Earth's atmosphere
The Earth's atmosphere is a layer of gases surrounding our planet and retained by the Earth's gravity. It contains roughly 78% nitrogen and 21% oxygen, with trace amounts of other gases. This mixture of gases is commonly known as air. The atmosphere has no abrupt boundary or cut-off. It slowly becomes thinner and fades away into outer space.
The atmosphere protects life on Earth by absorbing ultraviolet solar radiation and reducing temperature extremes between day and night.
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The Earth's atmosphere plays a vital role in sustaining life on this planet. Oxygen is needed for respiration by animals, plants, and some bacteria. Nitrogen is an inert gas that reduces the amount of oxygen available for the oxidation of natural materials, thus restricting spontaneous combustion (burning) of flammable materials and the corrosion of metals. Nitrogen is also used by "nitrogen-fixing" bacteria to produce compounds that are useful for plant growth. Plants that perform photosynthesis take up carbon dioxide from the air and release oxygen. Small amounts of carbon dioxide are also needed in human blood to act as a buffering agent.
Moreover, several regions of the atmosphere exert their protective effect from a distance. For instance, the ozone layer absorbs UV radiation that can damage the tissues and genetic material of living organisms. The mesosphere, in which millions of meteors burn up daily, protects the Earth's surface from being continually bombarded by these falling objects. The magnetosphere, which extends well beyond the atmosphere, protects the Earth from the damaging rain of charged particles carried by the solar wind.
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Three-quarters of the atmosphere's mass is within 11 km of the planetary surface. In the United States, persons who travel above an altitude of 50.0 miles (80.5 km) are designated as astronauts. An altitude of 120 km (75 mi or 400,000 ft) marks the boundary where atmospheric effects become noticeable during re-entry. The Karman line, at 100 km (62 mi), is also frequently used as the boundary between atmosphere and space.
Atmospheric layers
The properties of the Earth's atmosphere vary with altitude. Based on these properties, the atmosphere may be regarded as having different layers or zones. According to one system of nomenclature, there are five layers: the troposphere, stratosphere, mesosphere, thermosphere, and exosphere. The boundaries between these regions are called the tropopause, stratopause, mesopause, and exobase.
Troposphere
The troposphere (from the Greek words tropos = to turn or mix, and sphaira = ball) is the atmosphere's lowest and densest layer, and it is also known as the lower atmosphere. It starts from the Earth's surface and reaches up to about 7 km at the poles and 17 km at the equator, with some variation caused by weather factors. The upper boundary of this layer is called the tropopause.
The troposphere has a great deal of vertical mixing of its constituent gases, as a result of solar heat. As the Sun heats the Earth's surface, the air masses near the surface become warmer, rise, and release heat. That process further buoys the air masses. This sequence continues until all the water vapor in the air is removed.
The temperature of the troposphere decreases with height. At middle latitudes, the temperature drops from about +17°C at sea level to about -52°C at the beginning of the tropopause. At the poles, the troposphere is thinner and the temperature falls to only -45°C, while at the equator, the temperature at the top of the troposphere can reach -75°C.
Stratosphere
The stratosphere (from the New Latin word stratum = spread or bed) is situated directly above the troposphere and just below the mesosphere. In terms of its altitude range, it lies between about 10 km and 50 km at moderate latitudes, but it starts at about 8 km at the poles. This layer is dynamically stable, with no regular mixing of air and associated turbulence.
The stratosphere is stratified (layered) in temperature, with warmer layers higher up and cooler layers farther down—the reverse of the temperature variation in the troposphere. The upper layers of the stratosphere are heated by the presence of an ozone layer that absorbs ultraviolet (UV) radiation from the Sun—radiation that would otherwise be harmful to living organisms on Earth. The stratopause (at the top of the stratosphere) has a temperature of about 270K—fairly close to the temperature at ground level.
The base of the stratosphere occurs where heating by conduction from above and convection from below (through the troposphere) balance out. The stratosphere begins at lower altitudes near the poles because the ground temperatures are lower there.
