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Question: If the wavelength of light that is emitted from hydrogen atom when an electron falls from orbit \(n=...

If the wavelength of light that is emitted from hydrogen atom when an electron falls from orbit n=2n=2 to orbit n=1n=1 is 122 nm122\text{ nm}, then minimum wavelength of the series is:
A.9150 A9150\text{ }\overset{\circ }{\mathop{\text{A}}}\,
B.812 A812\text{ }\overset{\circ }{\mathop{\text{A}}}\,
C.915 A915\text{ }\overset{\circ }{\mathop{\text{A}}}\,
D.405 A405\text{ }\overset{\circ }{\mathop{\text{A}}}\,

Explanation

Solution

When the electron falls orbit n=2n=2 to orbit n=1n=1, we can use the formula 1λ=RH[1n121n22]\dfrac{1}{\lambda }={{R}_{H}}\left[ \dfrac{1}{n_{1}^{2}}-\dfrac{1}{n_{2}^{2}} \right] to calculate the minimum wavelength of the series. Here n1{{n}_{1}} is the orbit with lowest energy while n2{{n}_{2}} is an orbit with highest energy level. This formula gives us a relationship between wavelength and the number of orbits.
Formula used:
1λ=RH[1n121n22]\dfrac{1}{\lambda }={{R}_{H}}\left[ \dfrac{1}{n_{1}^{2}}-\dfrac{1}{n_{2}^{2}} \right]

Complete answer:
In the question it is given that when an electron falls from orbit n=2n=2 to orbit n=1n=1, its wavelength is 122 nm122\text{ nm}, therefore on substituting these values known to us in the formula 1λ=RH[1n121n22]\dfrac{1}{\lambda }={{R}_{H}}\left[ \dfrac{1}{n_{1}^{2}}-\dfrac{1}{n_{2}^{2}} \right] we get:
1122=RH[112122] 1122=RH[1114] 1122=RH[414] 1122=3RH4equation 1 \begin{aligned} & \dfrac{1}{122}={{R}_{H}}\left[ \dfrac{1}{{{1}^{2}}}-\dfrac{1}{{{2}^{2}}} \right] \\\ & \Rightarrow \dfrac{1}{122}={{R}_{H}}\left[ \dfrac{1}{1}-\dfrac{1}{4} \right] \\\ & \Rightarrow \dfrac{1}{122}={{R}_{H}}\left[ \dfrac{4-1}{4} \right] \\\ & \Rightarrow \dfrac{1}{122}=\dfrac{3{{R}_{H}}}{4}-\text{equation }1 \\\ \end{aligned}
As asked in the question, we need to find the minimum wavelength of the series. The wavelength will be minimum when orbit n1=1{{n}_{1}}=1 to orbit n2={{n}_{2}}=\infty . Substituting the values in the equation we get:
1λmin=RH[1121] 1λmin=RH[110] 1λmin=RHequation 2 \begin{aligned} & \dfrac{1}{{{\lambda }_{\min }}}={{R}_{H}}\left[ \dfrac{1}{{{1}^{2}}}-\dfrac{1}{\infty } \right] \\\ & \Rightarrow \dfrac{1}{{{\lambda }_{\min }}}={{R}_{H}}\left[ \dfrac{1}{1}-0 \right] \\\ & \Rightarrow \dfrac{1}{{{\lambda }_{\min }}}={{R}_{H}}-\text{equation }2 \\\ \end{aligned}
Now dividing equation 11 by equation 22, we get:
11221λmin=3R4R λmin122=34 λmin=34×122 λmin=91.5 nm λmin=915 A \begin{aligned} & \dfrac{\dfrac{1}{122}}{\dfrac{1}{{{\lambda }_{\min }}}}=\dfrac{\dfrac{3R}{4}}{R} \\\ & \Rightarrow \dfrac{{{\lambda }_{\min }}}{122}=\dfrac{3}{4} \\\ & \Rightarrow {{\lambda }_{\min }}=\dfrac{3}{4}\times 122 \\\ & \Rightarrow {{\lambda }_{\min }}=91.5\text{ nm} \\\ & \therefore {{\lambda }_{\min }}=915\text{ }\overset{\circ }{\mathop{\text{A}}}\, \\\ \end{aligned}

Hence the correct option is CC.

Additional information:
The formula used in the question i.e., the Rydberg’s formula is only applicable when hydrogen-like atoms are used to emit the light for various transitions which means that the atoms must have only one valence electron in their valence shell so that we may use Rydberg’s formula for it. The term 1/λ1/\lambda as stated in the formula is known as the wavenumber as a whole where λ\lambda is the wavelength of the light.

Note:
The term RH{{R}_{H}} is the Rydberg constant whose value is 109678109678. The formula that we used to solve the question is known as the Rydberg’s formula which helps us determine the wavelength of the emitted light for various transitions between the orbits.