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Earth's mechanically rigid outer layer, the lithosphere, is divided into tectonic plates. These plates are rigid segments that move relative to each other at one of three boundaries types: At convergent boundariestwo plates come together; at divergent boundariestwo plates are pulled apart; and at transform boundariestwo plates slide past one another laterally. Along these plate boundaries, earthquakesvolcanic activitymountain-buildingand oceanic trench formation can occur. As the tectonic plates migrate, oceanic crust is subducted under the leading edges of the plates at convergent boundaries.

At the same time, the upwelling of mantle material at divergent boundaries creates mid-ocean ridges. The combination of these processes recycles the oceanic crust back into the mantle.

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The remaining Tectonics and erosionvolcanic eruptionsfloodingweatheringglaciationthe growth of coral reefsand meteorite impacts are among the processes that constantly reshape Earth's surface over geological time. The continental crust consists of lower density material such as the igneous rocks granite and andesite.

Less common is basalta denser volcanic rock that is the primary constituent of the ocean floors. The most abundant silicate minerals on Earth's surface include quartzfeldsparsamphibolemicapyroxene and olivine. The pedosphere is the outermost layer of Earth's continental surface and is composed of soil and subject to soil formation processes.

The total arable land is The abundance of water on Earth's surface is a unique feature that distinguishes the "Blue Planet" from other planets in the Solar System. The mass of the oceans is approximately 1. The oceans cover an area of About Most fresh water, about The atmospheric pressure at Earth's sea level averages Earth's biosphere has significantly altered its atmosphere. Oxygenic photosynthesis evolved 2. The ozone layer blocks ultraviolet solar radiationpermitting life on land.

Water vapor, carbon dioxide, methanenitrous oxideand ozone are the primary greenhouse gases in the atmosphere. Earth's atmosphere has no definite boundary, slowly becoming thinner and fading into outer space.

This lowest layer is called the troposphere. Energy from the Sun heats this layer, and the surface below, causing expansion of the air. This lower-density air then rises and is replaced by cooler, higher-density air. The result is atmospheric circulation that drives the weather and climate through redistribution of thermal energy. Water vapor generated through surface evaporation is transported by circulatory patterns in the atmosphere.

When atmospheric conditions permit an uplift of warm, humid air, this water condenses and falls to the surface as precipitation. This water cycle is a vital mechanism for supporting life on land and is a primary factor in the erosion of surface features over geological periods.

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Precipitation patterns vary widely, ranging from several meters of water per year to less than a millimeter. Atmospheric circulation, topographic features, and temperature differences determine the average precipitation that falls in each region. The amount of solar energy reaching Earth's surface decreases with increasing latitude.

At higher latitudes, the sunlight reaches the surface at lower angles, and it must pass through thicker columns of the atmosphere. As a result, the mean annual air temperature at sea level decreases by about 0. Ranging from the equator to the polar regions, these are the tropical or equatorialsubtropicaltemperate and polar climates. The highest air temperature ever measured on Earth was Above the troposphere, the atmosphere is usually divided into the stratospheremesosphereand thermosphere.

Beyond these, the exosphere thins out into the magnetospherewhere the geomagnetic fields interact with the solar wind. Thermal energy causes some of the molecules at the outer edge of the atmosphere to increase their velocity to the point where they can escape from Earth's gravity.

This causes a slow but steady loss of the atmosphere into space. Because unfixed hydrogen has a low molecular massit can achieve escape velocity more readily, and it leaks into outer space at a greater rate than other gases. Photosynthesis provided a source of free oxygen, but the loss of reducing agents such as hydrogen is thought to have been a necessary precondition for the widespread accumulation of oxygen in the atmosphere.

Instead, most of the hydrogen loss comes from the destruction of methane in the upper atmosphere. The gravity of Earth is the acceleration that is imparted to objects due to the distribution of mass within Earth.

