Heat
Adapted from Wikipedia · Adventurer experience
Heat is a special kind of energy that moves from one place to another because of a difference in temperature. In science, heat is described as energy moving between things when their temperatures are different. It’s important to know that an object itself doesn’t “contain” heat — heat is the energy moving in or out of the object.
We often talk about heat as the warmth or energy inside an object, which is related to its temperature. For example, when you touch a hot stove, heat moves from the stove to your hand, making it warm. Scientists measure heat using tools and methods called calorimetry. This can involve watching how much ice melts or how the temperature of a material changes when heat is added or removed.
In the worldwide system used for measuring things called the International System of Units (SI), the unit for measuring heat is called the joule, written as “J.” This helps scientists all over the world talk about and compare amounts of heat in a clear way.
Notation and units
Heat is a type of energy. We measure it in units called joules (J). This is the standard unit used in science around the world, known as the International System of Units (SI). Some areas of engineering use different units, like the British thermal unit (BTU) or the calorie.
The rate at which heat moves is measured in watts (W). This means one joule of energy moving each second. The symbol for heat, Q, was introduced by scientists Rudolf Clausius and Macquorn Rankine around the year 1859.
History
Heat is a form of energy that moves between objects when their temperatures are different. It is not something objects "contain," but something that moves from one place to another.
In the past, scientists thought about heat in different ways. Some believed heat was a special kind of matter, like a fluid called "phlogiston" or "caloric." Others thought heat was related to the movement of tiny particles in objects. Over time, experiments showed that heat is connected to the movement of particles and to energy changes in objects.
Scientists have studied heat for centuries. In the 1600s and 1700s, they began to understand that heat might be linked to how fast particles in an object are moving. By the 1800s, the idea that heat is a form of energy became widely accepted. Today, we know that heat is one way energy can move, and it plays a key role in how we understand temperature and energy changes in the world around us.
Heat transfer
When a warm object touches a cool object, the warm object gets cooler and the cool object gets warmer. This happens because heat moves from the warmer object to the cooler one.
Heat can also move through space by radiation. For example, the Sun warms the Earth by sending out heat that travels through space.
Another way heat moves is through convection. This happens when a liquid or gas moves and carries heat with it. For example, when water in a pot heats up, the warm water rises to the top, and cooler water moves to the bottom to be heated.
In science, we learn how heat moves in different situations. Heat can make things work. For example, engines use heat to move. We can also use work to move heat from one place to another, like in a refrigerator.
Latent and sensible heat
In 1847, James Prescott Joule talked about two kinds of heat: latent heat and sensible heat. Latent heat is the energy a substance uses or gives off when it changes from one form to another, like when ice turns to water or water turns to steam. The temperature does not change during this process. Sensible heat is the energy that makes particles move faster or slower, which we feel as hot or cold.
Heat capacity
Heat capacity measures how much heat energy is needed to change the temperature of an object. It shows how much heat a material can hold. For example, the heat needed to warm up a small piece of metal is different from the heat needed to warm the same amount of water.
Different materials have different heat capacities. Some gases, like helium, keep a steady heat capacity. Others, like hydrogen, change a little depending on temperature. Heat can also change how materials look, like turning ice into water when it gets warm.
Hotness
Hotness is an important idea in thermodynamics. It helps us understand how things can make other things warmer or cooler. When something is hotter, it can give heat to something that is colder.
Some things change too fast or are too mixed up to have a temperature we can measure. But even these can still give or receive heat. For things that stay the same long enough, we can measure their temperature with a special tool called a thermometer. This measurement is called an empirical temperature.
The zeroth law of thermodynamics explains how we know when things are in balance with each other in terms of heat. It helps us understand how heat moves between different objects.
Classical thermodynamics
Heat and enthalpy
Further information: Internal energy and Enthalpy
In thermodynamics, heat is energy that moves between a system and its surroundings because of a temperature difference. It is not something inside the system, but something that moves in or out.
When heat moves into a closed system (one that does not gain or lose matter), it changes the system's internal energy. This can also happen if the system does work on its surroundings or if work is done on the system.
For example, if you heat water in a pot, the heat you add makes the water hotter. If the water then evaporates, it pushes the air away.
Heat and entropy
Main article: Entropy
When heat moves, it also affects a property called entropy, which measures how disordered or random things are. In 1856, a scientist named Rudolf Clausius said that when heat moves from a hotter place to a cooler one, the total entropy of the system and its surroundings always increases. This is one way of stating the second law of thermodynamics.
For example, imagine a hot cup of coffee. When it cools down, heat moves from the coffee to the surrounding air. The coffee becomes less hot, and the air becomes slightly warmer. Even though the total amount of energy stays the same, the entropy of the universe increases because the energy spreads out more evenly.
| Δ S = Q T {\displaystyle \Delta S={\frac {Q}{T}}} | 1 |
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