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heat

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Dictionary: heat   (hēt) pronunciation
 
n. Physics.
    1. A form of energy associated with the motion of atoms or molecules and capable of being transmitted through solid and fluid media by conduction, through fluid media by convection, and through empty space by radiation.
    2. The transfer of energy from one body to another as a result of a difference in temperature or a change in phase.
  1. The sensation or perception of such energy as warmth or hotness.
  2. An abnormally high bodily temperature, as from a fever.
    1. The condition of being hot.
    2. A degree of warmth or hotness: The burner was on low heat.
    1. The warming of a room or building by a furnace or another source of energy: The house was cheap to rent, but the heat was expensive.
    2. A furnace or other source of warmth in a room or building: The heat was on when we returned from work.
  3. A hot season; a spell of hot weather.
    1. Intensity, as of passion, emotion, color, appearance, or effect.
    2. The most intense or active stage: the heat of battle.
    3. A burning sensation in the mouth produced by spicy flavoring in food.
  4. Estrus.
  5. One of a series of efforts or attempts.
    1. Sports & Games. One round of several in a competition, such as a race.
    2. A preliminary contest held to determine finalists.
  6. Informal. Pressure; stress.
  7. Slang.
    1. An intensification of police activity in pursuing criminals.
    2. The police. Used with the.
  8. Slang. Adverse comments or hostile criticism: Heat from the press forced the senator to resign.
  9. Slang. A firearm, especially a pistol.

v., heat·ed, heat·ing, heats.

v.tr.
  1. To make warm or hot.
  2. To excite the feelings of; inflame.
  3. To increase the molecular or kinetic energy of (an object).
v.intr.
  1. To become warm or hot.
  2. To become excited emotionally or intellectually.
phrasal verb:

heat up Informal.

  1. To become acute or intense: “If inflation heats up, interest rates could increase” (Christian Science Monitor).

[Middle English hete, from Old English hǣtu.]


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Concept

Heat is a form of energy—specifically, the energy that flows between two bodies because of differences in temperature. Therefore, the scientific definition of heat is different from, and more precise than, the everyday meaning. Physicists working in the area of thermodynamics study heat from a number of perspectives, including specific heat, or the amount of energy required to change the temperature of a substance, and calorimetry, the measurement of changes in heat as a result of physical or chemical changes. Thermodynamics helps us to understand such phenomena as the operation of engines and the gradual breakdown of complexity in physical systems—a phenomenon known as entropy.

How It Works

Heat, Work, and Energy

Thermodynamics is the study of the relationships between heat, work, and energy. Work is the exertion of force over a given distance to displace or move an object, and is, thus, the product of force and distance exerted in the same direction. Energy, the ability to accomplish work, appears in numerous manifestations—including thermal energy, or the energy associated with heat.

Thermal and other types of energy, including electromagnetic, sound, chemical, and nuclear energy, can be described in terms of two extremes: kinetic energy, or the energy associated with movement, and potential energy, or the energy associated with position. If a spring is pulled back to its maximum point of tension, its potential energy is also at a maximum; once it is released and begins springing through the air to return to its original position, it begins gaining kinetic energy and losing potential energy.

All manifestations of energy appear in both kinetic and potential forms, somewhat like the way football teams are organized to play both offense or defense. Just as a football team takes an offensive role when it has the ball, and a defensive role when the other team has it, a physical system typically undergoes regular transformations between kinetic and potential energy, and may have more of one or the other, depending on what is taking place in the system.

What Heat Is and Is Not

Thermal energy is actually a form of kinetic energy generated by the movement of particles at the atomic or molecular level: the greater the movement of these particles, the greater the thermal energy. Heat is internal thermal energy that flows from one body of matter to another—or, more specifically, from a system at a higher temperature to one at a lower temperature. Thus, temperature, like heat, requires a scientific definition quite different from its common meaning: temperature measures the average molecular kinetic energy of a system, and governs the direction of internal energy flow between them.

Two systems at the same temperature are said to be in a state of thermal equilibrium. When this occurs, there is no exchange of heat. Though in common usage, "heat" is an expression of relative warmth or coldness, in physical terms, heat exists only in transfer between two systems. What people really mean by "heat" is the internal energy of a system—energy that is a property of that system rather than a property of transferred internal energy.

No Such Thing As "cold."

Though the term "cold" has plenty of meaning in the everyday world, in physics terminology, it does not. Cold and heat are analogous to darkness and light: again, darkness means something in our daily experience, but in physical terms, darkness is simply the absence of light. To speak of cold or darkness as entities unto themselves is rather like saying, after spending 20 dollars, "I have 20 non-dollars in my pocket."

If you grasp a snowball in your hand, of course, your hand gets cold. The human mind perceives this as a transfer of cold from the snowball, but, in fact, exactly the opposite happens: heat moves from your hand to the snow, and if enough heat enters the snowball, it will melt. At the same time, the departure of heat from your hand results in a loss of internal energy near the surface of your hand, which you experience as a sensation of coldness.

Transfers of Heat

In holding the snowball, heat passes from the surface of the hand by one means, conduction, then passes through the snowball by another means, convection. In fact, there are three methods heat is transferred: conduction, involving successive molecular collisions and the transfer of heat between two bodies in contact; convection, which requires the motion of fluid from one place to another; or radiation, which takes place through electromagnetic waves and requires no physical medium, such as water or air, for the transfer.

Conduction

Solids, particularly metals, whose molecules are packed relatively close together, are the best materials for conduction. Molecules of liquid or nonmetallic solids vary in their ability to conduct heat, but gas is a poor conductor, because of the loose attractions between its molecules.

The qualities that make metallic solids good conductors of heat, as a matter of fact, also make them good conductors of electricity. In the conduction of heat, kinetic energy is passed from molecule to molecule, like a long line of people standing shoulder to shoulder, passing a secret. (And, just as the original phrasing of the secret becomes garbled, some kinetic energy is inevitably lost in the series of transfers.)

As for electrical conduction, which takes place in a field of electric potential, electrons are freed from their atoms; as a result, they are able to move along the line of molecules. Because plastic is much less conductive than metal, an electrician uses a screwdriver with a plastic handle; similarly, a metal cooking pan typically has a wooden or plastic handle.

Convection

Wherever fluids are involved—and in physics, "fluid" refers both to liquids and gases—convection is a common form of heat transfer. Convection involves the movement of heated material—whether it is air, water, or some other fluid.

Convection is of two types: natural convection and forced convection, in which a pump or other mechanism moves the heated fluid. When heated air rises, this is an example of natural convection. Hot air has a lower density than that of the cooler air in the atmosphere above it, and, therefore, is buoyant; as it rises, however, it loses energy and cools. This cooled air, now denser than the air around it, sinks again, creating a repeating cycle that generates wind.

Examples of forced convection include some types of ovens and even a refrigerator or air conditioner. These two machines both move warm air from an interior to an exterior place. Thus, the refrigerator pulls hot air from the compartment and expels it to the surrounding room, while an air conditioner pulls heat from a building and releases it to the outside.

But forced convection does not necessarily involve humanmade machines: the human heart is a pump, and blood carries excess heat generated by the body to the skin. The heat passes through the skin by means of conduction, and at the surface of the skin, it is removed from the body in a number of ways, primarily by the cooling evaporation of perspiration.

