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Earth

     



    Earth
    Planet
    Earth /ˈɜːrθ/ is the third planet from the Sun, the densest planet in the Solar System, the largest of the Solar System's four terrestrial planets, and the only astronomical object known to harbor life. 
    Distance from Sun: 149.6 million km
    Radius: 6,371 km
    Age: 4.543 billion years
    Mass: 5.972 × 10^24 kg
    Population: 7.125 billion (2013) World Bank
    Moon: Moon

    "The Blue Marble" photograph of Earth, taken by the Apollo 17 lunar mission. The Arabian peninsula, Africa and Madagascar lie in the upper half of the disc, whereas Antarctica is at the bottom.
    "The Blue Marble" photograph of Earth, taken during the Apollo 17 lunar mission in 1972
    Orbital characteristics
    Epoch J2000[n 1]
    Aphelion
    152,100,000 km (94,500,000 mi)
    (1.01673 AU) [n 2]
    Perihelion
    147,095,000 km (91,401,000 mi)
    (0.9832687 AU) [n 2]
    Semi-major axis
    149,598,023 km (92,955,902 mi)
    (1.000001018 AU) [1]
    Eccentricity 0.0167086[1]
    Orbital period
    365.256363004 d [2]
    (1.00001742096 yr)
    Average orbital speed
    29.78 km/s (18.50 mi/s)[3]
    (107,200 km/h (66,600 mph))
    Mean anomaly
    358.617 deg
    Inclination
    7.155 deg to Sun's equator;
    1.57869 deg[4] to invariable plane;
    0.00005 deg to J2000 ecliptic
    Longitude of ascending node
    −11.26064 deg[3] to J2000 ecliptic
    Argument of perihelion
    114.20783 deg[3]
    Satellites
    One natural satellite;
    1305 operational artificial satellites[5][n 3]
    Physical characteristics
    Mean radius
    6,371.0 km (3,958.8 mi)[6]
    Equatorial radius
    6,378.1 km (3,963.2 mi)[7][8]
    Polar radius
    6,356.8 km (3,949.9 mi)[9]
    Flattening 0.0033528[10]
    1/298.257222101 (ETRS89)
    Circumference
    40,075.017 km (24,901.461 mi) (equatorial) [8]
    40,007.86 km (24,859.73 mi) (meridional) [11][12]
    Surface area
    510,072,000 km2 (196,940,000 sq mi)[13][14][n 4]
     (148,940,000 km2 (57,510,000 sq mi) (29.2%) land
      361,132,000 km2 (139,434,000 sq mi) (70.8%) water)
    Volume 1.08321×1012 km3 (2.59876×1011 cu mi)[3]
    Mass 5.97237×1024 kg (1.31668×1025 lb)[15]
    (3.0×10−6 M☉)
    Mean density
    5.514 g/cm3 (0.1992 lb/cu in)[3]
    Surface gravity
    9.807 m/s2 (32.18 ft/s2)[16]
    (1 g)
    Moment of inertia factor
    0.3307[17]
    Escape velocity
    11.186 km/s (6.951 mi/s)[3]
    Sidereal rotation period
    0.99726968 d[18]
    (23h 56m 4.100s)
    Equatorial rotation velocity
    1,674.4 km/h (1,040.4 mph)[19]
    Axial tilt
    23.4392811°[2]
    Albedo
    0.367 geometric[3]
    0.306 Bond[3]
    Surface temp. min mean max
    Kelvin 184 K[20] 288 K[21] 330 K[22]
    Celsius −89.2 °C 15 °C 56.7 °C
    Fahrenheit −128.5 °F 59 °F 134 °F
    Atmosphere
    Surface pressure
    101.325 kPa (at MSL)
    Composition by volume
    78.08% nitrogen (N2)[3] (dry air)
    20.95% oxygen (O2)
    0.930% argon
    0.039% carbon dioxide[23]
    ~ 1% water vapor (climate-variable)

    Earth /ˈɜːrθ/ (also the world[n 5], in Greek: Γαῖα Gaia,[n 6] or in Latin: Terra[26]) is the third planet from the Sun, the densest planet in the Solar System, the largest of the Solar System's four terrestrial planets, and the onlyastronomical object known to harbor life.


    According to evidence from radiometric dating and other sources, Earth was formed about 4.54 billion years ago.[27][28][29] Earth gravitationally interacts with other objects in space, especially the Sun and the Moon. During one orbit around the Sun, Earth rotates about its own axis 366.26 times, creating 365.26 solar days or one sidereal year.[n 7] Earth's axis of rotation is tilted 23.4° away from the perpendicular of its orbital plane, producing seasonal variations on the planet's surface with a period of one tropical year (365.24 solar days).[30]The Moon is Earth's only permanent natural satellite. Its gravitational interaction with Earth causes oceantides, stabilizes the orientation of Earth's rotational axis, and gradually slows Earth's rotational rate.


    Earth's lithosphere is divided into several rigid tectonic plates that migrate across the surface over periods ofmany millions of years. 71% of Earth's surface is covered with water,[31] with the remainder consisting of continents and islands that together have many lakes and other sources of water that contribute to thehydrosphere. Earth's polar regions are mostly covered with 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 magnetic field, and a convecting mantle that drives plate tectonics.


    Within its first billion years,[32] life appeared in Earth's oceans and began to affect its atmosphere and surface, promoting the proliferation of aerobic as well as anaerobic organisms. Since then, the combination of Earth'sdistance from the Sun, its physical properties and its geological history have allowed life to thrive and evolve. The earliest undisputed life on Earth arose at least 3.5 billion years ago. Earlier physical evidence of life includes graphite, a biogenic substance, in 3.7 billion-year-old metasedimentary rocks discovered in southwestern Greenland, as well as, "remains of biotic life" found in 4.1 billion-year-old rocks in Western Australia.[33][34] Earth's biodiversity has expanded continually except when interrupted by mass extinctions.[35]Although scholars estimate that over 99% of all species of life (over five billion)[36] that ever lived on Earth areextinct,[37][38] there are still an estimated 10–14 million extant species,[39][40] of which about 1.2 million have been documented and over 86% have not yet been described.[41] Over 7.3 billion humans[42] live on Earth and depend on its biosphere and minerals for their survival. Earth's human population is divided among about two hundred sovereign states which interact through diplomacy, conflict, travel, trade and communication media.

 
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