http://youtube.com/watch?v=M8g3u7BNrWM
Earth is the only planet whose English name does not derive from Greek/Roman mythology. The name derives from Old English and Germanic. There are, of course, hundreds of other names for the planet in other languages. In Roman Mythology, the goddess of the Earth was Tellus - the fertile soil (Greek: Gaia, terra mater - Mother Earth).
It was not until the time of Copernicus (the sixteenth century) that it was understood that the Earth is just another planet.
Mir space station and Earth's limb Earth, of course, can be studied without the aid of spacecraft. Nevertheless it was not until the twentieth century that we had maps of the entire planet. Pictures of the planet taken from space are of considerable importance; for example, they are an enormous help in weather prediction and especially in tracking and predicting hurricanes. And they are extraordinarily beautiful.
The Earth is divided into several layers which have distinct chemical and seismic properties (depths in km):
0- 40 Crust
40- 400 Upper mantle
400- 650 Transition region
650-2700 Lower mantle
2700-2890 D'' layer
2890-5150 Outer core
5150-6378 Inner core
The crust varies considerably in thickness, it is thinner under the oceans, thicker under the continents. The inner core and crust are solid; the outer core and mantle layers are plastic or semi-fluid. The various layers are separated by discontinuities which are evident in seismic data; the best known of these is the Mohorovicic discontinuity between the crust and upper mantle.
Most of the mass of the Earth is in the mantle, most of the rest in the core; the part we inhabit is a tiny fraction of the whole (values below x10^24 kilograms):
atmosphere = 0.0000051
oceans = 0.0014
crust = 0.026
mantle = 4.043
outer core = 1.835
inner core = 0.09675
The core is probably composed mostly of iron (or nickel/iron) though it is possible that some lighter elements may be present, too. Temperatures at the center of the core may be as high as 7500 K, hotter than the surface of the Sun. The lower mantle is probably mostly silicon, magnesium and oxygen with some iron, calcium and aluminum. The upper mantle is mostly olivene and pyroxene (iron/magnesium silicates), calcium and aluminum. We know most of this only from seismic techniques; samples from the upper mantle arrive at the surface as lava from volcanoes but the majority of the Earth is inaccessible. The crust is primarily quartz (silicon dioxide) and other silicates like feldspar. Taken as a whole, the Earth's chemical composition (by mass) is:
South America by Galileo
34.6% Iron
29.5% Oxygen
15.2% Silicon
12.7% Magnesium
2.4% Nickel
1.9% Sulfur
0.05% Titanium
The Earth is the densest major body in the solar system.
The other terrestrial planets probably have similar structures and compositions with some differences: the Moon has at most a small core; Mercury has an extra large core (relative to its diameter); the mantles of Mars and the Moon are much thicker; the Moon and Mercury may not have chemically distinct crusts; Earth may be the only one with distinct inner and outer cores. Note, however, that our knowledge of planetary interiors is mostly theoretical even for the Earth.
Unlike the other terrestrial planets, Earth's crust is divided into several separate solid plates which float around independently on top of the hot mantle below. The theory that describes this is known as plate tectonics. It is characterized by two major processes: spreading and subduction. Spreading occurs when two plates move away from each other and new crust is created by upwelling magma from below. Subduction occurs when two plates collide and the edge of one dives beneath the other and ends up being destroyed in the mantle. There is also transverse motion at some plate boundaries (i.e. the San Andreas Fault in California) and collisions between continental plates (i.e. India/Eurasia). There are (at present) eight major plates:
North American Plate - North America, western North Atlantic and Greenland Earth's Plate Boundaries delineated by earthquake epicenters South American Plate - South America and western South Atlantic
Antarctic Plate - Antarctica and the "Southern Ocean"
Eurasian Plate - eastern North Atlantic, Europe and Asia except for India
African Plate - Africa, eastern South Atlantic and western Indian Ocean
Indian-Australian Plate - India, Australia, New Zealand and most of Indian Ocean
Nazca Plate - eastern Pacific Ocean adjacent to South America
Pacific Plate - most of the Pacific Ocean (and the southern coast of California!)
There are also twenty or more small plates such as the Arabian, Cocos, and Philippine Plates. Earthquakes are much more common at the plate boundaries. Plotting their locations makes it easy to see the plate boundaries.
The Earth's surface is very young. In the relatively short (by astronomical standards) period of 500,000,000 years or so erosion and tectonic processes destroy and recreate most of the Earth's surface and thereby eliminate almost all traces of earlier geologic surface history (such as impact craters). Thus the very early history of the Earth has mostly been erased. The Earth is 4.5 to 4.6 billion years old, but the oldest known rocks are about 4 billion years old and rocks older than 3 billion years are rare. The oldest fossils of living organisms are less than 3.9 billion years old. There is no record of the critical period when life was first getting started.
Space Shuttle view of the Strait of Gibraltar 71 Percent of the Earth's surface is covered with water. Earth is the only planet on which water can exist in liquid form on the surface (though there may be liquid ethane or methane on Titan's surface and liquid water beneath the surface of Europa). Liquid water is, of course, essential for life as we know it. The heat capacity of the oceans is also very important in keeping the Earth's temperature relatively stable. Liquid water is also responsible for most of the erosion and weathering of the Earth's continents, a process unique in the solar system today (though it may have occurred on Mars in the past).
