Earth facts for kids
Earth seen from a satellite
|Reference date J2000.0|
|Longest distance from the Sun||152,097,701 km
|Shortest distance from the Sun||147,098,074 km
|Longest distance from the center of its orbital path
|How long it takes to complete an orbit||365.256366 days
|Average speed||29.783 km/s
|Angle above the reference plane
to the invariable plane
|Size and other qualities|
|Average radius||6,371.0 km (3,958.8 mi)|
|Surface area||510,072,000 km²|
|Volume||1.08321 × 10¹² km³|
|Mass||5.9736 × 1024 kg|
|Average density||5.515 g/cm³|
|Surface gravity||0.99732 g|
|Escape velocity||11.186 km/s|
|Avg. surface temp.||14°C|
Earth is the third planet from the Sun and the only astronomical object known to harbor life. According to radiometric dating and other sources of evidence, Earth formed over 4.5 billion years ago. Earth's gravity interacts with other objects in space, especially the Sun and the Moon (which is Earth's only natural satellite). Earth revolves around the Sun in 365.26 days, a period known as an Earth year. During this time, Earth rotates around its axis about 366.26 times.
Earth's axis of rotation is tilted, producing seasons on Earth. The gravitational interaction between Earth and the Moon causes ocean tides, stabilizes Earth's orientation on its axis, and gradually slows its rotation. Earth is the densest planet in the Solar System and the largest of the four terrestrial planets. Earth is situated in the Milky Way and orbits about 28,000 light-years from its center.
Earth's lithosphere is divided into several rigid tectonic plates that migrate across the surface over periods of many millions of years. About 71% of Earth's surface is covered with water, mostly by oceans. Earth is the only planet in our solar system that has a large amount of liquid water. About 71% of the surface of Earth is covered by oceans. Because of this, people some times called it "blue planet".
The remaining 29% is land consisting of continents and islands that together have many lakes, rivers and other sources of water that contribute to the hydrosphere. The majority of Earth's polar regions are covered in ice, including the Antarctic ice sheet and the sea ice of the Arctic ice pack. Earth's interior remains active with a solid iron inner core, a liquid outer core that generates the Earth's magnetic field, and a convecting (currents carrying heat from the interior to the planet's surface) mantle that drives plate tectonics.
Within the first billion years of Earth's history, life appeared in the oceans and began to affect the Earth's atmosphere and surface, leading to the rapid increase of aerobic and anaerobic organisms, these are organisms that do not require oxygen for growth. Some geological evidence indicates that life may have arisen as much as 4.1 billion years ago.
Since then, the combination of Earth's distance from the Sun, physical properties, and geological history have allowed life to evolve and thrive. In the history of the Earth, biodiversity has gone through long periods of expansion, occasionally punctuated by mass extinction events. Over 99% of all species that ever lived on Earth are extinct. Estimates of the number of species on Earth today vary widely; most species have not been described. Over 7.6 billion humans live on Earth and depend on its biosphere and natural resources for their survival. Humans have developed diverse societies and cultures.
- Geological history
- Origin of life and evolution
- Physical characteristics
- Asteroids and artificial satellites
- Cultural and historical viewpoint
- Related pages
- Images for kids
Earth's atmosphere and oceans were formed by volcanic activity and outgassing. Water vapor from these sources condensed into the oceans, augmented by water and ice from asteroids, protoplanets, and comets. In this model, atmospheric "greenhouse gases" kept the oceans from freezing when the newly forming Sun had only 70% of its current luminosity. Earth's magnetic field was established, which helped prevent the atmosphere from being stripped away by the solar wind.
A crust formed when the molten outer layer of Earth cooled to form a solid. Continents formed by plate tectonics, a process ultimately driven by the continuous loss of heat from Earth's interior. Over the period of hundreds of millions of years, the supercontinents have assembled and broken apart. Roughly 750 million years ago, one of the earliest known supercontinents, Rodinia, began to break apart. The continents later recombined to form Pannotia, then finally Pangaea, which also broke apart.
Origin of life and evolution
Chemical reactions led to the first self-replicating molecules about four billion years ago. A half billion years later, the last common ancestor of all current life arose. The evolution of photosynthesis allowed the Sun's energy to be harvested directly by life forms. The resultant oxygen accumulated in the atmosphere and due to interaction with ultraviolet solar radiation, formed a protective ozone layer in the upper atmosphere.
Among the earliest fossil evidence for life are fossils found in Western Australia. The earliest direct evidence of life on Earth is contained in 3.45 billion-year-old Australian rocks showing fossils of micro-organisms.