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Near Earth's surface, gravitational acceleration is approximately 9. Local differences in topographygeologyand deeper tectonic structure cause local and broad, regional differences in Earth's gravitational field, known as gravity anomalies.

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The main part of Earth's magnetic field is generated in the core, the site of a dynamo process that converts the kinetic energy of thermally and compositionally driven convection into electrical and magnetic field energy.

The field extends outwards from the core, through the mantle, and up to Earth's surface, where it is, approximately, a dipole. The poles of the dipole are located close to Earth's geographic poles. At the equator of the magnetic field, the magnetic-field strength at the surface is 3.

This causes secular variation of the main field and field reversals at irregular intervals averaging a few times every million years.

The most recent reversal occurred approximatelyyears ago. The extent of Earth's magnetic field in space defines the magnetosphere. Ions and electrons of the solar wind are deflected by the magnetosphere; solar wind pressure compresses the dayside of the magnetosphere, to about 10 Earth radii, and extends the nightside magnetosphere into a long tail. During magnetic storms and substormscharged particles can be deflected from the outer magnetosphere and especially the magnetotail, directed along field lines into Earth's ionosphere, where atmospheric atoms can be excited and ionized, causing the aurora.

Earth's rotation period relative to the Sun-its mean solar day-is 86, seconds of mean solar time 86, For bodies near the celestial equatorthis is equivalent to an apparent diameter of the Sun or the Moon every two minutes; from Earth's surface, the apparent sizes of the Sun and the Moon are approximately the same.

The orbital speed of Earth averages about The Moon and Earth orbit a common barycenter every When combined with the Earth-Moon system's common orbit around the Sun, the period of the synodic monthfrom new moon to new moon, is Viewed from the celestial north polethe motion of Earth, the Moon, and their axial rotations are all counterclockwise. Viewed from a vantage point above the north poles of both the Sun and Earth, Earth orbits in a counterclockwise direction about the Sun.

The orbital and axial planes are not precisely aligned: Earth's axis is tilted some Without this tilt, there would be an eclipse every two weeks, alternating between lunar eclipses and solar eclipses. The Hill sphereor the sphere of gravitational influence, of Earth is about 1.

Objects must orbit Earth within this radius, or they can become unbound by the gravitational perturbation of the Sun. The axial tilt of Earth is approximately Due to Earth's axial tilt, the amount of sunlight reaching any given point on the surface varies over the course of the year. This causes the seasonal change in climate, with summer in the Northern Hemisphere occurring when the Tropic of Cancer is facing the Sun, and winter taking place when the Tropic of Capricorn in the Southern Hemisphere faces the Sun.

During the summer, the day lasts longer, and the Sun climbs higher in the sky. In winter, the climate becomes cooler and the days shorter. In northern temperate latitudes, the Sun rises north of true east during the summer solstice, and sets north of true west, reversing in the winter.

The Sun rises south of true east in the summer for the southern temperate zone and sets south of true west. Above the Arctic Circlean extreme case is reached where there is no daylight at all for part of the year, up to six months at the North Pole itself, a polar night. In the Southern Hemisphere, the situation is exactly reversed, with the South Pole oriented opposite the direction of the North Pole. Six months later, this pole will experience a midnight suna day of 24 hours, again reversing with the South Pole.

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By astronomical convention, the four seasons can be determined by the solstices -the points in the orbit of maximum axial tilt toward or away from the Sun-and the equinoxeswhen Earth's rotational axis is aligned with its orbital axis.

In the Northern Hemisphere, winter solstice currently occurs around 21 December; summer solstice is near 21 June, spring equinox is around 20 March and autumnal equinox is about 22 or 23 September. In the Southern Hemisphere, the situation is reversed, with the summer and winter solstices exchanged and the spring and autumnal equinox dates swapped.

The angle of Earth's axial tilt is relatively stable over long periods of time. Its axial tilt does undergo nutation ; a slight, irregular motion with a main period of Both of these motions are caused by the varying attraction of the Sun and the Moon on Earth's equatorial bulge.

