The Blue Marble photograph of Earth, taken during the Apollo 17 lunar mission in 1972
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Orbital characteristics | |||||||||||||||||
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Epoch J2000 | |||||||||||||||||
Aphelion |
152100000 km (94500000 mi; 1.017 AU) |
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Perihelion |
147095000 km (91401000 mi; 0.98327 AU) |
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149598023 km (92955902 mi; 1.00000102 AU) |
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Eccentricity | 7086 0.016 | ||||||||||||||||
365.256363004 d (1.00001742096 yr) |
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Average orbital speed
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29.78 km/s (107200 km/h; 66600 mph) |
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358.617° | |||||||||||||||||
Inclination |
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64° to J2000 ecliptic −11.260 | |||||||||||||||||
83° 114.207 | |||||||||||||||||
Satellites |
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Physical characteristics | |||||||||||||||||
Mean radius
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6371.0 km (3958.8 mi) | ||||||||||||||||
Equatorial radius
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6378.1 km (3963.2 mi) | ||||||||||||||||
Polar radius
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6356.8 km (3949.9 mi) | ||||||||||||||||
Flattening |
3528 0.003 1/222101 ( 298.257ETRS89) |
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Circumference |
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Volume | 21×1012 km3 1.083 (76×1011 cu mi) 2.598 | ||||||||||||||||
Mass |
37×1024 kg ( 5.97268×1025 lb) 1.316 (×10−6 M☉) 3.0 |
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Mean density
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5.514 g/cm3(0.1992 lb/cu in) | ||||||||||||||||
9.807 m/s2( 1 g; 32.18 ft/s2) | |||||||||||||||||
0.3307 | |||||||||||||||||
11.186 km/s (40270 km/h; 25020 mph) |
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Sidereal rotation period
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26968 d 0.997
(23h 56m 4.100s) |
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Equatorial rotation velocity
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0.4651 km/s (1674.4 km/h; 1040.4 mph) |
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2811° 23.439 | |||||||||||||||||
Albedo | |||||||||||||||||
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Atmosphere | |||||||||||||||||
Surface pressure
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kPa (at 101.325 MSL) | ||||||||||||||||
Composition by volume |
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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, 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 about its axis about 366.26 times.
Earth's axis of rotation is tilted with respect to its orbital plane, 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'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. 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 mantle that drives plate tectonics.