Radiation

Outer space, of course, is cold, yet the Sun's rays warm the Earth, an apparent paradox. Because there is no atmosphere in space, convection is impossible. In fact, heat from the Sun is not dependant on any fluid medium for its transfer: it comes to Earth by means of radiation. This is a form of heat transfer significantly different from the other two, because it involves electromagnetic energy, instead of ordinary thermal energy generated by the action of molecules. Heat from the Sun comes through a relatively narrow area of the light spectrum, including infrared, visible light, and ultraviolet rays.

Every form of matter emits electromagnetic waves, though their presence may not be readily perceived. Thus, when a metal rod is heated, it experiences conduction, but part of its heat is radiated, manifested by its glow—visible light. Even when the heat in an object is not visible, however, it may be radiating electromagnetic energy, for instance, in the form of infrared light. And, of course, different types of matter radiate better than others: in general, the better an object is at receiving radiation, the better it is at emitting it.

Measuring Heat

The measurement of temperature by degrees in the Fahrenheit or Celsius scales is a part of everyday life, but measurements of heat are not as familiar to the average person. Because heat is a form of energy, and energy is the ability to perform work, heat is, therefore, measured by the same units as work.

The principal unit of work or energy in the metric system (known within the scientific community as SI, or the SI system) is the joule. Abbreviated "J," a joule is equal to 1 newton-meter (N · m). The newton is the SI unit of force, and since work is equal to force multiplied by distance, measures of work can also be separated into these components. For instance, the British measure of work brings together a unit of distance, the foot, and a unit of force, the pound. A foot-pound (ft · lb) is equal to 1.356 J, and 1 joule is equal to 0.7376 ft · lb.

In the British system, Btu, or British thermal unit, is another measure of energy used for machines such as air conditioners. One Btu is equal to 778 ft · lb or 1,054 J. The kilocalorie in addition to the joule, is an important SI measure of heat. The amount of energy required to change the temperature of 1 gram of water by 1°C is called a calorie, and a kilocalorie is equal to 1,000 calories. Somewhat confusing is the fact that the dietary Calorie (capital C), with which most people are familiar, is not the same as a calorie (lowercase C)—rather, a dietary Calorie is the equivalent of a kilocalorie.

Real-Life Applications

Specific Heat

Specific heat is the amount of heat that must be added to, or removed from, a unit of mass for a given substance to change its temperature by 1°C. Thus, a kilocalorie, because it measures the amount of heat necessary to effect that change precisely for a kilogram of water, is identical to the specific heat for that particular substance in that particular unit of mass.

The higher the specific heat, the more resistant the substance is to changes in temperature. Many metals, in fact, have a low specific heat, making them easy to heat up and cool down. This contributes to the tendency of metals to expand when heated (a phenomenon also discussed in the Thermal Expansion essay), and, thus, to their malleability.

Measuring and Calculating Specific Heat

The specific heat of any object is a function of its mass, its composition, and the desired change in temperature. The values of the initial and final temperature are not important—only the difference between them, which is the temperature change.

The components of specific heat are related to one another in the formula Q = mcδT. Here Q is the quantity of heat, measured in joules, which must be added. The mass of the object is designated by m, and the specific heat of the particular substance in question is represented with c. The Greek letter delta (δ) designates change, and δT stands for "change in temperature."

Specific heat is measured in units of J/kg · °C (joules per kilogram-degree Centigrade), though for the sake of convenience, this is usually rendered in terms of kilojoules (kJ), or 1,000 joules—that is, kJ/kg · °C. The specific heat of water is easily derived from the value of a kilo-calorie: it is 4.185, the same number of joules required to equal a kilocalorie.

Calorimetry

The measurement of heat gain or loss as a result of physical or chemical change is called calorimetry (pronounced kal-IM-uh-tree). Like the word "calorie," the term is derived from a Latin root meaning "heat."

The foundations of calorimetry go back to the mid-nineteenth century, but the field owes much to scientists' work that took place over a period of about 75 years prior to that time. In 1780, French chemist Antoine Lavoisier (1743-1794) and French astronomer and mathematician Pierre Simon Laplace (1749-1827) had used a rudimentary ice calorimeter for measuring the heats in formations of compounds. Around the same time, Scottish chemist Joseph Black (1728-1799) became the first scientist to make a clear distinction between heat and temperature.

By the mid-1800s, a number of thinkers had come to the realization that—contrary to prevailing theories of the day—heat was a form of energy, not a type of material substance. Among these were American-British physicist Benjamin Thompson, Count Rumford (1753-1814) and English chemist James Joule (1818-1889)—for whom, of course, the joule is named.

Calorimetry as a scientific field of study actually had its beginnings with the work of French chemist Pierre-Eugene Marcelin Berthelot (1827-1907). During the mid-1860s, Berthelot became intrigued with the idea of measuring heat, and by 1880, he had constructed the first real calorimeter.

Calorimeters

Essential to calorimetry is the calorimeter, which can be any device for accurately measuring the temperature of a substance before and after a change occurs. A calorimeter can be as simple as a styrofoam cup. Its quality as an insulator, which makes styrofoam ideal for holding in the warmth of coffee and protecting the hand from scalding as well, also makes styrofoam an excellent material for calorimetric testing. With a styrofoam calorimeter, the temperature of the substance inside the cup is measured, a reaction is allowed to take place, and afterward, the temperature is measured a second time.

The most common type of calorimeter used is the bomb calorimeter, designed to measure the heat of combustion. Typically, a bomb calorimeter consists of a large container filled with water, into which is placed a smaller container, the combustion crucible. The crucible is made of metal, having thick walls with an opening through which oxygen can be introduced. In addition, the combustion crucible is designed to be connected to a source of electricity.

In conducting a calorimetric test using a bomb calorimeter, the substance or object to be studied is placed inside the combustion crucible and ignited. The resulting reaction usually occurs so quickly that it resembles the explosion of a bomb—hence, the name "bomb calorimeter." Once the "bomb" goes off, the resulting transfer of heat creates a temperature change in the water, which can be readily gauged with a thermometer.

To study heat changes at temperatures higher than the boiling point of water (212°F or 100°C), physicists use substances with higher boiling points. For experiments involving extremely large temperature ranges, an aneroid (without liquid) calorimeter may be used. In this case, the lining of the combustion crucible must be of a metal, such as copper, with a high coefficient or factor of thermal conductivity.

Heat Engines

The bomb calorimeter that Berthelot designed in 1880 measured the caloric value of fuels, and was applied to determining the thermal efficiency of a heat engine. A heat engine is a machine that absorbs heat at a high temperature, performs mechanical work, and as a result, gives off heat at a lower temperature.

The desire to create efficient heat engines spurred scientists to a greater understanding of thermodynamics, and this resulted in the laws of thermodynamics, discussed at the conclusion of this essay. Their efforts were intimately connected with one of the greatest heat engines ever created, a machine that literally powered the industrialized world during the nineteenth century: the steam engine.

How a Steam Engine Works

Like all heat engines (except reverse heat engines such as the refrigerator, discussed below), a steam engine pulls heat from a high-temperature reservoir to a low-temperature reservoir, and in the process, work is accomplished. The hot steam from the high-temperature reservoir makes possible the accomplishment of work, and when the energy is extracted from the steam, the steam condenses in the low-temperature reservoir, becoming relatively cool water.

A steam engine is an external-combustion engine, as opposed to the internal-combustion engine that took its place at the forefront of industrial technology at the beginning of the twentieth century. Unlike an internal-combustion engine, a steam engine burns its fuel outside the engine. That fuel may be simply firewood, which is used to heat water and create steam. The thermal energy of the steam is then used to power a piston moving inside a cylinder, thus, converting thermal energy to mechanical energy for purposes such as moving a train.