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The poles also migrate a few meters across Earth's surface. This polar motion has multiple, cyclical components, which collectively are termed quasiperiodic motion. In addition to an annual component to this motion, there is a month cycle called the Chandler wobble. Earth's rotational velocity also varies in a phenomenon known as length-of-day variation. In modern times, Earth's perihelion occurs around 3 January, and its aphelion around 4 July. These dates change over time due to precession and other orbital factors, which follow cyclical patterns known as Milankovitch cycles.

The changing Earth-Sun distance causes an increase of about 6. Because the Southern Hemisphere is tilted toward the Sun at about the same time that Earth reaches the closest approach to the Sun, the Southern Hemisphere receives slightly more energy from the Sun than does the northern over the course of a year.

This effect is much less significant than the total energy change due to the axial tilt, and most of the excess energy is absorbed by the higher proportion of water in the Southern Hemisphere. A study from suggested that Planet Nine tilted all the planets of the Solar Systemincluding Earth, by about six degrees.

A planet that can sustain life is termed habitableeven 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.

A planet's life forms inhabit ecosystemswhose total is sometimes said to form a "biosphere". Terrestrial biomes lying within the Arctic or Antarctic Circlesat high altitudes or in extremely arid areas are relatively barren of plant and animal life; species diversity reaches a peak in humid lowlands at equatorial latitudes.

In Julyscientists reported identifying a set of genes from the last universal common ancestor LUCA of all organisms living on Earth. Earth has resources that have been exploited by humans. Large deposits of fossil fuels are obtained from Earth's crust, consisting of coalpetroleumand natural gas.

Earth's biosphere produces many useful biological products for humans, including food, woo pharmaceuticalsoxygen, 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.

Large areas of Earth's surface are subject to extreme weather such as tropical cycloneshurricanesor typhoons that dominate life in those areas. From tothese events caused an average of 11, human deaths per year. Many localized areas are subject to human-made pollution of the air and water, acid rain and toxic substances, loss of vegetation overgrazingdeforestationdesertificationloss of wildlife, species extinctionsoil degradationsoil depletion and erosion. There is a scientific consensus 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. Cartographythe study and practice of map-making, and geographythe study of the lands, features, inhabitants and phenomena on Earth, have historically been the disciplines devoted to depicting Earth.

Surveyingthe determination of locations and distances, and to a lesser extent navigationthe determination of position and direction, have developed alongside cartography and geography, providing and suitably quantifying the requisite information. Earth's human population reached approximately seven billion on 31 October Human population density varies widely around the world, but a majority live in Asia.

The northernmost permanent settlement in the world is Alerton Ellesmere Island in NunavutCanada. States claim the planet's entire land surface, except for parts of Antarctica and a few other unclaimed areas.

Earth has never had a planetwide government, but the United Nations is the leading worldwide intergovernmental organization.

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The first human to orbit Earth was Yuri Gagarin on 12 April The station's crewmade up of six people, is usually replaced every six months. The Moon is a relatively large, terrestrialplanet-like natural satellitewith a diameter about one-quarter of Earth's. It is the largest moon in the Solar System relative to the size of its planet, although Charon is larger relative to the dwarf planet Pluto.

The natural satellites of other planets are also referred to as "moons", after Earth's. The gravitational attraction between Earth and the Moon causes tides on Earth. The same effect on the Moon has led to its tidal locking : its rotation period is the same as the time it takes to orbit Earth. As a result, it always presents the same face to the planet. As the Moon orbits Earth, different parts of its face are illuminated by the Sun, leading to the lunar phases ; the dark part of the face is separated from the light part by the solar terminator.

The Moon may have dramatically affected the development of life by moderating the planet's climate. Paleontological evidence and computer simulations show that Earth's axial tilt is stabilized by tidal interactions with the Moon.

