All objects emit electromagnetic radiation as a result of their temperature. At everyday temperatures this radiation is predominantly in the infrared region of the electromagnetic spectrum, though very hot objects (such as the Sun or a glowing light bulb filament) also emit visible light. The hotter an object, the more radiation it emits per unit time, and the higher the frequency of the peak emission.
Because thermal radiation consists of electromagnetic waves, it can travel through empty space. This is why the Earth receives energy from the Sun across 150 million kilometres of vacuum, and why we feel the warmth of a fire even without direct contact or air movement.
The rate at which a body emits or absorbs thermal radiation depends on several factors.
The surface of a body plays a major role in determining how well it emits and absorbs radiation:
A perfect emitter and absorber of radiation is called a black body. Real surfaces approximate this behaviour to varying degrees depending on their colour and texture.
| Surface Type | Emission of Radiation | Absorption of Radiation |
|---|---|---|
| Dark, matt | Good emitter | Good absorber |
| Light, shiny | Poor emitter | Poor absorber (good reflector) |
The rate of emission of thermal radiation increases strongly with temperature. A hotter surface emits significantly more radiation per unit time than a cooler surface of the same area and type. At the same time, the net rate of energy exchange between a body and its surroundings depends on the difference in temperature: the greater the temperature difference, the faster the net energy transfer by radiation.
A larger surface area results in a greater rate of emission and absorption of thermal radiation, since more surface is available to emit or intercept radiation. For this reason, objects with large surface areas cool or warm by radiation more quickly than compact objects of the same volume and surface type.