Evolution of Steam Power

As with a number of advanced concepts in science and technology, the historical roots of the steam engine can be traced to the Greeks, who—just as they did with ideas such as the atom or the Sun-centered model of the universe—thought about it, but failed to develop it. The great inventor Hero of Alexandria (c. 65-125) actually created several steam-powered devices, but he perceived these as mere novelties, hardly worthy of scientific attention. Though Europeans adopted water power, as, for instance, in waterwheels, during the late ancient and medieval periods, further progress in steam power did not occur for some 1,500 years.

Following the work of French physicist Denis Papin (1647-1712), who invented the pressure cooker and conducted the first experiments with the use of steam to move a piston, English engineer Thomas Savery (c. 1650-1715) built the first steam engine. Savery had abandoned the use of the piston in his machine, but another English engineer, Thomas Newcomen (1663-1729), reintroduced the piston for his own steam-engine design.

Then in 1763, a young Scottish engineer named James Watt (1736-1819) was repairing a Newcomen engine and became convinced he could build a more efficient model. His steam engine, introduced in 1769, kept the heating and cooling processes separate, eliminating the need for the engine to pause in order to reheat. These and other innovations that followed—including the introduction of a high-pressure steam engine by English inventor Richard Trevithick (1771-1833)—transformed the world.

Carnot Provides Theoretical Understanding

The men who developed the steam engine were mostly practical-minded figures who wanted only to build a better machine; they were not particularly concerned with the theoretical explanation for its workings. Then in 1824, a French physicist and engineer by the name of Sadi Carnot (1796-1832) published his sole work, the highly influential Reflections on the Motive Power of Fire (1824), in which he discussed heat engines scientifically.

In Reflections, Carnot offered the first definition of work in terms of physics, describing it as "weight lifted through a height." Analyzing Watt's steam engine, he also conducted groundbreaking studies in the nascent science of thermodynamics. Every heat engine, he explained, has a theoretical limit of efficiency related to the temperature difference in the engine: the greater the difference between the lowest and highest temperature, the more efficient the engine.

Carnot's work influenced the development of more efficient steam engines, and also had an impact on the studies of other physicists investigating the relationship between work, heat, and energy. Among these was William Thomson, Lord Kelvin (1824-1907). In addition to coining the term "thermodynamics," Kelvin developed the Kelvin scale of absolute temperature and established the value of absolute zero, equal to −273.15°C or −459.67°F.

According to Carnot's theory, maximum effectiveness was achieved by a machine that could reach absolute zero. However, later developments in the understanding of thermodynamics, as discussed below, proved that both maximum efficiency and absolute zero are impossible to attain.

Reverse Heat Engines

It is easy to understand that a steam engine is a heat engine: after all, it produces heat. But how is it that a refrigerator, an air conditioner, and other cooling machines are also heat engines? Moreover, given the fact that cold is the absence of heat and heat is energy, one might ask how a refrigerator or air conditioner can possibly use energy to produce cold, which is the same as the absence of energy. In fact, cooling machines simply reverse the usual process by which heat engines operate, and for this reason, they are called "reverse heat engines." Furthermore, they use energy to extract heat.

A steam engine takes heat from a high-temperature reservoir—the place where the water is turned into steam—and uses that energy to produce work. In the process, energy is lost and the heat moves to a low-temperature reservoir, where it condenses to form relatively cool water. A refrigerator, on the other hand, pulls heat from a low-temperature reservoir called the evaporator, into which flows heat from the refrigerated compartment—the place where food and other perishables are kept. The coolant from the evaporator take this heat to the condenser, a high-temperature reservoir at the back of the refrigerator, and in the process it becomes a gas. Heat is released into the surrounding air; this is why the back of a refrigerator is hot.

Instead of producing a work output, as a steam engine does, a refrigerator requires a work input—the energy supplied via the wall outlet. The principles of thermodynamics show that heat always flows from a high-temperature to a low-temperature reservoir, and reverse heat engines do not defy these laws. Rather, they require an external power source in order to effect the transfer of heat from a low-temperature reservoir, through the gases in the evaporator, to a high-temperature reservoir.

The Laws of Thermodynamics

The First Law of Thermodynamics

There are three laws of thermodynamics, which provide parameters as to the operation of thermal systems in general, and heat engines in particular. The history behind the derivation of these laws is discussed in the essay on Thermodynamics; here, the laws themselves will be examined in brief form.

The physical law known as conservation of energy shows that within a system isolated from all outside factors, the total amount of energy remains the same, though transformations of energy from one form to another take place. The first law of thermodynamics states the same fact in a somewhat different manner.

According to the first law of thermodynamics, because the amount of energy in a system remains constant, it is impossible to perform work that results in an energy output greater than the energy input. Thus, it could be said that the conservation of energy law shows that "the glass is half full": energy is never lost. On the hand, the first law of thermodynamics shows that "the glass is half empty": no machine can ever produce more energy than was put into it. Hence, a perpetual motion machine is impossible, because in order to keep a machine running continually, there must be a continual input of energy.

The Second Law of Thermodynamics

The second law of thermodynamics begins from the fact that the natural flow of heat is always from a high-temperature to a low-temperature reservoir. As a result, no engine can be constructed that simply takes heat from a source and performs an equivalent amount of work: some of the heat will always be lost. In other words, it is impossible to build a perfectly efficient engine.

In effect, the second law of thermodynamics compounds the "bad news" delivered by the first law with some even worse news: though it is true that energy is never lost, the energy available for work output will never be as great as the energy put into a system. Linked to the second law is the concept of entropy, the tendency of natural systems toward breakdown, and specifically, the tendency for the energy in a system to be dissipated. "Dissipated" in this context means that the high-and low-temperature reservoirs approach equal temperatures, and as this occurs, entropy increases.

The Third Law of Thermodynamics

Entropy also plays a part in the third law of thermodynamics, which states that at the temperature of absolute zero, entropy also approaches zero. This might seem to counteract the "worse news" of the second law, but in fact, what the third law shows is that absolute zero is impossible to reach.

As stated earlier, Carnot's engine would achieve perfect efficiency if its lowest temperature were the same as absolute zero; but the second law of thermodynamics shows that a perfectly efficient machine is impossible. Relativity theory (which first appeared in 1905, the same year as the third law of thermodynamics) showed that matter can never exceed the speed of light. In the same way, the collective effect of the second and third laws is to prove that absolute zero—the temperature at which molecular motion in all forms of matter theoretically ceases—can never be reached.

Where to Learn More

Beiser, Arthur. Physics, 5th ed. Reading, MA: Addison-Wesley, 1991.

Bonnet, Robert L and Dan Keen. Science Fair Projects: Physics. Illustrated by Frances Zweifel. New York: Sterling, 1999.

Encyclopedia of Thermodynamics (Web site). <http://therion.minpet.unibas.ch/minpet/groups/thermodict/> (April 12, 2001).

Friedhoffer, Robert. Physics Lab in the Home. Illustrated by Joe Hosking. New York: Franklin Watts, 1997.

Manning, Mick and Brita Granström. Science School. New York: Kingfisher, 1998.

Macaulay, David. The New Way Things Work. Boston: Houghton Mifflin, 1998.

Moran, Jeffrey B. How Do We Know the Laws of Thermodynamics? New York: Rosen Publishing Group, 2001.

