Home
Class 12
PHYSICS
If temperature of ideal black body is de...

If temperature of ideal black body is decreased from T to T/2 than find out percentage loss in emissive rate

Text Solution

AI Generated Solution

The correct Answer is:
To solve the problem of finding the percentage loss in the emissive rate of an ideal black body when its temperature is decreased from \( T \) to \( \frac{T}{2} \), we can follow these steps: ### Step 1: Understand the Emissive Rate The emissive rate \( E \) of a black body is proportional to the fourth power of its absolute temperature \( T \). Mathematically, we can express this as: \[ E \propto T^4 \] ### Step 2: Calculate the Emissive Rate at Initial Temperature Let the emissive rate at the initial temperature \( T \) be \( E_1 \): \[ E_1 = k \cdot T^4 \] where \( k \) is a proportionality constant. ### Step 3: Calculate the Emissive Rate at Reduced Temperature When the temperature is decreased to \( \frac{T}{2} \), the new emissive rate \( E_2 \) can be calculated as: \[ E_2 = k \cdot \left(\frac{T}{2}\right)^4 \] Calculating \( E_2 \): \[ E_2 = k \cdot \frac{T^4}{16} \] ### Step 4: Find the Loss in Emissive Rate The loss in emissive rate can be calculated as: \[ \text{Loss} = E_1 - E_2 \] Substituting the values: \[ \text{Loss} = k \cdot T^4 - k \cdot \frac{T^4}{16} \] Factoring out \( k \cdot T^4 \): \[ \text{Loss} = k \cdot T^4 \left(1 - \frac{1}{16}\right) = k \cdot T^4 \cdot \frac{15}{16} \] ### Step 5: Calculate the Percentage Loss The percentage loss in emissive rate is given by: \[ \text{Percentage Loss} = \frac{\text{Loss}}{E_1} \times 100\% \] Substituting the values: \[ \text{Percentage Loss} = \frac{k \cdot T^4 \cdot \frac{15}{16}}{k \cdot T^4} \times 100\% \] The \( k \cdot T^4 \) terms cancel out: \[ \text{Percentage Loss} = \frac{15}{16} \times 100\% \] Calculating this gives: \[ \text{Percentage Loss} = 93.75\% \] ### Step 6: Final Result Thus, the percentage loss in the emissive rate when the temperature is decreased from \( T \) to \( \frac{T}{2} \) is approximately: \[ \text{Percentage Loss} \approx 93.75\% \]

To solve the problem of finding the percentage loss in the emissive rate of an ideal black body when its temperature is decreased from \( T \) to \( \frac{T}{2} \), we can follow these steps: ### Step 1: Understand the Emissive Rate The emissive rate \( E \) of a black body is proportional to the fourth power of its absolute temperature \( T \). Mathematically, we can express this as: \[ E \propto T^4 \] ...
Promotional Banner

Topper's Solved these Questions

  • GRAVITATION

    ALLEN|Exercise Exercise 4 A (Conceptual Subjective Exercise)|14 Videos
  • GRAVITATION

    ALLEN|Exercise Exercise 4 B (Brain Storming Subjective Exercise)|20 Videos
  • GRAVITATION

    ALLEN|Exercise Exercise 2 (Brain Teasers)|27 Videos
  • GEOMETRICAL OPTICS

    ALLEN|Exercise subjective|14 Videos
  • KINEMATICS-2D

    ALLEN|Exercise Exercise (O-2)|46 Videos

Similar Questions

Explore conceptually related problems

If the temperature of a black body is raised from 300K to 600K by what factor the rate of emission shall increase ?

Statement-1: When the temperature of a black body is doubled from t^(@)C to 2t^(@)C , the radiant power becomes 16 times. Statement-2: The radiant power of a body is proportional to fourth power of absolute temperature.

If the temperature of a black body incresese from 7^(@)C to 287^(@)C then the rate of energy radiation increases by

If the pressure of an ideal gas at constant volume is decreased by 20% then the percentage change in temperature will be

If the temperature of hot black body is raised by 5%, rate of heat energy radiated would be increased by how much percentage ?

The temperature of n-moles of an ideal gas is increased from T_0 to 2T_0 through a process p=alpha/T . Find work done in this process.

Calculate the temperature of the black body from given graph.

When the temperature of a black body increases, it is observed that the wavelength corresponding to maximum energy changes from 0.26mum to 0.13mum . The ratio of the emissive powers of the body at the respective temperatures is

The temperature of an spherical isolated black body falls from T_(1) and T_(2) in time t them time t is

Let the wavelength at which the the spectral emissive power of a black body (at a temperature T) is maximum, be denoted by lamda_(max) as the temperature of the body is increased by 1K, lamda_(max) decreases by 1 percent. The temperature T of the black body is

ALLEN-GRAVITATION-Exercise 3 (Miscellaneous Type Questions)
  1. Statemet-1: Two satellites A & B are in the same orbit around the eart...

    Text Solution

    |

  2. Statement-1: The acceleration of a particle near the earth surface dif...

    Text Solution

    |

  3. Statement-1: Kepler's law of areas is equivalent to the law of conserv...

    Text Solution

    |

  4. Statement-1: A satellite is moving in a circular orbit of the earth. I...

    Text Solution

    |

  5. Statement-1:A personfeels weightlessness in an artificial satellite of...

    Text Solution

    |

  6. Statement-1: Moon cannot be used as a satellite for communication. S...

    Text Solution

    |

  7. Statement-1: There is not atmosphere on the moon. Statement-2: The r...

    Text Solution

    |

  8. Statement-1: Pendulum clock stops working on the spaceship Statement...

    Text Solution

    |

  9. Statement-1: Escape velocity is independent of the angle of projection...

    Text Solution

    |

  10. Statement-1: The plane of the orbit of an artificial satellite must co...

    Text Solution

    |

  11. Statement-1:When a planet approches the point which is farthest from t...

    Text Solution

    |

  12. When a particle is projected from the surface of earth, its mechanical...

    Text Solution

    |

  13. When a particle is projected from the surface of earth its mechanical ...

    Text Solution

    |

  14. A solid sphere of mass M and radius R is surrounded by a spherical she...

    Text Solution

    |

  15. It is easier to draw up a wooden block along an inclined plane than ha...

    Text Solution

    |

  16. A solid sphere of mass M and radius R is surrounded by a spherical she...

    Text Solution

    |

  17. For circular orbits the potential energy of the companion star is cons...

    Text Solution

    |

  18. If temperature of ideal black body is decreased from T to T/2 than fin...

    Text Solution

    |

  19. In the picture below the planet orbits around the sun with a period of...

    Text Solution

    |

  20. In the picture below the planet orbits around the sun with a period of...

    Text Solution

    |