During the Neoproterozoic, much of Earth might have been covered in ice. This has been termed "Snowball Earth", and it is of particular interest because it preceded the Cambrian explosion. Following the Cambrian explosion, there have been five mass extinctions. The most recent such event was when an asteroid impact triggered the extinction of the non-avian dinosaurs and other large reptiles, but spared some small animals such as mammals.
Mammalian life expanded rapidly and branched out, and several million years ago an African ape-like animal such as Orrorin tugenensis gained the ability to stand upright. This led to tool use and encouraged communication that provided the nutrition and stimulation needed for a larger brain, which led to the evolution of humans.
Earth's expected long-term future is tied to that of the Sun. Over the next 1.1 billion years, solar luminosity will increase by 10%, and over the next 3.5 billion years by 40%. The Earth's increasing surface temperature will accelerate the inorganic carbon cycle, reducing Carbon dioxide concentration to levels lethally low for plant photosynthesis in approximately 500–900 million years.
The lack of vegetation will result in the loss of oxygen in the atmosphere, making animal life impossible. After another billion years all surface water will have disappeared and the mean global temperature will reach 70 °C (158 °F).
The Sun will evolve to become a red giant in about 5 billion years. Models predict that the Sun will expand to roughly about 250 times its present radius. Most, if not all, remaining life will be destroyed by the Sun's increased luminosity (peaking at about 5,000 times its present level). A 2008 simulation indicates that Earth's orbit will eventually decay due to tidal effects and drag, causing it to enter the Sun's atmosphere and be vaporized.
Earth's mass is composed mostly of iron (32.1%), oxygen (30.1%), silicon (15.1%), magnesium (13.9%), sulfur (2.9%), nickel (1.8%), calcium (1.5%), and aluminium (1.4%), with the remaining 1.2% consisting of trace amounts of other elements. The core region is estimated to be primarily composed of iron (88.8%), with smaller amounts of nickel (5.8%), sulfur (4.5%), and less than 1% trace elements. Over 99% of the crust is composed of 11 oxides, principally silica, alumina, iron oxides, lime, magnesia, potash and soda.
Earth's interior, like that of the other terrestrial planets, is divided into layers by their chemical or physical properties. The outer layer is a silicate solid crust, which is underlain by a highly viscous (sticky consistency between solid and liquid) solid mantle. The thickness of the crust varies from about 6 kilometres (3.7 mi) under the oceans to 30–50 km (19–31 mi) for the continents. The crust and the cold, rigid, top of the upper mantle are collectively known as the lithosphere, and it is of the lithosphere that the tectonic plates are composed.
The structure of Earth changes from the inside to the outside. The center of earth (Earth's core) is mostly iron (88.8%), nickel (5.8%), sulfur (4.5%), and less than 1% other elements. The Earth's crust is largely oxygen (47%). Oxygen is normally a gas but it can join with other chemicals to make compounds like water and rocks, 99.22% of rocks have oxygen in them. The most common oxygen-having rocks are silica, alumina, rust (made with iron), lime (made with calcium), magnesia, potash (made with potassium), and sodium oxide, and others. The radius of the inner core is about one fifth of that of Earth.
Earth's rigid outer layer is divided into tectonic plates. These plates are rigid segments that move relative to each other at one of three boundaries types:
- convergent boundaries, two plates come together
- divergent boundaries, two plates are pulled apart
- transform boundaries, two plates slide past one another
Along these plate boundaries, earthquakes, volcanic activity, mountain-building, and oceanic trench formation can occur. The oldest oceanic crust is located in the Western Pacific and is estimated to be 200 million years old. By comparison, the oldest dated continental crust is 4030 million years old.
The total surface area of Earth is about 510 million km2 (197 million sq mi). Of this, 70.8%, or 361.13 million km2 (139.43 million sq mi), is below sea level and covered by ocean water. Below the ocean's surface the continental shelf, mountains, volcanoes, oceanic trenches, submarine canyons, oceanic plateaus, abyssal plains, and a globe-spanning mid-ocean ridge system.
The remaining 29.2%, or 148.94 million km2 (57.51 million sq mi), not covered by water has terrain that varies greatly from place to place and consists of mountains, deserts, plains, plateaus, and other landforms.
Tectonics and erosion, volcanic eruptions, flooding, weathering, glaciation, the growth of coral reefs, and meteorite impacts are among the processes that constantly reshape the Earth's surface over geological time.
The elevation of the land surface varies from the low point of −418 m (−1,371 ft) at the Dead Sea, to a maximum altitude of 8,848 m (29,029 ft) at the top of Mount Everest.