Santrey, Laurence. Heat. Illustrated by Lloyd Birmingham. Mahwah, NJ: Troll Associates, 1985.

Suplee, Curt. Everyday Science Explained. Washington, D.C.: National Geographic Society, 1996.

"Temperature and Thermodynamics" PhysLINK.com (Web site). <http://www.physlink.com/ae_thermo.cfm> (April 12, 2001).


 

For the purposes of thermodynamics, it is convenient to define all energy while in transit, but unassociated with matter, as either heat or work. Heat is that form of energy in transit due to a temperature difference between the source from which the energy is coming and the sink toward which the energy is going. The energy is not called heat before it starts to flow or after it has ceased to flow. A hot object does contain energy, but calling this energy heat as it resides in the hot object can lead to widespread confusion. See also Energy; Internal energy.


 
Investment Dictionary: Heath-Jarrow-Morton Model - HJM Model
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A model that applies forward rates to an existing term structure of interest rates to determine appropriate prices for securities that are sensitive to changes in interest rates.

Investopedia Says:
The HJM model is very theoretical and is used at the most advanced levels of financial analysis. It is used mainly by arbitrageurs seeking arbitrage opportunities.

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Thesaurus: heat
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noun

  1. Intense warmth: fervor, hotness, torridity, torridness. See hot/cold/lukewarm.
  2. Intensity of feeling or reaction: excitation, excitement, warmth. See excite/bore/interest, feelings, hot/cold/lukewarm.
  3. A regular period of sexual excitement in female mammals: estrus, rut2, season. See sex/asexual.
  4. A member of a law-enforcement agency: bluecoat, finest, officer, patrolman, patrolwoman, peace officer, police, policeman, police officer, policewoman. Informal cop, law. Slang bull1, copper, flatfoot, fuzz, gendarme, man (often uppercase). Chiefly British bobby, constable, peeler. See law.

 
Antonyms: heat
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n

Definition: anger, passion
Antonyms: apathy, coolness, disinterest, frigidity

n

Definition: warmth
Antonyms: cold, cool, coolness

v

Definition: make or become hot
Antonyms: cool, freeze


 

n

The state of a body or of matter that is perceived as being opposite of cold and is characterized by elevation of temperature.

 

Energy transferred from one body to another as the result of a difference in temperature. Heat flows from a hotter body to a colder body when the two bodies are brought together. This transfer of energy usually results in an increase in the temperature of the colder body and a decrease in that of the hotter body. A substance may absorb heat without an increase in temperature as it changes from one phase to another — that is, when it melts or boils. The distinction between heat (a form of energy) and temperature (a measure of the amount of energy) was clarified in the 19th century by such scientists as J.-B. Fourier, Gustav Kirchhoff, and Ludwig Boltzmann.

For more information on heat, visit Britannica.com.

 
Architecture: heat
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The form of energy that is transferred by virtue of a temperature difference between two bodies, the transfer being from the warmer to the cooler body.


 

Energy possessed by a substance in the form of atomic or molecular kinetic energy. Heat contained within a body is the product of the body's mass, temperature, and specific heat capacity. Heat is transmitted by radiation, conduction, and convection. Changes in the heat content of a body may result in changes of state of matter within the body (e.g. liquid water converted to vapour; see latent heat of vaporization) or changes of temperature. The SI unit for heat is the joule.

 
heat, nonmechanical energy in transit, associated with differences in temperature between a system and its surroundings or between parts of the same system.

Measures of Heat

Temperature is a measure of the average translational kinetic energy of the molecules of a system. Heat is commonly expressed in either of two units: the calorie, an older metric unit, and the British thermal unit (Btu), an English unit commonly used in the United States. Scientists express heat in terms of the joule, a unit used for all forms of energy.

Specific Heat

As heat is added to a substance in the solid state, the molecules of the substance gain kinetic energy and the temperature of the substance rises. The amount of heat needed to raise a unit of mass of the substance one degree of temperature is called the specific heat of the substance. Because of the way in which the calorie and the Btu are defined, the specific heat of any substance is the same in either system of measurement. For example, the specific heat of water is 1 calorie per gram per degree Celsius; i.e., 1 calorie of heat is needed to raise the temperature of 1 gram of water by 1 degree Celsius; it is also 1 Btu per pound per degree Fahrenheit.

Heat of Fusion

When a solid reaches a certain temperature, it changes to a liquid. This temperature is a particular property of the substance and is called its melting point. While the solid-liquid transition is taking place, there is no change in temperature. All of the heat being added is being converted to the internal potential energy associated with the liquid state. The amount of heat needed to convert one unit of mass of a substance from a solid to liquid is called the heat of fusion, or latent heat of fusion, of the substance. Like specific heat, latent heat is also a property of the particular substance. The latent heat of fusion for the ice-to-water transition is 80 calories per gram.

Heat of Vaporization

After a substance is completely changed from a solid to a liquid, further addition of heat again causes the temperature to rise until it reaches the boiling point, the particular temperature at which the given substance changes from a liquid to a gas. During the liquid-gas transition, the temperature remains constant until the change is completed. The heat of vaporization, or latent heat of vaporization, is the heat that must be added to convert one unit of mass of the substance from a liquid to a gas.

Transfer of Heat

Heat may be transferred from one substance to another by three means—conduction, convection, and radiation. Conduction involves the transfer of energy from one molecule to adjacent molecules without the substance as a whole moving. Convection involves the movement of warmer parts of a substance away from the source of heat and takes place only in fluids, i.e., liquids and gases. Radiation is the transfer of heat energy in the form of electromagnetic radiation, principally in the infrared radiation portion of the spectrum.

Study and Analysis of Heat

The study of heat and its relationship to useful work is called thermodynamics and involves macroscopic quantities such as pressure, temperature, and volume without regard for the molecular basis of these quantities. Low-temperature physics is concerned with phenomena that occur at extremely low temperatures. The analysis of heat on the basis of the structure of matter is considered in the kinetic-molecular theory of gases and provides an explanation for the various gas laws. The gas laws in turn serve to define an absolute temperature scale based on theoretical considerations (see Kelvin temperature scale).

Bibliography

See M. C. Mott-Smith, Heat and Its Workings (1933, repr. 1962); R. Becker, Theory of Heat (tr. 1967).


 

In physics, a form of energy associated with the movement of atoms and molecules in any material. The higher the temperature of a material, the faster the atoms are moving, and hence the greater the amount of energy present as heat. (See infrared radiation.)

 
Essay: The nature of heat
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In Aristotle's physics, heat is one of the active qualities of a body. Hotness, as well as dryness, and their opposites, coldness and moistness, were the qualities that defined an element. Later, heat and temperature came to be viewed as lesser fundamental properties of matter, but opinions about the nature of heat varied sharply. Francis Bacon defined heat as local motion, and René Descartes and Robert Hooke described heat as the ceaseless motion of particles. Others, such as the Dutch physician Hermann Boerhaave, described heat as a subtle fluid, later called caloric, that could pass from one object to another.

During the beginning of the 19th century, the theory that heat was a form of motion won over the liquid, or caloric, theory. Even earlier, at the end of the 18th century, Count Rumford (Benjamin Thompson) had observed the large amount of heat produced during the boring of cannons and reached the conclusion that heat was added to the cannon by motion.

The German physician Julius Robert Mayer was one of the first to relate heat directly to mechanical work, writing of his discovery in 1842. That heat and mechanical work are both forms of energy was a very important discovery. It became the basis of a new science that gained quickly in importance during the 19th century: thermodynamics.

