Josef Stefan ( 24 March 1835 – 07 January 1893) was an Austrian physicist best known for his contributions to the study of heat radiation. He made significant advances in understanding the behavior of blackbody radiation, and his work laid the foundation for later developments in the field.
Stefan's most notable contribution is the formulation of Stefan's law, which describes the total energy radiated by a perfect black body per unit surface area and unit time. The law, published in 1879, states that the total energy radiated (E) is proportional to the fourth power of the absolute temperature (T) of the black body. Mathematically, it is expressed as:
E=σ⋅T4
where σ is the Stefan-Boltzmann constant.
Later, in 1884, Austrian physicist Ludwig Boltzmann extended Stefan's work, incorporating a constant of proportionality that became known as the Stefan-Boltzmann constant. This constant is crucial for quantifying the total power radiated by a black body at a given temperature.
Stefan's law has had profound implications for astrophysics and our understanding of stars, as it provides a basis for determining the temperature and energy output of celestial bodies. The Stefan-Boltzmann law remains fundamental in the study of thermodynamics and heat radiation.
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