling in a saucepan, the hot currents inside the mantle are transported outwards, then cool before sinking back down through the planet’s interior. It’s this convection mechanism that drives the movement of tectonic plates at the surface.

  • Crust

The crust may be oceanic, consisting of volcanic rocks and with an average thickness of six kilometres, or continental, composed of granite and 25 to 70 kilometres thick. Earth’s surface offers a range of landscapes, with volcanoes, mountains, deserts, oceans and more besides. As it has evolved, numerous and violent bombardments by meteorites, combined with erosion and tectonic plate motions have changed how it looks. And it’s still changing today, as the plates continue to move, oceans erode coastlines and certain regions dry.

Structure interne de la Terre.
Earth's internal structure © CNES

Blue planet

Earth is covered 71% by water, in the form of lakes, rivers, oceans, glaciers, ice caps and atmospheric water vapour. Water is everywhere, in its liquid, solid and gaseous states, making our planet unique in the solar system.

  • A shielding atmosphere

Earth has an atmosphere consisting of gas shrouding the planet and held by gravity. It’s composed mainly of nitrogen (N2 78%) and oxygen (O2 21%). This atmosphere lets through some of the Sun’s rays, which heat the surface, and most of this heat is trapped by a greenhouse effect that sustains temperatures conducive to life. It also shields our planet from harmful solar radiation and meteorites.

YouTube Link to YouTube page

Earth and Moon: paired for life

Earth and its only natural satellite, the Moon, are inseparable. Without the Moon, our blue planet would be very different. For example, the Moon has gradually slowed Earth’s rotation, giving us our 24-hour days. Our satellite also stabilizes the planet’s rotational axis at a tilt of 23.4° with respect to its orbital plane, which is why we have seasons.

Lever de Terre depuis la Lune, photo prise depuis le module de commande d’Apollo 11.
Earth rise seen on the surface of the Moon, photographed from the Apollo 11 command module © NASA/Michael Collins

Earth laid bare

Scientists working across a wide range of disciplines are studying Earth’s size, mass, figure and internal structure from its surface, as well as from data acquired by space-based instruments.

  • Studied from all angles

Earth is part of a system in which everything—land, oceans, lakes and rivers, snow and ice, the atmosphere and living organisms—is interlinked and works together. All of these elements are being studied specifically and from a global perspective. To achieve this, scientists notably use Earth-observation data acquired from space.

From space, satellites are also studying the shape and internal structure of Earth.

  • Round… well, almost

Regardless of what those who still like to believe Earth is flat may say, as far back as Antiquity, scholars such as Aristotle were already advancing the idea that the Earth is a sphere. He reached this conclusion simply by watching an eclipse of the Moon: he saw that when our satellite passes in the shadow of Earth, our planet’s outline is clearly circular.

L’ombre de la Terre sur la Lune, lors d’une éclipse lunaire, permet d’observer la rotondité de la planète.
Earth’s shadow cast on the Moon during a lunar eclipse confirms that our planet is round © NASA, Robert Markowitz

And yet… our planet isn’t quite round, as it in fact flattens at the poles. This shape of the Earth, known as the “geoid”, is due to the planet’s rotation, which generates a centrifugal force—what you experience when exiting a revolving door. This shape—or “figure”—of the Earth has been confirmed by satellites, which have even shown just how lumpy it is.

Représentation très précise du géoïde terrestre (surface où la gravité est la même) obtenue grâce au satellite GOCE. Les parties rouges/jaunes correspondent aux écarts en altitude de + 100 m par rapport au Géoïde, les bleues de – 100 m.
Highly precise representation of Earth’s geoid—the surface shaped only by gravity—obtained thanks to the GOCE satellite. The red/yellow zones correspond to deviations in elevation of +100 metres with respect to the geoid, and blue zones to deviations © ESA/HPF/DLR

Solid Earth

Certain fields of science are investigating what we call the “solid Earth”—covering volcanology, seismology, geodesy and magnetism—using data from satellites and ground sensors and instruments now available in ever-increasing volumes. To make these data more readily usable for scientists, CNES created the ForM@Ter data centre in 2014, in partnership with numerous other scientific bodies.

  • Magnetism under close watch

Earth’s magnetic field, which protects it from harmful solar particles, is also closely studied. We know this field is generated by convection movements inside the planet’s core. The crust, oceans and the upper atmosphere also play their part. Launched in 2013, the European Space Agency’s (ESA) SWARM mission, composed of four satellites, precisely measures the intensity and direction of the magnetic fields generated by these components of our planet.

Le champ magnétique protège la Terre du vent solaire.
Earth’s magnetic field shields it from the solar wind © ESA/ATG medialab

Fun fact

Another word you might hear when referring to the Earth is the lithosphere: this is the rigid outermost shell composed of the crust and upper mantle.

Quiz

The Earth-Sun distance has become a benchmark for astronomers. It’s known as an astronomical unit (AU): Earth orbits at a distance of 1 AU from the Sun, whereas Neptune is 30 AU from our star. But how many kilometres is 1 AU?