Sadi Carnot, intrigued by why British steam engines were more efficient than French ones, started investigating the physical processes that take place in a steam engine. Although he believed that heat was an indestructible fluid, he was the first to apply physics to a technical problem. He published the results in 1824 as Réflexions sur la puissance motrice du feu ("reflections on the motive power of fire"). However, this paper remained little known for ten years, until Emile Clapeyron discussed it in the Journal de l'Ecole Polytechnique

Carnot had found that the efficiency of a machine depends on the difference in temperature between the heat source that supplies the work (hot reservoir) to the machine and the temperature reservoir into which the machine discharges excess heat (cold reservoir). The mechanical equivalent of heat is the amount of heat that can produce a given amount of motion. Although Carnot had found an approximate value for the mechanical equivalent of heat, he died too early, at the age of 36, to publish this result.

Contrary to Carnot, James Prescott Joule believed that heat was a quantity that was destroyed in a machine to produce mechanical work. In a series of famous experiments, he measured the increase of temperature of water stirred by a determined amount of mechanical work. As a result, Joule also determined the mechanical equivalent of heat, five years after the similar work of Julius Mayer. His work was more quickly recognized than Mayer's, however, since Joule was a physicist and Mayer a physician.

 
A cynical view of the world by Ambrose Bierce


n.

    Heat, says Professor Tyndall, is a mode
        Of motion, but I know now how he's proving
    His point; but this I know -- hot words bestowed
        With skill will set the human fist a-moving,
    And where it stops the stars burn free and wild.
    Crede expertum -- I have seen them, child.
                                                          Gorton Swope


 
Word Tutor: heat
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pronunciation

IN BRIEF: Warmth.

pronunciation If you can't stand the heat, get out of the kitchen. — Harry Truman (1884-1972)

 
Wikipedia: Heat
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A related term is thermal energy, loosely defined as the energy of a body that increases with its temperature. Heat is also loosely referred to as thermal energy, although many definitions require this thermal energy to actually be in the process of movement between one body and another to be technically called heat (otherwise, many sources prefer to continue to refer to the static quantity as "thermal energy"). Heat is also known as "Energy".

Energy transfer by heat can occur between objects by radiation, conduction and convection. Temperature is used as a measure of the internal energy or enthalpy, that is the level of elementary motion giving rise to heat transfer. Energy can only be transferred by heat between objects - or areas within an object - with different temperatures (as given by the zeroth law of thermodynamics). This transfer happens spontaneously only in the direction of the colder body (as per the second law of thermodynamics). The transfer of energy by heat from one object to another object with an equal or higher temperature can happen only with the aid of a heat pump, which does work.

Contents

Overview

The first law of thermodynamics states that the energy of a closed system is conserved. Therefore, to change the energy of a system, energy must be transferred to or from the system. Heat and work are the only two mechanisms by which energy can be transferred to or from a control mass. Heat is the transfer of energy caused by the temperature difference. The unit for the amount of energy transferred by heat in the International System of Units SI is the joule (J), though the British Thermal Unit and the calorie are still used in the United States. The unit for the rate of heat transfer is the watt (W = J/s).

Heat Q can flow across the boundary of the system and thus change its internal energy U.

Heat transfer is a path function (process quantity), as opposed to a point function (state quantity). Heat flows between systems that are not in thermal equilibrium with each other; it spontaneously flows from the areas of high temperature to areas of low temperature. When two bodies of different temperature come into thermal contact, they will exchange internal energy until their temperatures are equalized; that is, until they reach thermal equilibrium. The adjective hot is used as a relative term to compare the object’s temperature to that of the surroundings (or that of the person using the term). The term heat is used to describe the flow of energy. In the absence of work interactions, the heat that is transferred to an object ends up getting stored in the object in the form of internal energy.

A red-hot iron rod from which heat transfer to the surrounding environment will be primarily through radiation.

Specific heat is defined as the amount of energy that has to be transferred to or from one unit of mass or mole of a substance to change its temperature by one degree. Specific heat is a property, which means that it depends on the substance under consideration and its state as specified by its properties. Fuels, when burned, release much of the energy in the chemical bonds of their molecules. Upon changing from one phase to another, a pure substance releases or absorbs heat without its temperature changing. The amount of heat transfer during a phase change is known as latent heat and depends primarily on the substance and its state.

Thermal energy

Thermal energy is a term often confused with that of heat. Loosely speaking, when heat is added to a thermodynamic system its thermal energy increases and when heat is withdrawn its thermal energy decreases. In this point of view, objects that are hot are referred to as being in possession of a large amount of thermal energy, whereas cold objects possess little thermal energy. Thermal energy then is often mistakenly defined as being synonym for the word heat. This, however, is not the case: an object cannot possess heat, but only energy. The term "thermal energy" when used in conversation is often not used in a strictly correct sense, but is more likely to be only used as a descriptive word. In physics and thermodynamics, the words “heat”, “internal energy”, “work”, "enthalpy" (heat content), "entropy", "external forces", etc., which can be defined exactly, i.e. without recourse to internal atomic motions and vibrations, tend to be preferred and used more often than the term "thermal energy", which is difficult to define.

History

In the history of science, the history of heat traces its origins from the first hominids to make fire and to speculate on its operation and meaning to modern day particle physicists who study the sub-atomic nature of heat. In short, the phenomenon of heat and its definition evolved from mythological theories of fire, to heat, to terra pinguis, phlogiston, to fire air, to caloric, to the theory of heat, to the mechanical equivalent of heat, to thermo-dynamics (sometimes called energetics) to thermodynamics. Most of the history of heat, then, is a precursor to the history of thermodynamics.

Notation

The total amount of energy transferred through heat transfer is conventionally abbreviated as Q. The conventional sign convention is that when a body releases heat into its surroundings, Q < 0 (-); when a body absorbs heat from its surroundings, Q > 0 (+). Heat transfer rate, or heat flow per unit time, is denoted by:

\dot{Q} = {dQ\over dt} \,\!.

It is measured in watts. Heat flux is defined as rate of heat transfer per unit cross-sectional area, and is denoted q, resulting in units of watts per square metre, though slightly different notation conventions can be used.

Entropy

In 1854, German physicist Rudolf Clausius defined the second fundamental theorem (the second law of thermodynamics) in the mechanical theory of heat (thermodynamics): "if two transformations which, without necessitating any other permanent change, can mutually replace one another, be called equivalent, then the generations of the quantity of heat Q from work at the temperature T, has the equivalence-value:"[1][2]

 {} \frac {Q}{T}

In 1865, he came to define this ratio as entropy symbolized by S, such that, for a closed, stationary system:

 \Delta S = \frac {Q}{T}

and thus, by reduction, quantities of heat δQ (an inexact differential) are defined as quantities of TdS (an exact differential):

 \delta Q = T dS \,

In other words, the entropy function S facilitates the quantification and measurement of heat flow through a thermodynamic boundary.

