(Redirected from Earth Sciences)
'Earth science' (also known as 'geoscience', 'the geosciences' or 'the Earth Sciences'), is an all-embracing term for the sciences related to the planet
Earth. It is arguably a special case in
planetary science, being the only known
life-bearing planet. There are both
reductionist and
holistic approaches to Earth science. The major historic
disciplines use
physics,
geology,
geography,
meteorology,
mathematics,
chemistry and
biology to build a quantitative understanding of the principal areas or ''
spheres'' of the Earth system.
Earth's spheres
Earth science generally recognizes 4 spheres, the lithosphere, the hydrosphere, the atmosphere, and the biosphere. These correspond to rocks, water, air, and life. Some practitioners include the cryosphere (ice) as a distinct portion of the hydrosphere and the pedosphere (soil) as an active, intermixed sphere as part of Earth's spheres.
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Geology describes the
rocky parts of the Earth's
crust (or
lithosphere) and its historic development. Major subdisciplines are
mineralogy and
petrology,
geochemistry,
geomorphology,
paleontology,
stratigraphy,
engineering geology and
sedimentology.
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Geophysics and
Geodesy investigate the
figure of the Earth, its reaction to forces and its
magnetic and
gravity fields. Geophysicists explore the
Earth's core and
mantle as well as the
tectonic and
seismic activity of the lithosphere.
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Soil science covers the outermost layer of the Earth's crust that is subject to soil formation processes (or
pedosphere). Major subdisciplines include
edaphology and
pedology.
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Oceanography and
hydrology (incl.
limnology) describe the marine and freshwater domains of the
watery parts of the Earth (or
hydrosphere). Major subdisciplines include
hydrogeology and
physical,
chemical, and
biological oceanography.
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Glaciology covers the
icy parts of the Earth (or
cryosphere).
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Atmospheric sciences cover the
gaseous parts of the Earth (or
atmosphere) between the surface and the
exosphere (~1000 km). Major subdisciplines are
meteorology,
climatology,
atmospheric chemistry and
atmospheric physics.
★ The most important and linking sphere is the biosphere, and consists of all forms of life, from single-celled organisms to pine trees to people. The interactions of Earth's other spheres - lithosphere/geosphere, hydrosphere, atmosphere and/or cryosphere and pedosphere - create the conditions that can support life.
Earth's energy
In
geology,
plate tectonics,
mountain ranges,
volcanoes, and
earthquakes are phenomena that can be explained in terms of
energy transformations in the
Earth's crust[1]. Recent studies suggest that the Earth transforms about 6.18 x 10
-12 J/s (joules per second) per kilogram. Given the
Earth's mass, the rate of energy transformations inside the Earth is about 37 x 10
12 J/s (37 terawatts). The heat escaping from inside the Earth is only about 0.02% of the amount of energy Earth receives from Sun in the form of sunlight, and radiates back into space in the form of
infrared blackbody radiation (~1.74 x 10
17 J/s = 174 petawatts).
From the study of
neutrinos radiated from the Earth (see
KamLAND), scientists have recently estimated that about 24 terawatts (65%) of this rate of
energy transformation is due to
radioactive decay (principally of
potassium 40,
thorium 232 and
uranium 238), and the remaining 13 terawatts is from the continuous gravitational ''sorting'' of the
core and
mantle of the earth, energies left over from the
formation of the Earth, about 4.57 billion years ago (this sorting represents continuing
gravitational collapse of the Earth into the maximally compact object which is consistent with its composition-- a process which releases gravitational potential energy), and finally - from
tidal flexing of Earth's interior and crust. The magnitude of all of these energy sources decline over time, and based on half-life alone, it has been estimated that the current
radioactive energy of the planet represents less than 1% of that which was available at the time the planet was formed.
As a result, geological forces of
continental accretion,
subduction and
sea floor spreading, account for 90% of the Earth's energy. The remaining 10% of geological tectonic energy comes through
hotspots produced by
mantle plumes, resulting in
shield volcanoes like
Hawaii,
geyser activity like
Yellowstone or
flood basalts like
Iceland.
