Wien displacement law

E31550

Wien's displacement law is a physical law that relates the temperature of a blackbody to the wavelength at which it emits radiation most intensely.

Aliases (1)

Statements (43)
Predicate Object
instanceOf empirical law
law of black-body radiation
physical law
appliesTo blackbody
approximationOf Planck radiation law
assumes continuous spectrum
isotropic emission
category laws of physics
radiation laws
constantApproximateValue 2.897771955×10^-3 m·K
constantSymbol b
describes relationship between blackbody temperature and peak emission wavelength
domain thermal equilibrium
field astrophysics
statistical mechanics
thermal radiation
thermodynamics
hasConsequence color of a blackbody shifts from red to blue as temperature increases
peak of solar spectrum lies in visible range due to Sun’s surface temperature
hasConstant Wien displacement constant
hasEquation λ_max = b / T
ν_max ≈ (k_B T)/h (for frequency form, approximate)
hasSIUnitForConstant meter kelvin
implies cooler bodies emit peak radiation at longer wavelengths
hotter bodies emit peak radiation at shorter wavelengths
isPartOf black-body radiation theory
namedAfter Wilhelm Wien
namedEntityType scientific law
predicts wavelength of peak emission for a blackbody at given temperature
relatedTo Planck radiation law
Rayleigh–Jeans law
Stefan–Boltzmann law
relatesQuantity temperature
wavelength of maximum spectral radiance
supportsConcept color–temperature relation of stars
symbolicForm λ_max T = b
usedFor design of thermal radiation sources
estimating surface temperature of stars from color
estimating temperature of incandescent objects from emission spectrum
infrared thermometry
thermal imaging calibration
validFor ideal blackbody
yearProposed 1893

Referenced by (2)
Subject (surface form when different) Predicate
Planck radiation law
Stefan–Boltzmann law ("Wien’s displacement law")
relatedTo

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