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	Earth At a Glance
	Name From Old English Average Distance from Sun 92,955,820 miles 149,597,890 km 1 Astronomical Unit Mass 1 Earth mass 5,973,700 x 1021 kg Equatorial Diameter 7,926 miles 12,756 km Length of Day 24 hours Length of Year 365.24 Earth days Known Moons 1 Compare Planets

We know our world as an abode for life. Earth is teeming with fish, mammals, birds, reptiles, insects, and even some oddball "extremophiles" -- life forms that live in extreme environments like deep inside ice at the poles or around hot springs at the bottom of the ocean. Today, the diversity of life on Earth, and its hardiness at adapting to extreme environments, prompt many scientists to think life could thrive elsewhere in our solar system, or on planets and moons around other stars in our Milky Way galaxy.

Warm water glows bright red in this infrared image from Earth orbit. The warm water is part of an El Niño event, which alters weather patterns in North America.

We know that Earth is the largest of the "terrestrial" planets in our solar system -- the four rocky planets close to the Sun.

Earth is tilted on its axis at 23.5 degrees, which creates the seasons. When one hemisphere is tilted toward the Sun, it experiences summer. The hemisphere tilted away experiences winter. Spring and fall occur when a hemisphere is between these two extremes.

Earth is the only planet where the normal temperature range allows water to exist on its surface as a liquid. In fact, oceans cover 70 percent of Earth's surface.

This is an extremely important factor for life as we know it.

Earth's atmosphere is another factor that makes life possible. Consisting of 78 percent nitrogen, 21 percent oxygen, and traces of other gases, it provides protection from most of the Sun's harmful radiation. It also protects us from most of the meteors that head for the planet; they burn up in the atmosphere before they can hit the ground.

The solid portions of Earth form three layers. The top layer is the crust, and is made of silicates -- rocks like quartz, feldspar, and others. The mantle lies beneath the crust, and contains most of Earth's mass. The mantle is made primarily of silicon, magnesium, and oxygen. The mantle wraps around a two-layered core: a partially molten outer layer of iron and nickel and an inner layer of solid iron. As Earth rotates, these layers spin at different rates, which generates our planet's magnetic field.

Earth's seven continents sit on large tectonic plates that float atop the mantle. Eons ago, the continents were joined together into a single land mass scientists have coined Pangaea. Starting about 200 million years ago, the plates began to drift apart, causing the continents to separate. They are still moving today, albeit extremely slowly. Earthquakes occur where tectonic plates run into each other and one plate is forced to slide underneath another.

Moon At a Glance
Average Distance from Earth 238,855 miles 384,400 km Equatorial Diameter 2,159 miles 3,475 km Length of Day 27.3 Earth days Surface Gravity 17 percent that of Earth Compare Moons

Earth's Moon
Earth's partner in its yearly trek around the Sun, the Moon, is geologically dead. Dried lava fields called "maria" -- Latin for seas -- cover its surface, along with impact craters. The maria formed about four billion years ago, when giant asteroids punched holes in the Moon's crust, allowing molten rock to bubble to the surface, where it cooled and hardened.

The mountains of Taurus-Littrow dwarf the Apollo 17 Moon lander, Challenger (at center).

The interaction has other important consequences. Over time, the Moon's rotation has become tidally locked, so that the same side of the Moon always faces Earth. And the Moon acts to stabilize a "wobble" in Earth's axis. Over billions of years, this has led to a much more stable climate, which was friendly to the evolution of life. The Earth-Moon interaction also slows Earth's rotation by about two milliseconds per day per century.

The Moon probably formed in a "big whack."

The theory arose after scientists analyzed the rocks brought to Earth by Apollo astronauts and Soviet Luna probes, as well as the readings of seismometers left on the lunar surface to record "moonquakes."

Their studies showed that the Moon's composition closely resembles that of Earth's crust and mantle. From this, scientists concluded that a Mars-sized body hit Earth within a few million years of its formation. The impact vaporized much of the material in Earth's crust and mantle and blasted them into space, forming a ring around the planet. This material quickly coalesced to form the Moon -- Earth's steady companion in its never-ending trek around the Sun.

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This document was last modified: September 13, 2008