TradeTrade is the voluntary exchange of goods, services, or both. Trade is also called commerce. A mechanism that allows trade is called a market. The original form of trade was barter, the direct exchange of goods and services. Modern traders instead generally negotiate through a medium of exchange, such as money. As a result, buying can be separated from selling, or earning. The invention of money (and later credit, paper money and non-physical money) greatly simplified and promoted trade. Trade between two traders is called bilateral trade, while trade between more than two traders is called multilateral trade. Trade exists for many reasons. Due to specialization and division of labor, most people concentrate on a small aspect of production, trading for other products. Trade exists between regions because different regions have a comparative advantage in the production of some tradable commodity, or because different regions' size allows for the benefits of mass production. As such, trade at market prices between locations benefits both locations. History of tradeTrade originated with the start of communication in prehistoric time. Trading was the main facility of prehistoric people, who bartered goods and services from each other. Peter Watson dates the history of long-distance commerce from circa 150,000 years ago.[1] Trade is believed to have taken place throughout much of recorded human history. There is evidence of the exchange of obsidian and flint during the stone age. Materials used for creating jewelry were traded with Egypt since 3000 BCE. Long-range trade routes first appeared in the 3rd millennium BCE, when Sumerians in Mesopotamia traded with the Harappan civilization of the Indus Valley. The Phoenicians were noted sea traders, travelling across the Mediterranean Sea, and as far north as Britain for sources of tin to manufacture bronze. For this purpose they established trade colonies the Greeks called emporia. From the beginning of Greek civilization until the fall of the Roman empire in the 5th century, a financially lucrative trade brought valuable spice to Europe from the far east, including China. Roman commerce allowed their empire to flourish and endure. Their widespread empire produced a stable and secure transportation network that enabled the shipment of trade goods without fear of significant piracy. The fall of the Roman empire, and the succeeding Dark Ages brought instability to Western Europe and a near collapse of the trade network. Nevertheless some trade did occur. For instance, Radhanites were a medieval guild or group (the precise meaning of the word is lost to history) of Jewish merchants who traded between the Christians in Europe and the Muslims of the Near East. From the 8th to the 11th century, the Vikings and Varangians traded as they sailed from and to Scandinavia. Vikings sailed to Western Europe, while Varangians to Russia. The Hanseatic League was an alliance of trading cities that maintained a trade monopoly over most of Northern Europe and the Baltic, between the 13th and 17th centuries. The tales of Marco Polo's travels to the far east sparked an interest in the spice trade.Vasco da Gama started the Spice trade in 1498. The spice trade was of major economic importance and helped spur the Age of Exploration. Spices brought to Europe from distant lands were some of the most valuable commodities for their weight, sometimes rivaling gold. In the 16th century, Holland was the centre of free trade, imposing no exchange controls, and advocating the free movement of goods. Trade in the East Indies was dominated by Portugal in the 16th century, the Netherlands in the 17th century, and the British in the 18th century. In 1776, Adam Smith published the paper An Inquiry into the Nature and Causes of the Wealth of Nations. It criticised Mercantilism, and argued that economic specialization could benefit nations just as much as firms. Since the division of labour was restricted by the size of the market, he said that countries having access to larger markets would be able to divide labour more efficiently and thereby become more productive. Smith said that he considered all rationalizations of import and export controls "dupery", which hurt the trading nation at the expense of specific industries. In 1799, the Dutch East India Company, formerly the world's largest company, became bankrupt, partly due to the rise of competitive free trade. In 1817, David Ricardo, James Mill and Robert Torrens showed that free trade might benefit the industrially weak as well as the strong, in the famous theory of comparative advantage. In Principles of Political Economy and Taxation Ricardo advanced the doctrine still considered the most counterintuitive in economics: The ascendancy of free trade was primarily based on national advantage in the mid 19th century. That is, the calculation made was whether it was in any particular country's self-interest to open its borders to imports. John Stuart Mill proved that a country with monopoly pricing power on the international market could manipulate the terms of trade through maintaining tariffs, and