Viewed from Earth, the Moon is just far enough away to have almost the same apparent-sized disk as the Sun. The angular size or solid angle of these two bodies match because, although the Sun's diameter is about times as large as the Moon's, it is also times more distant.

The most widely accepted theory of the Moon's origin, the giant-impact hypothesisstates that it formed from the collision of a Mars-size protoplanet called Theia with the early Earth. This hypothesis explains among other things the Moon's relative lack of iron and volatile elements and the fact that its composition is nearly identical to that of Earth's crust.

Earth has at least five co-orbital asteroidsincluding Cruithne and AA The tiny near-Earth asteroid RH makes close approaches to the Earth-Moon system roughly every twenty years. During these approaches, it can orbit Earth for brief periods of time.

The standard astronomical symbol of Earth consists of a cross circumscribed by a circle, representing the four corners of the world. Human cultures have developed many views of the planet.

In many cultures it is a mother goddess that is also the primary fertility deityand by the midth century, the Gaia Principle compared Earth's environments and life as a single self-regulating organism leading to broad stabilization of the conditions of habitability. Scientific investigation has resulted in several culturally transformative shifts in people's view of the planet. Initial belief in a flat Earth was gradually displaced in the Greek colonies of southern Italy during the late 6th century BC by the idea of spherical Earthwhich was attributed to both the philosophers Pythagoras and Parmenides.

It was only during the 19th century that geologists realized Earth's age was at least many millions of years. From Wikipedia, the free encyclopedia.

This article is about the planet. For its human cts, see the World. For other uses, see Earth disambiguation and Planet Earth disambiguation. Third planet from the Sun in the Solar System.

The Blue Marblethe first full-view photograph of the planet, was taken by Apollo 17 astronauts en route to the Moon in Alternative names. Semi-major axis.

Orbital period. Average orbital speed. Mean anomaly. Equatorial radius. Polar radius. Surface area. Mean density. Surface gravity. Moment of inertia factor. Escape velocity.

Sidereal rotation period. Axial tilt. Surface pressure. Main article: History of Earth. Main article: Geological history of Earth.

Life timeline. This box: view talk edit. Single-celled life. Multicellular life. Earliest water. Earliest life. Earliest oxygen. Atmospheric oxygen.

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Oxygen crisis. Sexual reproduction.

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Earliest plants. Earliest animals. Ediacara biota. Cambrian explosion. Earliest apes. See also: Human timelineand Nature timeline. Main articles: Abiogenesis and Evolutionary history of life.

Main article: Future of Earth. See also: Global catastrophic risk. Main articles: Figure of the EarthEarth radiusand Earth's circumference.

See also: Abundance of elements on Earth. Main article: Structure of the Earth. Main article: Earth's internal heat budget. Pacific Plate.

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African Plate [n 17]. North American Plate. Eurasian Plate. Antarctic Plate. Indo-Australian Plate. South American Plate. Main article: Plate tectonics. Main article: Hydrosphere. Main article: Atmosphere of Earth. Main articles: Weather and Climate. Hurricane Felix seen from low Earth orbit, September Lenticular cloud over an ice pressure ridge near Mount DiscoveryAntarcticaNovember Massive clouds above the Mojave DesertFebruary Main article: Gravity of Earth.

Main article: Earth's magnetic field. Main article: Magnetosphere. Main article: Earth's rotation.

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Main article: Earth's orbit. Main article: Biosphere. Main articles: Natural resource and Land use.

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Main articles: Human geography and World. Main article: Moon. Main article: Earth in culture. Gould Belt. Orion Arm. Virgo SCl. Laniakea SCl. Observable Universe. Celestial sphere Earth phase Earth physical characteristics tables Earth science Earth system science List of gravitationally rounded objects of the Solar System Outline of Earth Timeline of natural history Timeline of the far future. The quantities given are the values at the instant J The difference between Earth's perihelion and aphelion is 5 million kilometers.

