Construct · 1 fields · 2 citations
One name. One construct. A landmark on the map.
● anchor · a standalone construct Nearest construct by meaningStefan-Boltzmann lawcompare the meaningsEvery construct on the map is compared with every other by the meaning of its definitions, and the closest one is surfaced here. The nearest construct to black-body radiation is Stefan-Boltzmann law.
Hold this as a prompt, not a verdict. Two constructs sitting close in meaning is a reason to read them side by side and decide for yourself whether they are one idea under two names. It is not proof that they are. Compare the meanings in the Collider.
A single standalone construct; nearby constructs are located against it in the Collider. Tap a field for its definition, unit, and measures.
Gustav Kirchhoff introduced the idea in 1860, proving that for a body in thermal equilibrium, meaning one whose temperature has settled and stopped changing, the ratio of the radiation it emits to the radiation it absorbs depends only on temperature and wavelength, and he named the idealized perfect absorber that also emits the maximum possible radiation a black body. Black-body radiation is the characteristic electromagnetic radiation such a body gives off: a smooth spectrum whose shape and total intensity are fixed by temperature alone, independent of the body's material or shape. Classical physics could not reproduce the measured spectrum, and Max Planck resolved the problem in 1901 with what became Planck's law by assuming that energy is emitted only in discrete packets, a hypothesis that opened quantum theory. The construct is a landmark because a single number, the temperature, fixes the entire spectrum, which is why it underlies work from the surface temperatures inferred for stars to the calibration of infrared thermometers and the measurement of the 2.7 K cosmic microwave background.[1][2]
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