Earth's atmosphere seen at the limb The Earth's atmosphere is 77% nitrogen, 21% oxygen, with traces of argon, carbon dioxide and water. There was probably a very much larger amount of carbon dioxide in the Earth's atmosphere when the Earth was first formed, but it has since been almost all incorporated into carbonate rocks and to a lesser extent dissolved into the oceans and consumed by living plants. Plate tectonics and biological processes now maintain a continual flow of carbon dioxide from the atmosphere to these various "sinks" and back again. The tiny amount of carbon dioxide resident in the atmosphere at any time is extremely important to the maintenance of the Earth's surface temperature via the greenhouse effect. The greenhouse effect raises the average surface temperature about 35 degrees C above what it would otherwise be (from a frigid -21 C to a comfortable +14 C); without it the oceans would freeze and life as we know it would be impossible. (Water vapor is also an important greenhouse gas.)
View from Apollo 11 The presence of free oxygen is quite remarkable from a chemical point of view. Oxygen is a very reactive gas and under "normal" circumstances would quickly combine with other elements. The oxygen in Earth's atmosphere is produced and maintained by biological processes. Without life there would be no free oxygen.
The interaction of the Earth and the Moon slows the Earth's rotation by about 2 milliseconds per century. Current research indicates that about 900 million years ago there were 481 18-hour days in a year.
Earth has a modest magnetic field produced by electric currents in the outer core. The interaction of the solar wind, the Earth's magnetic field and the Earth's upper atmosphere causes the auroras (see the Interplanetary Medium). Irregularities in these factors cause the magnetic poles to move and even reverse relative to the surface; the geomagnetic north pole is currently located in northern Canada. (The "geomagnetic north pole" is the position on the Earth's surface directly above the south pole of the Earth's field; see this diagram.)
The Earth's magnetic field and its interaction with the solar wind also produce the Van Allen radiation belts, a pair of doughnut shaped rings of ionized gas (or plasma) trapped in orbit around the Earth. The outer belt stretches from 19,000 km in altitude to 41,000 km; the inner belt lies between 13,000 km and 7,600 km in altitude.
Earth's Satellite
Earth has only one natural satellite, the Moon. But
thousands of small artificial satellites have also been placed in orbit around the Earth.
Asteroids 3753 Cruithne and 2002 AA29 have complicated orbital relationships with the Earth; they're not really moons, the term "companion" is being used. It is somewhat similar to the situation with Saturn's moons Janus and Epimetheus.
Lilith doesn't exist but it's an interesting story.
Distance Radius Mass
Satellite (000 km) (km) (kg)
--------- -------- ------ -------
Moon 384 1738 7.35e22
More about Earth and the Moon
Web www.nineplanets.org
more Earth images and movies
the Blue Marble, very high resolution true color imagery
from NSSDC
U.S. Geological Survey
An image of Earth as seen from Mars taken by Mars Global Surveyor
pictures of Terrestrial Clouds from space (LANL)
text and pictures of Terrestrial Impact Craters (LANL)
pictures of Terrestrial and Hawaiian Volcanoes (LANL)
Volcano World
Electric Volcano
Geomagnetism FAQ
more about the magnetic pole
A Beginner's Guide to the Earth's Magnetosphere
The Magnetosphere
Earth Viewer, an interactive map of the Earth
Earth As Seen From Space (images and astronaut quotes; by Calvin Hamilton of LANL)
Earth from Space, NASA images of Earth
Geography resources
why the sky is blue
Landsat images of the USA
AVHRR images USA land use (AVHRR false color) Encyclopedia of the Atmospheric Environment
Open Issues
Our knowledge of the interior of the Earth is derived almost entirely from highly indirect evidence. How can we get more information?
Despite substantial increases in the solar "constant" the average temperature on the surface of the Earth has remained very stable for several billion years. The best theory is that this has been accomplished by varying the amount of carbon dioxide in the atmosphere to regulate the greenhouse effect. But just how is this done? The Gaia Hypothesis asserts that the biosphere actively regulates it. More detailed information about Venus and Mars may provide clues.
How much more carbon dioxide can we dump into the Earth's atmosphere before it ends up like Venus?
2007-04-06 07:35:17
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answer #1
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answered by Anonymous
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To pass on my genetic material to future generations,a nd help proliferate the species. At least, that is my scientific purpose.
My personal purpose, since I can't spend all my time reproducing, is to try to help make the world a better place for those future generations, to understand where I came from and where we might be going, and to be happy since I think I only have one shot at this.
2007-04-05 12:22:44
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answer #2
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answered by kiddo 4
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From a biological standpoint, to continue the species - same as all other organisms. From a social standpoint, to interact with others and create something better than what we could alone. Other than that, the reasons are mostly too subjective for disclosure.
2007-04-05 11:52:08
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answer #3
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answered by the buffster 5
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Mankind is the only creature on this world that thinks like that. There is no ultimate purpose. We are born,live and die and that's all. No higher reason,wisdom,necessity is involved.WE developed big brains that developed big EGO's.
2007-04-05 11:29:54
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answer #4
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answered by Anonymous
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To pertain existence, and continue the human race
2007-04-05 11:49:33
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answer #5
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answered by 2447 3
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being a Good citizen of this world as we living''i want to share a part whether it Posible or Impossible Mission there is always an answer to a ""CLUE""i expect to feel a cool air today or rain tommorow
2007-04-05 11:52:55
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answer #6
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answered by Anonymous
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Men exist to woo women. Women exist to be wooed. Everything else is commentary.
2007-04-05 11:50:44
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answer #7
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answered by Anonymous
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I often wonder my purpose in life. Destined to be the first man to run naked on the moon? Cool! Good to see you back, missed you!
2016-05-18 00:51:42
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answer #8
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answered by ? 3
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same reason all other species exist on earth. to regenerate and replenish the earth.
2007-04-05 21:40:01
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answer #9
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answered by Zeppfan35 3
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To learn and grow ...like everything else that lives on earth.
2007-04-05 11:27:46
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answer #10
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answered by Anonymous
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To be Jordan's Mom. What better could I do for the world?
2007-04-05 11:28:09
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answer #11
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answered by Colette B 5
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