Kirchhoff's Law of Radiation

IMPORTANT

Kirchhoff's Law of Radiation: Overview

This Topic covers sub-topics such as Kirchhoff's Law of Radiation and Thought Experiment to Prove Kirchhoff's Law of Radiation

Important Questions on Kirchhoff's Law of Radiation

EASY
IMPORTANT

 In accordance with Kirchhoff's law (Assume transmissivity at0 for all the cases)

MEDIUM
IMPORTANT

With an increase in wavelength, the monochromatic emissive power of a black body

EASY
IMPORTANT

 The absorptivity of black body equals to

EASY
IMPORTANT

If radiant energy E B emitted by the black surface strikes the non-black surface. If non-black surface has absorptivity α, it will absorb how many radiations?

EASY
IMPORTANT

 If two surfaces are at the same temperature, then the conditions correspond to mobile thermal equilibrium for which the resultant interchange of heat is zero are

HARD
IMPORTANT

State Kirchhoff's law of radiation and prove it theoretically.

MEDIUM
IMPORTANT

A planet of radius Rp is revolving around a star of radius R*, which is at temperature T*. The distance between the star and the planet is d. If the planet's temperature is fT, then f is proportional to

EASY
IMPORTANT

Relation between emissivity e and absorptive power a is (for black body)
 

EASY
IMPORTANT

State Kirchhoff’s law of radiation.

EASY
IMPORTANT

State:

Kirchhoff's law of radiation. 

EASY
IMPORTANT

"Spectral line of the emission is same as that of the absorption" is the statement of

EASY
IMPORTANT

The temperatures of two bodies A and B are 727°C and 327°C, respectively. The ratio HA:HB of heat radiated by the bodies is

EASY
IMPORTANT

Assertion: When a green glass is heated in a furnace and taken out, it is found to glow with red light.

Reason: Red and green are complementary.

EASY
IMPORTANT

A body has same temperature as that of the surrounding. Then

MEDIUM
IMPORTANT

Three objects coloured black, gray and white can with stand hostile conditions at 2800°C. These objects are thrown into furnace where each of them attains a temperature of 2000°C. Which object will glow brightest?

EASY
IMPORTANT

"Good emitters are good absorbers" is a statement concluded from

EASY
IMPORTANT

From Kirchhoff's law the ratio of emissive power and absorption power of all bodies -

EASY
IMPORTANT

Two bodies A and B having temperatures 327 and 427 are radiating heat to the surrounding. The surrounding temperature is 27 . The ratio of rate of heat radiation of A to that of B is

MEDIUM
IMPORTANT

Two spheres of radii 8 cm and 2 cm are cooling. Their temperatures are 127 and 527 respectively. Find the ratio of energy radiated by them in the same time

EASY
IMPORTANT

"Good emitters are good absorbers" is a statement concluded from