that the response to this might be reciprocity in trade policy. Ricardo and others had suggested this earlier. This was taken as evidence against the universal doctrine of free trade, as it was believed that more of the economic surplus of trade would accrue to a country following reciprocal, rather than completely free, trade policies. This was followed within a few years by the infant industry scenario developed by Mill anticipated New Trade Theory by promoting the theory that government had the "duty" to protect young industries, although only for a time necessary for them to develop full capacity. This became the policy in many countries attempting to industrialize and out-compete English exporters. The Great Depression was a major economic recession that ran from 1929 to 1941. During this period, there was a great drop in trade and other economic indicators. The lack of free trade was considered by many as a principal cause of the depression, and World War II. During the war, in 1944, 44 countries signed the Bretton Woods Agreement, intended to prevent national trade barriers, to avoid depressions. It set up rules and institutions to regulate the international political economy: the International Monetary Fund and the International Bank for Reconstruction and Development (later divided into the World Bank and Bank for International Settlements). These organizations became operational in 1946 after enough countries ratified the agreement. In 1947, 23 countries agreed to the General Agreement on Tariffs and Trade to promote free trade. Free trade advanced further in the late 20th century and early 2000s:
Development of moneyTo meet Wikipedia's quality standards, this article or section may require cleanup.See rationale on the talk page, or replace this tag with a more specific message. Editing help is available. This article has been tagged since August 2005. Main article: History of money The first instances of money were objects with intrinsic value. This is called commodity money and includes any commonly-available commodity that has intrinsic value; historical examples include pigs, rare seashells, whale's teeth, and (often) cattle. In medieval Iraq, bread was used as an early form of money. In Mexico under Montezuma cocoa beans were money. [1] Roman denariusCurrency was introduced as a standardized money to facilitate a wider exchange of goods and services. This first stage of currency, where metals were used to represent stored value, and symbols to represent commodities, formed the basis of trade in the Fertile Crescent for over 1500 years. Numismatists have examples of coins from the earliest large-scale societies, although these were initially unmarked lumps of precious metal[2]. Ancient Sparta minted coins from iron to discourage its citizens from engaging in foreign trade. The system of commodity money in many instances evolved into a system of representative money. In this system, the material that constitutes the money itself had very little intrinsic value, but none the less such money achieves significant market value through being scarce as an artifact. This page about Trading includes information from a Wikipedia article. Additional articles about Trading News stories about Trading External links for Trading Videos for Trading Wikis about Trading Discussion Groups about Trading Blogs about Trading Images of Trading |
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In this system, the material that constitutes the money itself had very little intrinsic value, but none the less such money achieves significant market value through being scarce as an artifact. In 1887 the Michelson-Morley experiment, using an interferometer to attempt to detect the change in the speed of light caused by the Earth moving with respect to the aether, was a famous null result, showing that there really was no static, pervasive medium throughout space and through which the Earth moved as though through a wind. The system of commodity money in many instances evolved into a system of representative money. This evolved into the luminiferous aether of the 19th century, but the idea was known to have significant shortcomings - specifically that if the Earth is moving through a material medium, the medium would have to be both extremely tenuous (because the earth is not being detectably slowed in its orbit), and extremely rigid (because vibrations propagate so fast). Ancient Sparta minted coins from iron to discourage its citizens from engaging in foreign trade. In the 17th century, theories of the nature of light had required the idea of an aethereal medium which would be the medium to convey waves of light (Newton relied on this idea to explain refraction and radiated heat). Numismatists have examples of coins from the earliest large-scale societies, although these were initially unmarked lumps of precious metal[2]. This led to the development of the vacuum tube. This first stage of currency, where metals were used to represent stored value, and symbols to represent commodities, formed the basis of trade in the Fertile Crescent for over 1500 years. A number