Definitions

In modern terms, heat is concisely defined as energy in transit. Scottish physicist James Clerk Maxwell, in his 1871 classic Theory of Heat, was one of the first to enunciate a modern definition of “heat”. In short, Maxwell outlined four stipulations on the definition of heat. One, it is “something which may be transferred from one body to another”, as per the second law of thermodynamics. Two, it can be spoken of as a “measurable quantity”, and thus treated mathematically like other measurable quantities. Three, it “can not be treated as a substance”; for it may be transformed into something which is not a substance, e.g. mechanical work. Lastly, it is “one of the forms of energy”. Similar such modern, succinct definitions of heat are as follows:

  • In a thermodynamic sense, heat is never regarded as being stored within a body. Like work, it exists only as energy in transit from one body to another; in thermodynamic terminology, between a system and its surroundings. When energy in the form of heat is added to a system, it is stored not as heat, but as kinetic and potential energy of the atoms and molecules making up the system.[3]
  • The noun heat is defined only during the process of energy transfer by conduction or radiation.[4]
  • Heat is defined as any spontaneous flow of energy from one object to another, caused by a difference in temperature between the objects.[5]
  • Heat may be defined as energy in transit from a high-temperature object to a lower-temperature object.[6]
  • Heat as an interaction between two closed systems without exchange of work is a pure heat interaction when the two systems, initially isolated and in a stable equilibrium, are placed in contact. The energy exchanged between the two systems is then called heat.[7]
  • Heat is a form of energy possessed by a substance by virtue of the vibrational movement, i.e. kinetic energy, of its molecules or atoms.[8] The kinetic energy and heat may formally be equivalent, but they are not identical.
  • Heat is the transfer of energy between substances of different temperatures.

Thermodynamics

Internal energy

Heat is related to the internal energy U of the system and work W done by the system by the first law of thermodynamics:

\Delta U = Q + W \

which means that the energy of the system can change either via work or via heat flows across the boundary of the thermodynamic system. In more detail, Internal energy is the sum of all microscopic forms of energy of a system. It is related to the molecular structure and the degree of molecular activity and may be viewed as the sum of kinetic and potential energies of the molecules; it comprises the following types of energies:[9]

Type Composition of Internal Energy (U)
Sensible energy the portion of the internal energy of a system associated with kinetic energies (molecular translation, rotation, and vibration; electron translation and spin; and nuclear spin) of the molecules.
Latent energy the internal energy associated with the phase of a system.
Chemical energy the internal energy associated with the atomic bonds in a molecule.
Nuclear energy the tremendous amount of energy associated with the strong bonds within the nucleus of the atom itself.
Energy interactions those types of energies not stored in the system (e.g. heat transfer, mass transfer, and work), but which are recognized at the system boundary as they cross it, which represent gains or losses by a system during a process.
Thermal energy the sum of sensible and latent forms of internal energy.

The transfer of heat to an ideal gas at constant pressure increases the internal energy and performs boundary work (i.e. allows a control volume of gas to become larger or smaller), provided the volume is not constrained. Returning to the first law equation and separating the work term into two types, "boundary work" and "other" (e.g. shaft work performed by a compressor fan), yields the following:

\Delta U + W_{boundary} = Q + W_{other}\

This combined quantity ΔU + Wboundary is enthalpy, H, one of the thermodynamic potentials. Both enthalpy, H, and internal energy, U are state functions. State functions return to their initial values upon completion of each cycle in cyclic processes such as that of a heat engine. In contrast, neither Q nor W are properties of a system and need not sum to zero over the steps of a cycle. The infinitesimal expression for heat, δQ, forms an inexact differential for processes involving work. However, for processes involving no change in volume, applied magnetic field, or other external parameters, δQ, forms an exact differential. Likewise, for adiabatic processes (no heat transfer), the expression for work forms an exact differential, but for processes involving transfer of heat it forms an inexact differential.

Heat capacity

For a simple compressible system such as an ideal gas inside a piston, the changes in enthalpy and internal energy can be related to the heat capacity at constant pressure and volume, respectively. Constrained to have constant volume, the heat, Q, required to change its temperature from an initial temperature, T0, to a final temperature, Tf is given by:

Q = \int_{T_0}^{T_f}C_v\,dT = \Delta U\,\!

Removing the volume constraint and allowing the system to expand or contract at constant pressure:

Q = \ \Delta U + \int_{V_0}^{V_f}P\,dV = \ \Delta H = \int_{T_0}^{T_f}C_p\,dT \,\!

For incompressible substances, such as solids and liquids, the distinction between the two types of heat capacity disappears, as no work is performed. Heat capacity is an extensive quantity and as such is dependent on the number of molecules in the system. It can be represented as the product of mass, m , and specific heat capacity, c_s \,\! according to:

C_p = mc_s \,\!

or is dependent on the number of moles and the molar heat capacity, c_n \,\! according to:

C_p = nc_n \,\!

The molar and specific heat capacities are dependent upon the internal degrees of freedom of the system and not on any external properties such as volume and number of molecules.

The specific heats of monatomic gases (e.g., helium) are nearly constant with temperature. Diatomic gases such as hydrogen display some temperature dependence, and triatomic gases (e.g., carbon dioxide) still more.

In liquids at sufficiently low temperatures, quantum effects become significant. An example is the behavior of bosons such as helium-4. For such substances, the behavior of heat capacity with temperature is discontinuous at the Bose-Einstein condensation point.

The quantum behavior of solids is adequately characterized by the Debye model. At temperatures well below the characteristic Debye temperature of a solid lattice, its specific heat will be proportional to the cube of absolute temperature. For low-temperature metals, a second term is needed to account for the behavior of the conduction electrons, an example of Fermi-Dirac statistics.

Phase Changes

The boiling point of water, at sea level and normal atmospheric pressure and temperature, will always be at nearly 100 °C, no matter how much heat is added. The extra heat changes the phase of the water from liquid into water vapor. The heat added to change the phase of a substance in this way is said to be "hidden" and thus it is called latent heat (from the Latin latere meaning "to lie hidden"). Latent heat is the heat per unit mass necessary to change the state of a given substance, or:

L = \frac{Q}{\Delta m} \,\!

and

Q = \int_{M_0}^{M} L\,dm.

Note that, as pressure increases, the L rises slightly. Here, Mo is the amount of mass initially in the new phase, and M is the amount of mass that ends up in the new phase. Also, L generally does not depend on the amount of mass that changes phase, so the equation can normally be written:

Q = LΔm.

Sometimes L can be time-dependent if pressure and volume are changing with time, so that the integral can be written as:

Q = \int L\frac{dm}{dt}dt.

Heat transfer mechanisms

Heat tends to move from a high-temperature region to a low-temperature region. This heat transfer may occur by the mechanisms of conduction and radiation. In engineering, the term convective heat transfer is used to describe the combined effects of conduction and fluid flow and is regarded as a third mechanism of heat transfer.

Conduction

Conduction is the most significant means of heat transfer in a solid. On a microscopic scale, conduction occurs as hot, rapidly moving or vibrating atoms and molecules interact with neighboring atoms and molecules, transferring some of their energy (heat) to these neighboring atoms. In insulators the heat flux is carried almost entirely by phonon vibrations.

Fire test used to test the heat transfer through firestops and penetrants used in construction listing and approval use and compliance.

The "electron fluid" of a conductive metallic solid conducts nearly all of the heat flux through the solid. Phonon flux is still present, but carries less than 1% of the energy. Electrons also conduct electric current through conductive solids, and the thermal and electrical conductivities of most metals have about the same ratio. A good electrical conductor, such as copper, usually also conducts heat well. The Peltier-Seebeck effect exhibits the propensity of electrons to conduct heat through an electrically conductive solid. Thermoelectricity is caused by the relationship between electrons, heat fluxes and electrical currents.