Commercial airliners typically cruise at an altitude near 10 km in temperate latitudes, in the lower reaches of the stratosphere. In this manner, they avoid the atmospheric turbulence that occurs in the troposphere.
Mesosphere
The mesosphere (from the Greek word mesos = middle) is the layer between about 50 km and about 80–85 km above the Earth's surface. It is sandwiched between the stratosphere and the thermosphere. The temperature in this layer decreases with increasing altitude and can be as low as 200K (≈-99°F), varying according to latitude and season.
Given that it lies between the maximum altitude for most aircraft and the minimum altitude for most spacecraft, this region of the atmosphere is directly accessible only through the use of sounding rockets. As a result, it is one of the most poorly understood regions of the atmosphere.
Millions of meteors burn up daily in the mesosphere, as a result of collisions with the gas particles contained there, leading to a high concentration of iron and other metal atoms. The collisions almost always create enough heat to burn the falling objects long before they reach the ground. Thus the mesosphere protects the Earth from a barrage of would-be meteorites.
The stratosphere and mesosphere are referred to as the middle atmosphere. Regions above the mesosphere are called the upper atmosphere.
The mesopause, at an altitude of about 80 km, separates the mesosphere from the thermosphere. The mesopause lies near the turbopause, the band below which different chemical species are well mixed by turbulent eddies.
Thermosphere
The thermosphere (from the Greek word thermos for heat) extends from an altitude of 80–85 km to 640+ km. It lies directly above the mesosphere and right below the exosphere.
At these high altitudes, the residual atmospheric gases sort into strata according to their molecular masses. The temperature in this layer increases with altitude, due to the absorption of extremely energetic solar radiation by the small amount of oxygen present. Temperatures are highly dependent on solar activity and can rise to 2,000°C. Solar radiation causes the air particles in this layer to become ionized, that is, electrically charged (see Ionosphere under Additional atmospheric regions).
Astronauts travel at altitudes that exceed 80 km (50 miles), which means that they travel within or go beyond the thermosphere. An altitude of 120 km (75 miles) marks the boundary where atmospheric effects become noticeable during re-entry.
Exosphere
The exosphere (from the Greek word exo = out or outside) is the uppermost layer of the atmosphere. Its lower boundary at the edge of the thermosphere is estimated to be 500 km to 1,000 km above the Earth's surface, and its upper boundary at about 10,000 km.
It is only from the exosphere that atmospheric gases can, to any appreciable extent, escape into outer space. The main gases in the exosphere are the lightest ones, mainly hydrogen and helium, with some atomic oxygen near the exobase (the lowest altitude of the exosphere). The few particles of gas here can reach 2,500°C (4,500°F) during the day.
The atmosphere in this layer is sufficiently rarified for satellites to orbit the Earth, although they still receive some atmospheric drag. The exact altitude at which the exosphere ends and space begins is not well-defined, and attempting to attach a specific value to it is not particularly useful.
Additional atmospheric regions
Atmospheric regions are also named in other ways, as follows.
- Ozone layer (Ozonosphere): In the stratosphere, in an altitude range of about 10–50 km, the concentration of ozone is a few parts per million, which is much higher than the ozone concentration in the lower atmosphere (although it is still small compared to the main components of the atmosphere). This layer, known as the ozone layer, is vitally important to life because it absorbs biologically harmful UV radiation from the Sun.
- Ionosphere: This is the region of the atmosphere that contains ions (that form a "plasma"), created by the interaction of solar radiation with gas particles. The ionosphere overlaps with the mesosphere and thermosphere, going up to an altitude of 550 km. Its value in practical terms is that it enables the propagation of radio wave signals, which bounce off the ions and can be transmitted to distant places on the Earth.
- Magnetosphere: It is the region where the Earth's magnetic field interacts with the solar wind. Its inner boundary is the ionosphere, but it extends for tens of thousands of kilometers, with a long tail away from the Sun.