of electrical properties become observable at this vacuum level, and this renewed interest in vacuum. Currency was introduced as a standardized money to facilitate a wider exchange of goods and services. The study of vacuum then lapsed until 1855 when Heinrich Geissler invented the mercury displacement pump and achieved a record vacuum of about 0.1 Torr. [1]. In 1654, Otto von Guericke conducted his famous Magdeburg hemispheres experiment, showing that teams of horses could not separate two hemispheres from which the air had been evacuated. In Mexico under Montezuma cocoa beans were money. Robert Boyle later conducted experiments on the properties of vacuum. In medieval Iraq, bread was used as an early form of money. Some people believe that although Torricelli produced the first vacuum, it was Blaise Pascal who recognized it for what it was. This is called commodity money and includes any commonly-available commodity that has intrinsic value; historical examples include pigs, rare seashells, whale's teeth, and (often) cattle. Following work by Galileo, Evangelista Torricelli argued in 1643 that there was a vacuum at the top of a mercury barometer. The first instances of money were objects with intrinsic value. Opposition to the idea of a vacuum existing in nature continued into the Scientific Revolution, with scholars such as Paolo Casati taking an anti-vacuist position. Main article: History of money. This speculation became irrelevant after the Paris condemnations of Bishop Tempier, which required there to be no restrictions on the powers of God, which led to the conclusion that God could create a vacuum if he so wished. Free trade advanced further in the late 20th century and early 2000s:. There was much discussion of whether the air moved in quickly enough as the plates were separated, or, following William Burley whether a 'celestial agent' prevented the vacuum arising—that is, whether nature abhorred a vacuum. In 1947, 23 countries agreed to the General Agreement on Tariffs and Trade to promote free trade. Medieval thought experiments into the idea of a vacuum considered whether a vacuum was present, if only for an instant, between two flat plates when they were rapidly separated. These organizations became operational in 1946 after enough countries ratified the agreement. The absence of anything implied the absence of God, and hearkened back to the void prior to the story of creation in the book of Genesis. It set up rules and institutions to regulate the international political economy: the International Monetary Fund and the International Bank for Reconstruction and Development (later divided into the World Bank and Bank for International Settlements). In the Middle Ages, the idea of a vacuum was thought to be immoral or even heretical. During the war, in 1944, 44 countries signed the Bretton Woods Agreement, intended to prevent national trade barriers, to avoid depressions. Later Greek philosophers thought that a vacuum could exist outside the cosmos, but not inside it. The lack of free trade was considered by many as a principal cause of the depression, and World War II. Similarly, Aristotle considered the creation of a vacuum impossible—nothing could not be something. During this period, there was a great drop in trade and other economic indicators. He believed that all physical things were instantiations of an abstract Platonic ideal, and could not imagine an "ideal" form of a vacuum. The Great Depression was a major economic recession that ran from 1929 to 1941. Plato found the idea of a vacuum inconceivable. This became the policy in many countries attempting to industrialize and out-compete English exporters. Ancient Greek philosophers did not like to admit the existence of a vacuum, asking themselves "how can 'nothing' be something?". This was followed within a few years by the infant industry scenario developed by Mill anticipated New Trade Theory by promoting the theory that government had the "duty" to protect young industries, although only for a time necessary for them to develop full capacity. Historically, there has been much dispute over whether such a thing as a vacuum can exist. This was taken as evidence against the universal doctrine of free trade, as it was believed that more of the economic surplus of trade would accrue to a country following reciprocal, rather than completely free, trade policies. String theory is believed to be analogous to quantum field theory but one with a huge number of vacua - with the so-called anthropic landscape. Ricardo and others had suggested this earlier. If the theory is obtained by quantization of a classical theory, each stationary point of the energy in the configuration space gives rise to a single vacuum. John Stuart Mill proved that a country with monopoly pricing power on the international market could manipulate the terms of trade through maintaining tariffs, and that the response to this might be reciprocity in trade policy. In free (non-interacting) quantum field theories, this state is analogous to the ground state of a quantum harmonic oscillator. That is, the calculation made was