The abundance of water on Earth's surface is a unique feature that distinguishes the "Blue Planet" from other planets in the Solar System. Earth's hydrosphere consists chiefly of the oceans, but technically includes all water surfaces in the world, including inland seas, lakes, rivers, and underground waters. The deepest underwater location is Challenger Deep of the Mariana Trench in the Pacific Ocean with a depth of 10,911.4 m (35,799 ft).
About 97.5% of the water is saline; the remaining 2.5% is fresh water. Most fresh water, about 68.7%, is present as ice in ice caps and glaciers. The oceans are also a reservoir of dissolved atmospheric gases, which are essential for the survival of many aquatic life forms. Sea water has an important influence on the world's climate, with the oceans acting as a large heat reservoir. Shifts in the oceanic temperature distribution can cause major weather changes, such as the El Niño–Southern Oscillation.
The air animals and plants use to live is only the first level of the air around the Earth (the troposphere). The day to day changes in this level of air are named weather; the changes between places far away from each other and from year to year are named the climate. Rain and storms are both in this level. Above this first level, there are four other levels.
The air gets colder as it goes up in the first level; in the second level (the stratosphere), the air gets warmer as it goes up. This level has a special kind of oxygen called ozone. The ozone in this air keeps living things safe from damaging rays from the Sun. Some gasses – especially methane and carbon dioxide – work like a blanket to keep things warm.
The middle level (the mesosphere) gets colder and colder with height; the fourth level (the thermosphere) gets warmer and warmer; and the last level (the exosphere) is almost outer space and has very little air at all. The three outer levels have a lot of electric power moving through them; this is called the ionosphere and is important for radio and other electric waves in the air. It is also where the Northern Lights are.
A planet that can sustain life is termed habitable, even if life did not originate there. Earth provides liquid water—an environment where complex organic molecules can assemble and interact, and sufficient energy to sustain metabolism. The distance of Earth from the Sun, as well as its orbit, rate of rotation, axial tilt, geological history, sustaining atmosphere, and magnetic field all contribute to the current climatic conditions at the surface.
Natural resources and land use
Large deposits of fossil fuels are obtained from Earth's crust, consisting of coal, petroleum, and natural gas. These deposits are used by humans both for energy production and for chemical production. Mineral ore bodies have also been formed within the crust, these bodies form concentrated sources for many metals and other useful elements.
Earth's biosphere produces many useful biological products for humans, including food, wood, pharmaceuticals, oxygen, and the recycling of many organic wastes. The land-based ecosystem depends upon topsoil and fresh water, and the oceanic ecosystem depends upon dissolved nutrients washed down from the land.
Natural and environmental hazards
Large areas of Earth's surface are subject to extreme weather such as tropical cyclones, hurricanes, or typhoons that dominate life in those areas. Many places are subject to earthquakes, landslides, tsunamis, volcanic eruptions, tornadoes, sinkholes, blizzards, floods, droughts, wildfires, and other calamities and disasters.
Many localized areas are subject to human-made pollution of the air and water, acid rain and toxic substances, loss of vegetation (overgrazing, deforestation, desertification), loss of wildlife, species extinction, soil degradation, soil depletion and erosion.
There is a scientific agreement linking human activities to global warming due to industrial carbon dioxide emissions. This is predicted to produce changes such as the melting of glaciers and ice sheets, more extreme temperature ranges, significant changes in weather and a global rise in average sea levels.
Asteroids and artificial satellites
Earth has at least five co-orbital asteroids. The tiny near-Earth asteroid 2006 RH120 makes close approaches to the Earth–Moon system roughly every twenty years. During these approaches, it can orbit Earth for brief periods of time.
As of April 2018[update], there are 1,886 operational, human-made satellites orbiting Earth. There are also inoperative satellites, including Vanguard 1, the oldest satellite currently in orbit, and over 16,000 pieces of tracked space debris. Earth's largest artificial satellite is the International Space Station.
Cultural and historical viewpoint
Human cultures have developed many views of the planet. Earth is sometimes personified as a deity. Scientific investigation has resulted in several shifts in people's view of the planet. Initial belief in a flat Earth was gradually changed in the Greek colonies of southern Italy during the late 6th century BC. By the end of the 5th century BC, the sphericity of Earth was universally accepted among Greek intellectuals.
Earth was generally believed to be the center of the universe until the 16th century. Westerners before the 19th century generally believed Earth to be only a few thousand years old at most. It was only during the 19th century that geologists realized Earth's age was at least many millions of years, when radioactivity and radioactive dating were discovered. The perception of Earth shifted again in the 20th century when humans first viewed it from orbit, and especially with photographs of Earth returned by the Apollo program.
Images for kids
This view from orbit shows the full moon partially obscured by Earth's atmosphere
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