Home
Class 12
PHYSICS
A black body is at a temperature of 2880...

A black body is at a temperature of 2880 K. The energy of radiation emitted by this object with wavelength between 499 nm and 500 nm is`U_(1)`, between 999 nm and 1000 nm is `U_(2)` and between 1499 nm and 1500 nm is `U_(3)`. The Wein's constant `b = 2.88 xx 10^(6) "nm K"`. Then

A

`U_1 = 0`

B

`U_2 = 0`

C

`U_1 = U_2`

D

`U_2 gt U_1`

Text Solution

AI Generated Solution

The correct Answer is:
To solve the problem, we need to analyze the radiation emitted by a black body at a temperature of 2880 K and compare the energies of radiation emitted in specific wavelength ranges. We will use Wien's Displacement Law to find the wavelength at which the intensity of radiation is maximum. ### Step-by-Step Solution: **Step 1: Calculate the wavelength at maximum intensity (λ_max)** According to Wien's Displacement Law, the wavelength at which the intensity is maximum is given by the formula: \[ \lambda_{\text{max}} = \frac{b}{T} \] where \( b = 2.88 \times 10^6 \, \text{nm K} \) and \( T = 2880 \, \text{K} \). **Calculation:** \[ \lambda_{\text{max}} = \frac{2.88 \times 10^6 \, \text{nm K}}{2880 \, \text{K}} = 1000 \, \text{nm} \] **Step 2: Analyze the wavelength ranges for U1, U2, and U3** - \( U_1 \) is the energy emitted between 499 nm and 500 nm. - \( U_2 \) is the energy emitted between 999 nm and 1000 nm. - \( U_3 \) is the energy emitted between 1499 nm and 1500 nm. **Step 3: Determine the position of λ_max relative to U1, U2, and U3** Since \( \lambda_{\text{max}} = 1000 \, \text{nm} \): - The wavelength range for \( U_1 \) (499 nm to 500 nm) is far below \( \lambda_{\text{max}} \). - The wavelength range for \( U_2 \) (999 nm to 1000 nm) is at the peak intensity. - The wavelength range for \( U_3 \) (1499 nm to 1500 nm) is far above \( \lambda_{\text{max}} \). **Step 4: Compare the energies** - Since \( U_2 \) is at the maximum intensity, it will have the highest energy. - \( U_1 \) is significantly lower than \( \lambda_{\text{max}} \) and thus will have less energy. - \( U_3 \) is also far from the peak, and its energy will be lower than \( U_2 \) but could be comparable to \( U_1 \). **Conclusion:** From the analysis, we can conclude: - \( U_2 > U_1 \) - \( U_2 > U_3 \) - \( U_1 \) and \( U_3 \) will have lower energies than \( U_2 \). Thus, the correct answer is that \( U_2 \) is greater than \( U_1 \).
Promotional Banner

Similar Questions

Explore conceptually related problems

A blackbody is at a temperature of 2880K. The energy of radiation emitted by this object with wavelength between 499nm and 500nm is U_1 , between 999nm and 1000nm is U_2 and between 1499 nm and 1500 nm is U_3 . The Wien constant b=2.88xx10^6nmK . Then

A black body is at a temperature of 5760 K . The energy of radiation emitted by the body at wavelength 250 nm is U_(1) at wavelength 500 nm is U_(2) and that at 1000 nm is U_(3) . Wien's consant, b = 2.88 xx 10^(6) nmK . Which of the following is correct?

Energy of radiation emitted by a black body at temperature 3000 K is u_(1) for wavelength between 8000 Å and 9000Å , u_(2) for wavelength between 9000 Å and 10000Å and u_(3) forwavelength between 10000Åand 11000Å .Which of the following is true? [Wien’s constant b=2.88xx10^(-3)mK]

Compare the energies of two radiations E_(1) with wavelength 800 nm and E_(2) with wavelength 400 nm.

Find the wavelength in a hydrogen spectrum between the range 500nm to 700nm

Experimental investigations show that the intensity of solar radiation is maximum for a wavelength 480 nm in the visible ragion. Estimate the surface temperature of sun. (Given Wien's constant b = 2.88 xx 10^(-3) m K ).

White light is a mixture of light of wavelengths between 400 nm and 700 nm. If this light goes through water (mu = 1.33) what are the limits of the wavelength there ?

The energy of a photon is 3 xx10^(-12)erg .What is its wavelength in nm? (h=6.62 xx 10^(-27)erg-s,3 xx 10^(10)cm s^(-1))

The intensity of radiation emitted by the sun has its maximum value at a wavelength of 510 nm and that emitted by the North star has the maximum value at 350 nm. If these stars behave like black bodies, then the ratio of the surface temperatures of the sun and the north star is

The intensity of radiation emitted by the sun has its maximum value at a wavelength of 510 nm and that emitted by the North star has the maximum value at 350 nm. If these stars behave like black bodies, then the ratio of the surface temperatures of the sun and the north star is