- Van Allen radiation belts: These are regions where charged particles (forming a plasma) from the solar wind are trapped by the Earth's magnetic field. When the belts "overload", particles strike the upper atmosphere and fluoresce, producing the effects known as the polar auroras. Qualitatively, there are two belts: an inner belt, consisting mostly of protons, and an outer belt, consisting mostly of electrons.
- Homosphere (or Turbosphere) and Heterosphere: The region below the turbopause (that is, below an altitude of about 100 km) is known as the homosphere or turbosphere, where the chemical constituents are well mixed and the composition of the atmosphere remains fairly uniform (see Composition of the atmosphere below) [1]. The region above the turbopause is called the heterosphere, where, in the absence of mixing, the chemical composition of the atmosphere varies (see Composition of the heterosphere below).
Pressure, density, and mass
- Atmospheric pressure (or barometric pressure) is a direct result of the weight of the air. It is highest at the Earth's surface and decreases with altitude. This is because air at the surface is compressed by the weight of all the air above it. Air pressure varies with location and time, because the amount (and weight) of air above the Earth varies with location and time.
- Atmospheric pressure drops by ~50% at an altitude of about 5 km. (In other words, about 50% of the total atmospheric mass is within the lowest 5 km). The average atmospheric pressure at sea level is about 101.3 kilopascals (about 14.7 pounds per square inch).
- The density of air at sea level is about 1.2 kg/m3, and it decreases as altitude increases.
- The average mass of the atmosphere is about 5,000 trillion metric tons.
Thickness of the atmosphere
- 57.8% of the atmosphere is below the summit of Mount Everest.
- 72% of the atmosphere is below the common cruising altitude of commercial airliners (about 10,000 m or 32,800 ft).
- 99.99999% of the atmosphere is below the highest flight altitude of the aircraft X-15, which reached 354,300 ft (108 km) on August 22, 1963. Therefore, most of the atmosphere (99.9999%) is below 100 km, although in the rarified region above this there are auroras and other atmospheric effects.
- The atmosphere exists at altitudes of 1,000 km and higher, but it is so thin as to be considered nonexistent.
Composition of the atmosphere
| ppmv: parts per million by volume | |
| Gas | Volume |
|---|---|
| Nitrogen (N2) | 780,840 ppmv (78.084%) |
| Oxygen (O2) | 209,460 ppmv (20.946%) |
| Argon (Ar) | 9,340 ppmv (0.9340%) |
| Carbon dioxide (CO2) | 350 ppmv |
| Neon (Ne) | 18.18 ppmv |
| Helium (He) | 5.24 ppmv |
| Methane (CH4) | 1.745 ppmv |
| Krypton (Kr) | 1.14 ppmv |
| Hydrogen (H2) | 0.55 ppmv |
| Not included in above dry atmosphere: | |
| Water vapor (highly variable) | typically 1% |
Source for figures above: NASA. Carbon dioxide and methane updated (to 1998) by IPCC TAR table 6.1 [2]. The NASA total was 17 ppmv over 100%, and CO2 was increased here by 15 ppmv. To normalize, N2 should be reduced by about 25 ppmv and O2 by about 7 ppmv.
Minor components of air not listed above include:
| Gas | Volume |
|---|---|
| nitrous oxide | 0.5 ppmv |
| xenon | 0.09 ppmv |
| ozone | 0.0 to 0.07 ppmv |
| nitrogen dioxide | 0.02 ppmv |
| iodine | 0.01 ppmv |
| carbon monoxide | trace |
| ammonia | trace |
Composition of the heterosphere
Above the turbopause (about 100 km), the Earth's atmosphere begins to have a composition that varies with altitude. This is essentially because, in the absence of mixing, the density of a gas falls off exponentially with increasing altitude, at a rate that depends on the molecular mass of the gas. Higher mass constituents, such as oxygen and nitrogen, fall off more quickly than lighter constituents such as helium, molecular hydrogen, and atomic hydrogen. Thus, as the altitude increases in the heterosphere, the atmosphere is dominated successively by helium, molecular hydrogen, and atomic hydrogen. The precise altitude of the heterosphere and the layers it contains varies significantly with temperature[3].
