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Thermal Properties Of Matter
Assuming the sun to be a spherical body of radius R at a temperature of T K, evaluate the total radiant power, incident on Earth, at a distance r from the Sun.
where r0 is the radius of the Earth and σ is Stefan’s constant
C.
Some More Questions From Thermal Properties of Matter Chapter
If Cp and Cv denote the specific heats of nitrogen per unit mass at constant pressure and constant volume respectively, then
A radiation of energy E falls normally on a perfectly reflecting surface. The momentum transferred to the surface is
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