whether it was in any particular country's self-interest to open its borders to imports. In quantum field theory and string theory, the term "vacuum" is used to represent the ground state in the Hilbert space, that is, the state with the lowest possible energy. The ascendancy of free trade was primarily based on national advantage in the mid 19th century. The best support for vacuum fluctuations is the Casimir effect. In Principles of Political Economy and Taxation Ricardo advanced the doctrine still considered the most counterintuitive in economics:. Vacuum fluctuations may also be related to the so-called cosmological constant in the theory of gravitation, if indeed this entity were to be observed in nature on a macroscopic scale. In 1817, David Ricardo, James Mill and Robert Torrens showed that free trade might benefit the industrially weak as well as the strong, in the famous theory of comparative advantage. While most agree that this represents a significant part of particle physics, it is a concept that would benefit from a deeper understanding than currently available. In 1799, the Dutch East India Company, formerly the world's largest company, became bankrupt, partly due to the rise of competitive free trade. This is called vacuum fluctuation. Smith said that he considered all rationalizations of import and export controls "dupery", which hurt the trading nation at the expense of specific industries. The lowest possible energy state is called the zero-point energy and consists of a seething mass of virtual particles that have brief existence. Since the division of labour was restricted by the size of the market, he said that countries having access to larger markets would be able to divide labour more efficiently and thereby become more productive. More fundamentally, quantum mechanics predicts that vacuum energy can never be exactly zero. It criticised Mercantilism, and argued that economic specialization could benefit nations just as much as firms. Even the space between molecules is not a perfect vacuum. In 1776, Adam Smith published the paper An Inquiry into the Nature and Causes of the Wealth of Nations. Each atom exists as a probability function of space, which has a certain non-zero value everywheres in a given volume. Trade in the East Indies was dominated by Portugal in the 16th century, the Netherlands in the 17th century, and the British in the 18th century. Another reason that perfect vacuum is impossible is the Heisenberg uncertainty principle which states that no particle can ever have an exact position. In the 16th century, Holland was the centre of free trade, imposing no exchange controls, and advocating the free movement of goods. If this soup of photons is in thermodynamic equilibrium with the walls, it can be said to have a particular temperature, as well as a pressure. Spices brought to Europe from distant lands were some of the most valuable commodities for their weight, sometimes rivaling gold. One reason is that the walls of a vacuum chamber emit light in the form of black-body radiation: visible light if they are at a temperature of thousands of degrees, infrared light if they are cooler. The spice trade was of major economic importance and helped spur the Age of Exploration. Even an ideal vacuum, thought of as the complete absence of anything, will not in practice remain empty. Vasco da Gama started the Spice trade in 1498. 1913, p.720). The Hanseatic League was an alliance of trading cities that maintained a trade monopoly over most of Northern Europe and the Baltic, between the 13th and 17th centuries. (See "Polar Magnetic Phenomena and Terrella Experiments", in The Norwegian Aurora Polaris Expedition 1902-1903 (publ. Vikings sailed to Western Europe, while Varangians to Russia. It does not seem unreasonable therefore to think that the greater part of the material masses in the universe is found, not in the solar systems or nebulae, but in "empty" space. From the 8th to the 11th century, the Vikings and Varangians traded as they sailed from and to Scandinavia. We have assumed that each stellar system in evolutions throws off electric corpuscles into space. For instance, Radhanites were a medieval guild or group (the precise meaning of the word is lost to history) of Jewish merchants who traded between the Christians in Europe and the Muslims of the Near East. He wrote: "It seems to be a natural consequence of our points of view to assume that the whole of space is filled with electrons and flying electric ions of all kinds. Nevertheless some trade did occur. In 1913, Norwegian explorer and physicist Kristian Birkeland may have been the first to predict that space is not only a plasma, but also contains "dark matter". The fall of the Roman empire, and the succeeding Dark Ages brought instability to Western Europe and a near collapse of the trade network. The deep vacuum of space could make it an attractive environment for certain processes, for instance those that require ultraclean surfaces. Their widespread empire produced a stable and secure transportation network that enabled the shipment of trade goods without fear