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Two stars radiate maximum energy at wave...

Two stars radiate maximum energy at wavelength `3.6xx10^(-7)` m and `4.8xx10^(-7)` m respectively. What is the ratio of their temperatures ?

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To find the ratio of the temperatures of two stars that radiate maximum energy at different wavelengths, we can use Wien's Displacement Law. Here’s a step-by-step solution: ### Step 1: Identify the wavelengths Let: - \( \lambda_{m1} = 3.6 \times 10^{-7} \, \text{m} \) (wavelength for star 1) - \( \lambda_{m2} = 4.8 \times 10^{-7} \, \text{m} \) (wavelength for star 2) ### Step 2: Apply Wien's Displacement Law Wien's Displacement Law states that the wavelength corresponding to maximum energy (\( \lambda_m \)) is inversely proportional to the temperature (T) of the black body. Mathematically, this can be expressed as: \[ \lambda_m \cdot T = b \] where \( b \) is a constant. From this, we can write: \[ \lambda_{m1} \cdot T_1 = \lambda_{m2} \cdot T_2 \] ### Step 3: Rearrange the equation to find the temperature ratio We need to find the ratio of the temperatures \( \frac{T_1}{T_2} \): \[ \frac{T_1}{T_2} = \frac{\lambda_{m2}}{\lambda_{m1}} \] ### Step 4: Substitute the values of the wavelengths Substituting the values of \( \lambda_{m1} \) and \( \lambda_{m2} \): \[ \frac{T_1}{T_2} = \frac{4.8 \times 10^{-7}}{3.6 \times 10^{-7}} \] ### Step 5: Simplify the ratio The \( 10^{-7} \) in the numerator and denominator cancels out: \[ \frac{T_1}{T_2} = \frac{4.8}{3.6} \] Now, simplify \( \frac{4.8}{3.6} \): - Dividing both the numerator and denominator by 1.2: \[ \frac{4.8 \div 1.2}{3.6 \div 1.2} = \frac{4}{3} \] ### Final Answer Thus, the ratio of the temperatures \( \frac{T_1}{T_2} \) is: \[ T_1 : T_2 = 4 : 3 \] ---

To find the ratio of the temperatures of two stars that radiate maximum energy at different wavelengths, we can use Wien's Displacement Law. Here’s a step-by-step solution: ### Step 1: Identify the wavelengths Let: - \( \lambda_{m1} = 3.6 \times 10^{-7} \, \text{m} \) (wavelength for star 1) - \( \lambda_{m2} = 4.8 \times 10^{-7} \, \text{m} \) (wavelength for star 2) ### Step 2: Apply Wien's Displacement Law ...
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