Convection

Convection is usually the dominant form of heat transfer in liquids and gases. This is a term used to characterise the combined effects of conduction and fluid flow. In convection, enthalpy transfer occurs by the movement of hot or cold portions of the fluid together with heat transfer by conduction. Commonly an increase in temperature produces a reduction in density. Hence, when water is heated on a stove, hot water from the bottom of the pan rises, displacing the colder denser liquid which falls. Mixing and conduction result eventually in a nearly homogeneous density and even temperature. Two types of convection are commonly distinguished, free convection, in which gravity and buoyancy forces drive the fluid movement, and forced convection, where a fan, stirrer, or other means is used to move the fluid. Buoyant convection is due to the effects of gravity, and hence does not occur in microgravity environments.

Radiation

Radiation is the only form of heat transfer that can occur in the absence of any form of medium (i.e., through a vacuum). Thermal radiation is a direct result of the movements of atoms and molecules in a material. Since these atoms and molecules are composed of charged particles (protons and electrons), their movements result in the emission of electromagnetic radiation, which carries energy away from the surface. At the same time, the surface is constantly bombarded by radiation from the surroundings, resulting in the transfer of energy to the surface. Since the amount of emitted radiation increases with increasing temperature, a net transfer of energy from higher temperatures to lower temperatures results.

The power that a black body emits at various frequencies is described by Planck's law. For any given temperature, there is a frequency fmax at which the power emitted is a maximum. Wien's displacement law, and the fact that the frequency of light is inversely proportional to its wavelength in vacuum, mean that the peak frequency fmax is proportional to the absolute temperature T of the black body. The photosphere of the Sun, at a temperature of approximately 6000 K, emits radiation principally in the visible portion of the spectrum. The Earth's atmosphere is partly transparent to visible light, and the light reaching the Earth's surface is absorbed or reflected. The Earth's surface emits the absorbed radiation, approximating the behavior of a black body at 300 K with spectral peak at fmax. At these lower frequencies, the atmosphere is largely opaque and radiation from the Earth's surface is absorbed or scattered by the atmosphere. Though some radiation escapes into space, it is absorbed and subsequently re-emitted by atmospheric gases. It is this spectral selectivity of the atmosphere that is responsible for the planetary greenhouse effect.

The common household lightbulb has a spectrum overlapping the blackbody spectra of the sun and the earth. A portion of the photons emitted by a tungsten light bulb filament at 3000K are in the visible spectrum. However, most of the energy is associated with photons of longer wavelengths; these will not help a person see, but will still transfer heat to the environment, as can be deduced empirically by observing a household incandescent lightbulb. Whenever EM radiation is emitted and then absorbed, heat is transferred. This principle is used in microwave ovens, laser cutting, and RF hair removal.

Heat exposure as part of a fire test for firestop products.

Other heat transfer mechanisms

  • Latent heat: Transfer of heat through a physical change in the medium such as water-to-ice or water-to-steam involves significant energy and is exploited in many ways: steam engine, refrigerator etc. (see latent heat of fusion)
  • Heat pipes: Using latent heat and capillary action to move heat, heat pipes can carry many times as much heat as a similar-sized copper rod. Originally invented for use in satellites, they are starting to have applications in personal computers.

Heat dissipation

In cold climates, houses with their heating systems form dissipative systems. In spite of efforts to insulate such houses to reduce heat losses to their exteriors, considerable heat is lost, or dissipated, from them, which can make their interiors uncomfortably cool or cold. For the comfort of its inhabitants, the interior of a house must be maintained out of thermal equilibrium with its external surroundings. In effect, domestic residences are oases of warmth in a sea of cold and the thermal gradient between the inside and outside is often quite steep. This can lead to problems such as condensation and uncomfortable draughts (drafts) which, if left unaddressed, can cause structural damage to the property. This is why modern insulation techniques are required to reduce heat loss.

In such a house, a thermostat is a device capable of starting the heating system when the house's interior falls below a set temperature, and of stopping that same system when another (higher) set temperature has been achieved. Thus the thermostat controls the flow of energy into the house, that energy eventually being dissipated to the exterior.

References

  1. ^ Published in Poggendoff’s Annalen, Dec. 1854, vol. xciii. p. 481; translated in the Journal de Mathematiques, vol. xx. Paris, 1855, and in the Philosophical Magazine, August 1856, s. 4. vol. xii, p. 81
  2. ^ Clausius, R. (1865). The Mechanical Theory of Heat] – with its Applications to the Steam Engine and to Physical Properties of Bodies. London: John van Voorst, 1 Paternoster Row. MDCCCLXVII.
  3. ^ Smith, J.M., Van Ness, H.C., Abbot, M.M. (2005). Introduction to Chemical Engineering Thermodynamics. McGraw-Hill. ISBN 0073104450. 
  4. ^ Baierlein, Ralph (2003). Thermal Physics. Cambridge University Press. ISBN 0521658381. 
  5. ^ Schroeder, Daniel V. (2000). An introduction to thermal physics. San Francisco, California: Addison-Wesley. p. p. 18. ISBN 0-321-27779-1. "Heat is defined as any spontaneous flow of energy from one object to another, caused by a difference in temperature between the objects." 
  6. ^ Discourse on Heat and Work - Department of Physics and Astronomy, Georgia State University: Hyperphysics (online)
  7. ^ Perrot, Pierre (1998). A to Z of Thermodynamics. Oxford University Press. ISBN 0198565526. 
  8. ^ Clark, John, O.E. (2004). The Essential Dictionary of Science. Barnes & Noble Books. ISBN 0760746168. 
  9. ^ Cengel, Yungus, A.; Boles, Michael (2002). Thermodynamics - An Engineering Approach, 4th ed.. McGraw-Hill. pp. 17-18. ISBN 0-07-238332-1. 

See also

External links


 
Translations: Heat
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Dansk (Danish)
n. - varme, hede, temperatur, ophidselse, brunst, heat, løb
v. tr. - varme, opvarme, gøre hed
v. intr. - blive varm, blive hed

idioms:

  • heat barrier    varmemur
  • heat capacity    varmekapacitet, opvarmningsevne
  • heat of the moment    et øjebliks ophidselse
  • heat shield    varmeskjold
  • heat stroke    hedeslag
  • heat up    opvarme
  • heat wave    hedebølge
  • in heat    brunstig, i løbetid
  • the heat of something    varmen fra noget, højdepunktet for et eller andet
  • the heat of the day    dagens højdepunkt

Nederlands (Dutch)
hitte, vuur, kookplaat, voorronde (sport), loopsheid, drift, druk, temperatuur, verhitten, verwarmen, stoken, opwinden, aan de kook brengen

Français (French)
n. - (gén, Phys, Météo) chaleur, (Culin) feu, température, chauffage, (Sport) épreuve éliminatoire, série, (Zool) en chaleur, (fig) véhémence
v. tr. - (gén) chauffer, (Culin) faire chauffer, (Méd) échauffer (le sang)
v. intr. - chauffer

idioms:

  • heat barrier    mur thermique, mur de chaleur
  • heat capacity    capacité calorifique
  • heat shield    (Aérosp) bouclier thermique
  • heat stroke    coup de chaleur (avec collapsus)
  • heat up    chauffer, se réchauffer (l'air), faire chauffer, faire réchauffer
  • heat wave    vague de chaleur
  • in heat    en chaleur
  • in the heat of the moment    dans le feu de l'action, au moment le plus chaud
  • on heat    en chaleur
  • take the heat    soulager, apaiser
  • the heat of    la chaleur de
  • the heat of the day    au moment le plus chaud de la journée