of significant piracy. The idea of using this wind with a solar sail has been proposed for interplanetary travel. Roman commerce allowed their empire to flourish and endure. Spacecraft can be buffeted by solar winds, but planets are too massive to be affected. From the beginning of Greek civilization until the fall of the Roman empire in the 5th century, a financially lucrative trade brought valuable spice to Europe from the far east, including China. Beyond planetary atmospheres, the pressure from photons and other particles from the sun become significant. For this purpose they established trade colonies the Greeks called emporia. [2]. The Phoenicians were noted sea traders, travelling across the Mediterranean Sea, and as far north as Britain for sources of tin to manufacture bronze. Studies have discovered that some satellites retrieved from orbit are coated with a very thin layer of urine and fecal matter evidently released from Russian and US space missions. Long-range trade routes first appeared in the 3rd millennium BCE, when Sumerians in Mesopotamia traded with the Harappan civilization of the Indus Valley. The atmosphere in Low Earth Orbit is increasingly being polluted with man-made debris. Materials used for creating jewelry were traded with Egypt since 3000 BCE. Most Earth satellites operate in this region, and they need to fire their engines every few days to maintain orbit. There is evidence of the exchange of obsidian and flint during the stone age. In Low Earth Orbit (about 300 km altitude) the atmospheric density is still sufficient to produce significant drag on satellites. Trade is believed to have taken place throughout much of recorded human history. The density of gas decreases with distance from the object. Peter Watson dates the history of long-distance commerce from circa 150,000 years ago.[1]. Stars, planets and moons keep their atmosphere by gravitational attraction, so atmospheres have no firm boundary. Trading was the main facility of prehistoric people, who bartered goods and services from each other. Neither these photons nor the neutrinos produce a significant interaction with matter, so stars, planets and spacecraft move freely in this near perfect vacuum of interstellar space. Trade originated with the start of communication in prehistoric time. The current temperature is about 3 K, being merely 3 degrees above the absolute zero of temperature. . All of the observable universe is also filled with large numbers of photons, the so-called cosmic background radiation, and quite likely a correspondingly large number of neutrinos. As such, trade at market prices between locations benefits both locations. A perfect vacuum is an ideal state that cannot practically be obtained in a laboratory, nor even in outer space, where there are a few hydrogen atoms per cubic centimeter at 10−14 Pascal or 10−16 Torr. Trade exists between regions because different regions have a comparative advantage in the production of some tradable commodity, or because different regions' size allows for the benefits of mass production. The properties of the vacuum remain largely unknown. Due to specialization and division of labor, most people concentrate on a small aspect of production, trading for other products. It is cold and has no friction. Trade exists for many reasons. Much of outer space has the density and pressure of an almost perfect vacuum. Trade between two traders is called bilateral trade, while trade between more than two traders is called multilateral trade. The lowest pressures currently achievable in laboratory are about 10-13 Pa. The invention of money (and later credit, paper money and non-physical money) greatly simplified and promoted trade. Vessels lined with a highly gas-permeable material such as palladium (which is a high-capacity hydrogen sponge) create special outgassing problems. As a result, buying can be separated from selling, or earning. Your system may be able to evacuate nitrogen, (the main component of air,) to the desired vacuum, but your chamber could still be full of residual atmospheric hydrogen and helium. Modern traders instead generally negotiate through a medium of exchange, such as money. Smaller molecules can leak in more easily and are more easily absorbed by certain materials, and molecular pumps are less effective at pumping gases with lower molecular weights. The original form of trade was barter, the direct exchange of goods and services. The impact of molecular size must be considered. A mechanism that allows trade is called a market. The porosity of the metallic chamber walls may have to be considered, and the grain direction of the metallic flanges should be parallel to the flange face. Trade is also called commerce. Some oils and greases will boil off in extreme vacuums. Trade is the voluntary exchange of goods, services, or both. The water absorption of aluminium and palladium becomes an unacceptable source of outgassing, and even the absorptivity of hard metals such as stainless steel or titanium must be considered. As of mid-2005, there is a proposal for a Central American Free Trade Agreement, which would also include the United States and the Dominican Republic. In ultra-high vacuum systems, some very odd leakage paths and outgassing sources must be considered. January 1, 1995 World Trade Organization was created to facilitate free trade, by mandating mutual most favoured nation trading status between all signatories. Some systems are cooled well below room temperature by liquid nitrogen to shut down residual outgassing and simultaneously cryopump the system. 