Tectonic process are driven by heat from the Earth's interior. The process is a simple heat engine which works via the upward buoyancy-induced motion of hot, low density
magma after expansion by heat. The processes
metamorphically alter crustal rocks, and (more importantly from the energy view) during
orogenies, lift them up into mountain ranges. The potential energy represented by the mountain range's weight and height thus represents heat from the core of the Earth which has been partly transformed into gravitational potential energy. This potential energy may be suddenly released in landslides or
tsunamis. Similarly, the energy release which drives an earthquake represents stresses in rocks that are mechanical potential energy which has been similarly stored from tectonic processes. An earthquake thus ultimately represents kinetic energy which is being released from elastic potential energy in rocks, which in turn has been stored from heat energy released by radioactive decay and gravitational collapse in the Earth's interior.
The energy which is responsible for the geological processes of erosion and deposition is a result of the interaction of solar energy and gravity. An estimated 23% of the total insolation is used to drive the
water cycle. When
water vapour condenses to fall as
rain, it dissolves small amounts of
carbon dioxide, making a weak
acid. This acid acting upon the metallic
silicate minerals that form most rocks produces
chemical weathering, removing the metals, and leading to the production of rocks and sand, carried by wind and water downslope through gravity to be deposited at the edge of continents in the sea.
Physical weathering of rocks is produced by the expansion of ice crystals, left by water in the joint planes of rocks. A
geologic cycle is continued when these eroded
sediments are buried and later uplifted into mountains.
Similarly meteorological phenomena like
wind,
rain,
hail,
snow,
lightning,
tornadoes and
hurricanes, are all a result of energy transformations brought about by solar energy on the planet Earth. It has been estimated that the average total ''solar incoming radiation'' (or
insolation) is about 1350 watts per square meter incident to the summit of the atmosphere, at the equator at midday, a figure known as the
solar constant. Although this amount varies a little each year, as a result of
solar flares,
prominences and the
sunspot cycle. Some 34% of this is immediately reflected by the planetary
albedo, as a result of clouds, snowfields, and even reflected light from water, rock or vegetation. As more energy is received in the tropics than is re-radiated, while more energy is radiated at the poles than is received, climatic homeostasis is only maintained by a transfer of energy from the tropics to the poles.
This transfer of energy is what drives the winds and the
ocean currents. Like biological processes, all meteorological processes involve transformation of energy from a concentrated form such as sunlight into a less concentrated form, such as far infrared radiation (i.e., heat radiation) at the much smaller characteristic temperatures that occur on Earth, and thus is diffused into many photons. However, energy may be temporarily locally stored during this process, and the sudden release of such stored sources is responsible for the dramatic processes mentioned above. For example, the kinetic energy of a snow-avalanche or hurricane is due to the sudden release of energy previously captured from solar radiations.
Methodology
Like all other scientists, Earth scientists apply the
scientific method: formulate hypotheses after observation of and gathering data about natural phenomena and then test those hypotheses. In Earth science, data usually plays a major role in testing and formulating hypotheses.
Partial list of the major Earth Science topics
Atmosphere
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Atmospheric chemistry
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Climatology
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Meteorology
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Hydrometeorology
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Paleoclimatology
Biosphere
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Biogeography
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Paleontology
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Palynology
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Micropaleontology
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Geomicrobiology
Hydrosphere
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Hydrology
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Glaciology
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Limnology
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Hydrogeology
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Oceanography
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Chemical oceanography
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Marine biology
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Marine geology
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Paleoceanography
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Physical oceanography
Lithosphere or geosphere
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Geology
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Economic geology
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Engineering geology
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Environmental geology
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Historical geology
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Glaciology
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Quaternary geology
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Planetary geology
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Sedimentology
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Stratigraphy
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Structural geology
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Geochemistry
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Geography
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Physical geography
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Geomorphology
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Geophysics
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Geochronology
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Geodynamics (see also
Tectonics)
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Geomagnetics
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Gravimetry (also part of
Geodesy)
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Seismology
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Hydrogeology
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Mineralogy
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Crystallography
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Gemology
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Petrology
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Volcanology
Pedosphere
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Soil science
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Edaphology
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Pedology
Systems
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Environmental science
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Geography
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Human geography
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Physical Geography
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Gaia theories
Others
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Cartography
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Geoinformatics (
GIS)
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Geostatistics
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Geodesy and
Surveying
Notes and references
1. http://okfirst.ocs.ou.edu/train/meteorology/EnergyBudget.html
See also
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List of basic earth science topics
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List of geoscience organizations