Perfectly black body - class-XI
Description: perfectly black body | |
Number of Questions: 24 | |
Created by: Sangita Pandit | |
Tags: physics heat transfer thermal properties energy production |
The coefficient of transmission for an ideal black body is :
Out of the following, which body is not an ideal black body?
Read the following statements carefully
(A) Black body radiation is white
(B) Emissivity of a body is equal to its absorptive power
Mark correct option:
The absorptivity of Lamp black is:
Black body spectrum is
Stefan-Boltzmanns Law for a perfect black body is represented by
Ferry's black body is accurately represented by
Ferry's black body is
Black body radiation is
The original temperature of a black body is $727^\circ C$. Calculate temperature at which total radiant energy from this black body becomes double:
Temp. of black body is $3000K$ when black body cools. Then change in wavelength $\Delta \lambda=9$ micron corresponding to maximum energy density. Now temp. of black body is:
The rate of emission of radiation of a black body at 273$^{ \circ }{ C }$ is E, then the rate of emission of radiation of this body at 0$^{ \circ }{ C }$ will be :-
For non black bodies, the range of values of emissivity $e$ is
A blackbody does not
An ideal black body is a :
Which of the following is more close to a black body?
Initially a black body at absolute temperature $T$ is kept inside a closed chamber at absolute temperature $T _{o}$. Now the chamber is slightly opened to allow sun rays to enter. It is observed that temperatures $T$ and $T _{o}$ remains constant.Which of the following statement is/are true?
An ideal black body at room temperature is thrown in a furnace. It is observed that
A spherical body of area A and emissivity $e = 0.6$ is kept inside a perfectly black body. Total heat radiated by the body at temperature $T$
Emissivity of a perfect black body is
Radiation coming from the hole of a Ferry's Black body is called
Which of the following is an example of a black body radiation?
The Wien's displacement law for a black body is
($T$ is the absolute temperature in $K$
$b$ is a constant of proportionality
$e$ is the emissivity of the black body)