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Willhelm Wien

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Willhelm Wien. Nobel Prize Winner 1911 'For his discoveries regarding the laws ... In 1911 Wien won the Nobel prize for his work. concerned with the radiation of heat. ... – PowerPoint PPT presentation

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Title: Willhelm Wien


1
Willhelm Wien
  • Nobel Prize Winner 1911

For his discoveries regarding the laws governing
the radiation of heat
2
A Brief History (For Further Information see your
Handout)
  • Born on 13th January 1864 in East Prussia.
  • Started School in 1879 and in 1882 went
  • to the University of Gottingen to study
    Mathematics
  • and the Natural Sciences.
  • Appointed Professor of Physics at
    Aix-La-Chapelle
  • in 1896
  • Appointed to the same position at the University
    of
  • Giessen in 1899
  • In 1911 Wien won the Nobel prize for his work
  • concerned with the radiation of heat.

3
Why is Wien Important?
  • He is responsible for the creation of the
  • definition of Black Bodies.
  • Wien developed a law which later became
  • known as Wiens Displacement Law.
  • Wiens other work made possible the
  • calculation of factors relevant to Nuclear
  • Reactions.

These developments of Wiens led to many advances
in Physics they allowed Astrophysicists to
measure the temperature of stars by their peak
emission
4
What is a Black Body?
  • A perfect absorber of radiation, absorbing 100
    of the
  • radiation that strikes it. No reflection
    occurs, hence the
  • term Black Body.
  • A perfect emitter of radiation, radiating 100
    of that
  • which it produces.
  • Stars are a theoretical example of Black Bodies.

Demonstration of a Black Body Absorber
5
Demonstration of a Black Body
Tin Can
6
Development of Wiens Law
  • The link between the temperature of a body
  • and the wavelength of its peak emission

Peak emission measured using Spectroscopy
  • Discovery that the wavelength of peak
  • is inversely proportional to the temperature
  • of the body
  • Discovery of the constant of proportionality
  • which links the two
  • 2.9 10-3 m K

Such that
?max T A constant ( 2.9 10-3 m K )
7
Wiens Law and the Electromagnetic Spectrum
8
(Consult your hand-out for diagrams relevant to
this page)
  • Wiens Law in reference to stars.
  • Black Bodies that emit radiation appear
  • different colours according to their
  • temperature.
  • Radiation emitted by the human body.
  • Worked example using Wiens Law.
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