An object's or space's temperature increases when heat energy moves into it, increasing the average
kinetic energy of its atoms, e.g., of things and air in a room. Heat energy leaving an object or space lowers its temperature. Heat flows from one place to another (always from a higher temperature to a lower one) by up to three processes: conduction, convection and radiation: • In
conduction, energy is passed from one atom to another by direct contact. • In
convection, heat energy moves by conduction into some movable fluid (such as air or water) and the fluid moves from one place to another, carrying the heat with it. At some point the heat energy in the fluid is usually transferred to some other object by means conduction again. The movement of the fluid can be driven by
negative buoyancy, as when cooler (and therefore denser) air drops and thus upwardly displaces warmer (less dense) air (
natural convection), or by fans or pumps (
forced convection). • In
radiation, the heated atoms make electromagnetic emissions absorbed by remote other atoms, whether nearby or at astronomical distance. For example, the sun radiates heat as both invisible and visible electromagnetic energy. What we know as
light is but a narrow region of the electromagnetic spectrum. If, in a place or thing, more energy is received than is lost, its temperature increases. If the amount of energy coming in and going out are exactly the same, the temperature stays constant—there is thermal balance, or
thermal equilibrium. ==See also==