NVAEasyJEE 2023Bohr Model & Hydrogen Spectrum

JEE Chemistry 2023 Question with Solution

The electron in the nnth orbit of Li2+^{2+} is excited to (n+1)(n + 1)th orbit using the radiation of energy 1.47×1017J1.47 \times 10^{-17} \, \text{J}. The value of nn is _____.

% Given Given: RH=2.18×1018JR_H = 2.18 \times 10^{-18} \, J

Answer

Correct answer:1

Step-by-step solution

Standard Method

Given: electron in Li2+^{2+} is excited from nn to (n+1)(n+1) using radiation of energy 1.47×1017J1.47 \times 10^{-17} \, \text{J}.

Find: the value of nn.

For a hydrogen-like species, the energy difference between two orbits is

ΔE=RHZ2(1n121n22)\Delta E = R_H Z^2 \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right)

For Li2+^{2+}, Z=3Z = 3. Here the transition is from nn to (n+1)(n+1), so

ΔE=RH×9(1n21(n+1)2)\Delta E = R_H \times 9 \left( \frac{1}{n^2} - \frac{1}{(n+1)^2} \right)

Substituting the given values,

1.47×1017=2.18×1018×9(1n21(n+1)2)1.47 \times 10^{-17} = 2.18 \times 10^{-18} \times 9 \left( \frac{1}{n^2} - \frac{1}{(n+1)^2} \right)

Since 2.18×9=19.622.18 \times 9 = 19.62, this gives

1.47×1017=1.962×1017(1n21(n+1)2)1.47 \times 10^{-17} = 1.962 \times 10^{-17} \left( \frac{1}{n^2} - \frac{1}{(n+1)^2} \right)

So,

1.471.96=34=1n21(n+1)2\frac{1.47}{1.96} = \frac{3}{4} = \frac{1}{n^2} - \frac{1}{(n+1)^2}

Now testing n=1n = 1,

112122=114=34\frac{1}{1^2} - \frac{1}{2^2} = 1 - \frac{1}{4} = \frac{3}{4}

This satisfies the equation.

Therefore, the value of nn is 11.

Quick Check

Given: 1n21(n+1)2=34\frac{1}{n^2} - \frac{1}{(n+1)^2} = \frac{3}{4}.

Find: nn.

Check the smallest integer value first:

n=1n = 1

Then

112122=114=34\frac{1}{1^2} - \frac{1}{2^2} = 1 - \frac{1}{4} = \frac{3}{4}

This matches immediately.

Therefore, the correct value is 11.

Common mistakes

  • Using Z=1Z = 1 instead of Z=3Z = 3 for Li2+^{2+}. Li2+^{2+} is a hydrogen-like ion with nuclear charge 33, so the energy expression must contain Z2=9Z^2 = 9. Always identify the atomic number before substitution.

  • Writing the transition energy with the levels reversed. For excitation from lower to higher orbit, use the magnitude of the energy difference between nn and (n+1)(n+1) correctly. Do not treat the absorbed radiation energy as negative here.

  • Forgetting that the final orbit is (n+1)(n+1), not a separate unknown unrelated to nn. Substitute the levels as n1=nn_1 = n and n2=n+1n_2 = n+1 before solving.

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