1994 The GATT Marrakech Agreement specified formation of the WTO. Once the bulk of the outgassing materials are boiled off and evacuated, the system may be cooled to lower vapour pressures and minimize residual outgassing during actual operation. January 1, 1994 NAFTA took effect. If necessary, this outgassing of the system can also be performed at room temperature, but this takes much more time. 1992 European Union lifted barriers to internal trade in goods and labour. The system is usually baked, preferably under vacuum, to temporarily raise the vapour pressure of all outgassing materials in the system and boil them off. Ultra-high vacuum systems are usually made of stainless steel with metal-gasketed conflat flanges. On a larger scale, the principles are the same as in a Cryomodule. Cryopumping incorporates the use of introducing cryogenics and a vacuum system. One such method to create a high vacuum to ultra high vacuum is by the use of cryopumps. Yet more specialized pumps become useful:. Even higher vacuums are possible, but they generally require custom-built equipment, strict operational procedures, and a fair amount of trial-and-error. With careful design and operation, 1μPa is possible. With these standard precautions, vacuums of 1 mPa are easily achieved with off-the-shelf molecular pumps. As a result, many materials that work well in low vacuums, such as epoxy, will become a problematic source of outgassing when attempting to achieve high vacuums. All materials, solid or liquid, have a small vapour pressure, and their outgassing becomes important when the vacuum pressure falls below this vapour pressure. The system must be clean and free of organic matter to minimize outgassing. High vacuum systems generally require metal chambers with metal O-ring seals such as Klein flanges or ISO flanges. As with mechanical pumps, the base pressure will be reached when leakage, outgassing, and backstreaming equal the pump speed, but now minimizing leakage and outgassing to a level comparable to backstreaming becomes much more difficult. Both of these pumps will stall and fail to pump if exhausted directly to atmospheric pressure, so they must be exhausted to a lower grade vacuum created by a mechanical pump. Diffusion pumps blow out molecules with jets of oil, while turbomolecular pumps use high speed fans. Both types of pumps blow out gas molecules that diffuse into the pump. The two main types of molecular pumps are the diffusion pump and the turbomolecular pump. In high vacuum, however, pressure gradients have little effect on fluid flows, and molecular pumps can attain their full potential. Since there is no seal, a small pressure at the exhaust can easily force flow backstream through the pump; this is called stall. They do this at the expense of the seal between the vacuum and their exhaust. Molecular pumps sweep out a larger area than mechanical pumps, and do so more frequently, making them capable of much higher pumping speeds as measured in volume per time. This regime is generally called high vacuum.. When the distance between the molecules increases, the molecules interact with the walls of the chamber more often than the other molecules, and molecular pumping becomes more effective than compression pumping. At atmospheric pressure and mild vacuums, molecules interact with each other and push on their neighboring molecules in what is known as viscous flow. Matter flows differently at different pressures based on the laws of fluid dynamics. Fortunately, once the pressure has dropped below 1 kPa or so, another vacuum pumping technique becomes possible. Better pumping technologies must be used to go beyond this barrier. Adding more pumps in parallel or bigger pumps of the same type can still improve the pump-down speed, but they will not reduce the base pressure below ultimate. In this situation, the vacuum will approach the pump's ultimate pressure - the best vacuum that this type of pump can achieve under ideal conditions. However, there is a point where backstream leakage through the pump and outgassing of the pump oils become the dominant mass flows into the chamber. If the dominant mass flow into the vacuum system is chamber leakage or outgassing of materials under vacuum, then the vacuum can be improved simply by installing bigger pumps with a higher volume flow rate. The base pressure of a rubber- and plastic-sealed piston pump system is typically 1 to 50 kPa, while a scroll pump might reach 10 Pa and a rotary vane oil pump with a clean and empty metallic chamber can easily achieve 0.1 Pa. Outgassing can be reduced by desiccation prior to vacuum pumping. When the pump's mass