February Orbital Debris Quarterly News. Retrieved 18 April Based on data from the Vector Map and Global Landcover Archived 26 March at the Wayback Machine datasets, extreme values for coverage of lakes and streams are 0. The ice shields of Antarctica and Greenland are counted as land, even though much of the rock that supports them lies below sea level. Over a year, this discrepancy adds up to a full sidereal day. Why should it use up the soil?

See: Chorowicz, Jean October Journal of African Earth Sciences.

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Bibcode : JAfES. See the Challenger Deep article for more details. Astronomy and Astrophysics. Due to the inverse square law, the radiation at perihelion is about Retrieved 23 September Retrieved 26 July Allen's Astrophysical Quantities.

Retrieved 13 March Union of Concerned Scientists. Retrieved 27 September David R. Lide ed. Handbook of Chemistry and Physics 81st ed. The Astronomical Almanac. Archived from the original on 26 August Retrieved 25 February Available online from National Geospatial-Intelligence Agency.

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In Ahrens, Thomas J ed. Bibcode : geph. Archived from the original on 16 October Retrieved 3 August In McCarthy, Dennis D. Retrieved 29 April Archived from the original on 24 April Table 8o-1 ".

University of British Columbia, Okanagan. Retrieved 26 November The World Factbook. Central Intelligence Agency. Retrieved 5 August August Celestial Mechanics and Dynamical Astronomy. Bibcode : CeMDA. The Astronomical Journal.

Bibcode : AJ Retrieved 17 August Cox, ed. Allen's Astrophysical Quantities 4th ed. Arizona State University. Archived from the original on 16 June Retrieved 7 August Retrieved 22 April Archived from the original on 4 January Earth System Research Laboratory.

National Oceanic and Atmospheric Administration. Archived from the original on 26 July Archived from the original on 1 September Retrieved 27 April Chad Matlick in " Beowulf : Lines to ".

The oldest dated rocks on Earth are of several different types. 1. There are early rocks recovered from the Moon. This is relevant because the Moon was once part of the Earth: see giant impact hypothesis. During Apollo 16, Lunar sample , dated at billion years, was brought back. Dating On Earth Asian Wiki is owned by Michael J. Kalous, MA, LCPC. The main focus of his practice is: Specializing in Relationships, Family, Faith, and Self-Development. Home. Dating On The Earth Wiki, icrushes dating site, rencontre femme dans le 52, dating roseburg oregon.

West Virginia University. Hosted at Bible Gateway. Reprinted by S. Humphrey Milford London Hosted at the Dept. Codex Junius 11I. Hosted at Project Gutenberg. Hosted at Old English at the University of Virginia, Retrieved 6 August Angela Hall as Dictionary of Northern Mythologyp. Brewer Oxford University Press Oxfor Oxford English Dictionary 3rd ed.

Oxford University Press. September Subscription or UK public library membership required. Bibcode : Sci The Age of the Earth. California: Stanford University Press. Newman, William L.

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Retrieved 20 September Dalrymple, G. Brent Geological Society, London, Special Publications. Bibcode : Natur. Archived from the original on 9 January Retrieved 30 January An impact origin of the Earth-Moon system. American Geophysical Union, Fall Meeting Abstract U51A Lunar and Planetary Institute.

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Universities Space Research Association. Retrieved 27 June Guinan ed. San Francisco: Astronomical Society of the Pacific. Bibcode : ASPC. Retrieved 27 March Continents and Supercontinents.

Oxford University Press US. June Bibcode : Tectp. Reviews of Geophysics. Bibcode : RvGSP December Journal of Asian Earth Sciences. Bibcode : JAESc. Australian Journal of Earth Sciences. Bibcode : AuJES. American Scientist. Could another one start? American Museum of Natural History. Retrieved 28 June Page Paleontology Science Center. Archived from the original on 4 March Retrieved 2 March Ford; Worm, Boris February Scientific American.

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