Deutsch (German)
v. - erhitzen, heizen, aufwärmen
n. - Hitze, Heizung, Druck, (Zool.) Brunst, Vorlauf, Wärme

idioms:

  • heat barrier    (aer.) Hitzemauer
  • heat capacity    Wärmekapazität
  • heat shield    Wärmeschutz, (Astronaut) Hitzeschild
  • heat stroke    Hitzschlag
  • heat up    erwärmen
  • heat wave    Hitzewelle
  • in heat    läufig, brünstig
  • in the heat of the moment    die Hitze des Gefechts
  • on heat    brünstig werden/sein, rossig werden/sein, läufig werden/sein, rollig werden/sein
  • take the heat    eine Situation entschärfen
  • the heat of    die Hitze des
  • the heat of the day    heißester Teil des Tages

Ελληνική (Greek)
v. - θερμαίνω/-ομαι, ζεσταίνω/-ομαι, εξάπτω, ανάβω
n. - θερμότητα, ζέστη, κάψα, λάβρα, καύσωνας, έξαψη, πάθος, φλόγα, ενθουσιασμός, οργή, οργασμός, σεξουαλική διέγερση, (αθλοπ.) αγώνας δρόμου, κούρσα, προκριματικός αγώνας, (αστυνομικοί) μπάτσοι, μπασκιναρία

idioms:

  • heat barrier    θερμό κύμα
  • heat capacity    (φυσ.) θερμοχωρητικότητα
  • heat of the moment    η έξαψη της στιγμής
  • heat shield    θερμανθεκτική ασπίδα
  • heat stroke    (παθολ.) θερμοπληξία
  • heat up    ανάβω, υπερθερμαίνω/-ομαι
  • heat wave    (μετεωρ.) κύμα καύσωνα
  • in heat    σε οργασμό
  • the heat of something    στη φούντωση, στο φόρτε
  • the heat of the day    στη λάβρα της ημέρας

Italiano (Italian)
scaldare, riscaldare, calore, gara, calura

idioms:

  • heat barrier    barriera del calore
  • heat capacity    capacità termica
  • heat of the moment    nella foga del momento
  • heat shield    schermo anti-calore
  • heat stroke    colpo di sole
  • heat up    riscaldarsi
  • heat wave    ondata di caldo
  • in heat    in calore
  • the heat of    il centro di
  • the heat of the day    il momento più caldo della giornata

Português (Portuguese)
v. - esquentar
n. - calor (m), ardor (m), cio (m), inflamação (f), coerção (f)

idioms:

  • heat barrier    barreira (f) térmica (Téc.)
  • heat capacity    capacidade (f) térmica (Téc.)
  • heat of the moment    moda (f)
  • heat shield    isolamento (m) térmico (Téc.)
  • heat stroke    ataque (m) de insolação (Med.)
  • heat up    aquecer
  • heat wave    onda (f) de calor
  • in heat    no cio
  • the heat of    o calor de
  • the heat of the day    a notícia quente do dia

Русский (Russian)
зной, повышенная температура, нагрев, горячность, что-л. сделанное за один прием, пыл, нагревать, накаливать, возбуждать

idioms:

  • heat barrier    тепловой барьер
  • heat capacity    теплоемкость
  • heat of the moment    сгоряча
  • heat shield    теплозащитный экран
  • heat stroke    тепловой удар
  • heat up    подогревать
  • heat wave    тепловая волна
  • in heat    в разгаре
  • the heat of    разгар чего-л.
  • the heat of the day    разгар дня, самые жаркие часы дня

Español (Spanish)
n. - calor, calefacción, eliminatoria, serie, temperatura, fiebre, picante, pasión, acción intensa, esfuerzo único e intenso, (jer) presión policiaca, (jer) la policía, (zool) celo
v. tr. - calentar, recalentar, calor, calefacción, eliminatoria, serie
v. intr. - calentarse, excitarse

idioms:

  • heat barrier    barrera del calor
  • heat capacity    capacidad térmica
  • heat shield    escudo contra el calor
  • heat stroke    insolación
  • heat up    calentar, acalorar
  • heat wave    ola de calor
  • in heat    en celo, encelado
  • in the heat of the moment    mientras tiene la sangre caliente, en el calor del momento
  • on heat    en celo
  • take the heat    llevarse la culpa
  • the heat of    momento de máxima acción
  • the heat of the day    cuando el sol aprieta, las horas de más calor

Svenska (Swedish)
v. - upphetta (äv. bildl.), elda, hetsa
n. - hetta, värme, iver, lopp, brunst, tryck, smälta (bergsvet.), polis, skjutvapen, påtryckningar

中文(简体)(Chinese (Simplified))
热, 高潮, 热度, 把...加热, 使激动, 加热, 发热, 激昂

idioms:

  • heat barrier    热障, 速度极限
  • heat capacity    热容量
  • heat of the moment    一时的激动, 盛怒之下
  • heat shield    热屏蔽, 挡热板
  • heat stroke    中暑
  • heat up    加热
  • heat wave    热浪, 热波
  • in heat    发情, 发情期
  • the heat of something    ...的白热阶段
  • the heat of the day    在大太阳下

中文(繁體)(Chinese (Traditional))
n. - 熱, 高潮, 熱度
v. tr. - 把...加熱, 使激動
v. intr. - 加熱, 發熱, 激昂

idioms:

  • heat barrier    熱障, 速度極限
  • heat capacity    熱容量
  • heat of the moment    一時的激動, 盛怒之下
  • heat shield    熱遮罩, 擋熱板
  • heat stroke    中暑
  • heat up    加熱
  • heat wave    熱浪, 熱波
  • in heat    發情, 發情期
  • the heat of something    ...的白熱階段
  • the heat of the day    在大太陽下

한국어 (Korean)
n. - 더위, 열, 온도, 열렬함
v. tr. - 뜨겁게 하다, 흥분 시키다
v. intr. - 뜨거워지다, 흥분하다

idioms:

  • heat up    데우다
  • in heat    암내가 나서
  • the heat of something    ~의 열
  • the heat of the day    한낮 더위

日本語 (Japanese)
n. - 熱さ, 熱, 温度, 暑さ, 暖気, 熱烈さ, 興奮, 紅潮, 盛り, 一回, 熱情
v. - 熱くする, 熱くなる, 暖める, 暖まる, 興奮させる, 憤激させる, 熱する, 激させる

idioms:

  • heat barrier    熱障壁, 熱の障壁
  • heat capacity    熱容量
  • heat of the moment    勢い, 時のはずみ
  • heat shield    熱遮蔽, 熱シールド
  • heat stroke    熱中症
  • heat up    暖める, 加熱する
  • heat wave    長期にわたる酷暑, 熱波
  • in heat    盛りがついて, 激怒して, 温床に
  • the heat of    温度, 真っ最中
  • the heat of the day    炎天下で

العربيه (Arabic)
‏(فعل) يسخن, يحمي, يثير (الاسم) احترار, حماوة, حرارة, طقس حار, توقد, تأجج, اهتياج, انفعال, حدة في المذاق, تشدد في تطبيق القانون, ضغط للتأثير في مجرى الأحداث, ذروة, معمعان, وطيس‏

עברית (Hebrew)
n. - ‮חום, להט, תחרות מוקדמת, שיזוף, טעם חריף, התקופה הקולטנית של המעגל המיני אצל יונקים ממין נקבה‬
v. tr. - ‮חימם, הלהיט, ריגש‬
v. intr. - ‮התחמם‬


 
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