Biological significance
The Earth's atmosphere plays a vital role in sustaining life on this planet. Oxygen is needed for respiration by animals, plants, and some bacteria. Nitrogen is an inert gas that reduces the amount of oxygen available for the oxidation of natural materials, thus restricting spontaneous combustion (burning) of flammable materials and the corrosion of metals. Nitrogen is also used by "nitrogen-fixing" bacteria to produce compounds that are useful for plant growth. Plants that perform photosynthesis take up carbon dioxide from the air and release oxygen. Carbon dioxide and water vapor act as "greenhouse gases" that keep the Earth sufficiently warm to maintain life. Water vapor in the air is part of the water cycle that produces precipitation in the form of rain and snow. In addition, water vapor prevents exposed living tissue from drying up.
Moreover, several regions of the atmosphere exert their protective effect from a distance. For instance, the ozone layer absorbs UV radiation that can damage the tissues and genetic material of living organisms. The mesosphere, in which millions of meteors burn up daily, protects the Earth's surface from being continually bombarded by these falling objects. The magnetosphere, which extends well beyond the atmosphere, protects the Earth from the damaging rain of charged particles carried by the solar wind.
History of the Earth's atmosphere
The history of the Earth's atmosphere prior to one billion years ago is poorly understood, but one plausible sequence of events is given below.
The modern atmosphere is sometimes referred to as Earth's "third atmosphere", to distinguish its chemical composition from two notably different earlier compositions. It is thought that the original atmosphere was primarily helium and hydrogen. Heat (from the still-molten crust and the Sun) dissipated this atmosphere.
About 3.5 billion years ago, the surface had cooled sufficiently to form a solid crust, still heavily populated with volcanoes that released steam, carbon dioxide, and ammonia. This led to formation of the "second atmosphere", composed primarily of carbon dioxide and water vapor, with some nitrogen but virtually no oxygen. (Simulations run at the University of Waterloo and University of Colorado in 2005 suggested that it may have had up to 40% hydrogen [4]). This second atmosphere had approximately 100 times as much gas as the current atmosphere. It is generally believed that the greenhouse effect, caused by high levels of carbon dioxide, kept the Earth from freezing.
During the next few million years, water vapor condensed to form rain and oceans, which began to dissolve carbon dioxide. Approximately 50% of the carbon dioxide was absorbed into the oceans.
Fossil evidence indicates that cyanobacteria were among the earliest types of bacterial life, existing approximately 3.3 billion years ago. They were the first organisms to carry out the photosynthetic conversion of carbon dioxide into oxygen, thus playing a major role in transforming the atmosphere from an anoxic state (a state without oxygen) to an oxic state (a state with oxygen).
Later, photosynthesizing plants emerged and converted more carbon dioxide into oxygen. Over time, excess carbon became locked into fossil fuels, sedimentary rocks (notably limestone), and animal shells. As oxygen was released, it reacted with ammonia to generate nitrogen. In addition, bacteria also converted ammonia into nitrogen.
As more plants appeared, the levels of oxygen increased significantly, while carbon dioxide levels dropped. At first, the oxygen combined with various elements (such as iron), but eventually oxygen accumulated in the atmosphere. With the appearance of an ozone layer, life forms were better protected from UV radiation. This oxygen-nitrogen atmosphere is the "third atmosphere".
ReferencesISBN links support NWE through referral fees
- The thermosphere: a part of the heterosphere, by J. Vercheval.
See also
- Air glow
- Atmospheric electricity
- Atmospheric dispersion modeling
- Compressed air
- Global warming
- Greenhouse effect
- Historical temperature record
- Intergovernmental Panel on Climate Change (IPCC)
External links
- NASA atmosphere models
- NASA's Earth Fact Sheet
- American Geophysical Union: Atmospheric Sciences
- Layers of the Atmosphere
- The AMS Glossary of Meteorology
|
Troposphere | Stratosphere | Mesosphere | Thermosphere | Exosphere |
|
Tropopause | Stratopause | Mesopause | Exobase |
|
Ozone layer | Turbopause | Ionosphere |
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