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Question: The maximum in the energy distribution spectrum of the Sun occurs at 4753 \( A^\circ \) and 6050K te...

The maximum in the energy distribution spectrum of the Sun occurs at 4753 AA^\circ and 6050K temperature. What will be the temperature of the star in K whose energy distribution shows a maximum at 9506 AA^\circ ?

Explanation

Solution

The energy distribution spectrum of any body is governed by the Wien’s displacement law. This law is valid for wavelengths corresponding to maximum emissions.

Formula used: λT= constant\lambda T = {\text{ constant}} where λ\lambda is the wavelength at maximum energy of the body in consideration and TT is the temperature corresponding to it on the energy distribution curve.

Complete step by step solution:
In this question we are provided with the following data for two different bodies:
Wavelength of max. energy of Sun λS=4753A{\lambda _S} = 4753A^\circ .
Temperature at this wavelength TS=6050K{T_S} = 6050K .
Wavelength of max. energy of star λ=9506A\lambda = 9506A^\circ .
Here, A{A^\circ } is called Angstrom and we know that 1A=1010m1{A^\circ } = {10^{ - 10}}m .
We are required to find the temperature TT of the star.
We know that the Wien’s displacement law in equation form is given as:
λT= constant\lambda T = {\text{ constant}}
So, when we use this equation for the Sun and the given star we get,
λSTS=λT{\lambda _S}{T_S} = \lambda T
Where λs{\lambda _s} is the wavelength of the sun at maximum energy, Ts{T_s} is the temperature at this wavelength, λ\lambda is the wavelength of the given star at maximum energy and TT is the temperature at this wavelength.
Putting the values in this gives us:
4753×6050=9506×T4753 \times 6050 = 9506 \times T
Moving the unknown TT on the LHS and solving we get,
T=4753×60509506T = \dfrac{{4753 \times 6050}}{{9506}}
T=3025K\Rightarrow T = 3025K
As the units of wavelength are same for both the given stars, the units of Temperature would also remain the same i.e. Kelvin.
\therefore Hence, the temperature of the star is 3025 Kelvins.

Note:
Ideally, Wien’s displacement law works for ideal bodies that absorb and emit all frequencies of light. This law implies that the energy distribution curve for all the bodies follows the same basic curve but the peak occurs at different wavelengths for different temperatures.