flow drops to the same level as the mass flows into the chamber, the system asymptotically approaches a constant pressure called the base pressure. Evaporation and sublimation into a vacuum is called outgassing, and the most common source is water absorbed by materials in the chamber. Meanwhile, the leakage rates, evaporation rates, and sublimation rates produce a constant mass flow into the system. So although the pumping speed remains constant when measured in litres/second, it drops exponentially when measured in kilograms/second. A mechanical vacuum pump moves the same volume of gas with each cycle, but as the chamber's pressure drops, this volume contains less and less mass. The pump's cavity is then sealed from the chamber, opened to the atmosphere, and squeezed back to a minute size. Because of the pressure differential, some air from the chamber is pushed into the pump's small cavity. Inside the pump, a mechanism expands a small sealed cavity to create a deep vacuum. This is the principle behind most mechanical vacuum pumps. By repeatedly closing off a compartment of the vacuum and exhausting it, it is possible to pump air out of a chamber of fixed size in a manner analogous to pumping a milkshake out of a glass. For example, your muscles expand your lungs to create a partial vacuum inside them, and air rushes in to fill the vacuum. The easiest way to create an artificial vacuum is to expand the volume of a container. Astrophysicists prefer to use density to describe these environments, in units of particles per cubic metre. In interplanetary and interstellar space, isotropic gas pressure is insignificant when compared to solar pressure, solar wind, and dynamic pressure. This vacuum state is called high vacuum, and the study of fluid flows in this regime is called particle gas dynamics. When the MFP is greater than the chamber, pump, spacecraft, or other objects present, the continuum assumptions of fluid mechanics do not apply. As gas pressure decreases, the mean free path (MFP) of the gas molecules increases. Here, 29.92 inHg means perfect vacuum. Thus a vacuum of 26 inHg is equivalent to a pressure of (29.92 - 26) or 3.92 inHg. This means that the pressure in vacuum, when specified in inches of mercury, is equal to the specified inches of mercury subtracted from 29.92. For commercial purposes, vacuum is often measured in inches of mercury (inHg). It is often also measured using the barometric scale, or as a percentage of atmospheric pressure in bars or atms. The SI unit of pressure is the pascal (abbreviation Pa), but vacuum is usually measured in millimeters of mercury (mmHg) or Torr, with 1 mmHg or 1 Torr equaling 133.3223684 pascals. Engineers measure the degree of vacuum in units of pressure. In engineering, a vacuum is any region where the gas pressure is less than atmospheric pressure. The antithesis of a vacuum, which is also an ideal unachievable state, is called a plenum. A complete characterization of the physical state would require further parameters, such as temperature. Physicists use the term partial vacuum to describe real-life non-ideal vacuum. In modern day usage vacuum is considered to exist in an enclosed space or chamber, when the pressure of gaseous environment is lower than atmospheric pressure (760 Torr or 101 kPa), or has been reduced as much as necessary to prevent the influence of some gas on a process being carried out in that space. A perfect vacuum is an ideal state that cannot practically be obtained in a laboratory, nor even in outer space where there are a few hydrogen atoms per cubic centimeter at 10−14 pascal or 10−16 torr. Vacuum ranges do not have universally agreed definitions and often depend on the size of the vacuum chamber, but a typical distribution is as follows:. . A perfect vacuum with a gaseous pressure of absolute zero is a philosophical concept with no physical reality; see sections below on Vacuum in Space and The Quantum Mechanical Vacuum. vacua) which means "empty," but space can never be perfectly empty. The root of the word vacuum is the Latin word vacuus (pl. For other uses, see vacuum cleaner, vacuum exercise and Vacuum (musical group).'. Converting them to solids by electrically combining them with other materials, called ion pumping. Converting the molecules of gas to their solid phase by freezing them, called cryopumping or cryotrapping. light bulb. vacuum tube. vacuum welding. process purging. ultra-clean inert storage. adhesive preparation. vacuum deposition as in semiconductor fabrication. thermal insulation as in a thermos. freeze drying. Interstellar space = approximately 1 fPa (10−17 Torr) [1]. Pressure on the Moon = approximately 1 nPa (10−11 Torr). Cryopumped MBE chamber = 100 nPa to 1 nPa (10−9 Torr to 10−11 Torr). Near earth outer space = approximately 100 µPa (10−6 Torr). Mechanical vacuum pump = approximately 100 Pa to 100 µPa (1 Torr to 10−6 Torr). Mechanical water-sealed liquid ring vacuum pump = approximately 3.2 kPa (24 Torr). Vacuum cleaner = approximately 80 kPa (600 Torr). Atmospheric pressure = variable, but standardised at 101.325 kPa (760 Torr) or 760 mm of mercury. |