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Calculate Wavelength of Second Balmer Line in Singly Ionized Helium

The wavelength of the first spectral line in the Balmer series of hydrogen atom is 6561 A˚6561\text{ \AA}. The wavelength of the second spectral line in the Balmer series of singly-ionized helium atom is

Options

A

1215 A˚1215\text{ \AA}

Correct
B

1640 A˚1640\text{ \AA}

C

2430 A˚2430\text{ \AA}

D

4687 A˚4687\text{ \AA}

Topics & Concepts

Step-by-Step Solution

To determine the wavelength of the second spectral line in the Balmer series of a singly-ionized helium atom (He+\text{He}^+), we use the Rydberg formula for hydrogen-like species:

1λ=RZ2(1n12−1n22)\frac{1}{\lambda} = R Z^2 \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right)

where:

  • RR is the Rydberg constant,
  • ZZ is the atomic number of the atom,
  • n1n_1 and n2n_2 are the principal quantum numbers of the lower and higher energy levels, respectively.

Step 1: First spectral line in the Balmer series of the Hydrogen atom (HH)

For hydrogen, the atomic number is ZH=1Z_{\text{H}} = 1. The Balmer series corresponds to transitions ending at n1=2n_1 = 2. The first line of the Balmer series corresponds to a transition from n2=3n_2 = 3 to n1=2n_1 = 2.

Given:

  • λH,1=6561 A˚\lambda_{\text{H}, 1} = 6561 \text{ \AA}

Applying the Rydberg formula:
1λH,1=R(1)2(122−132)\frac{1}{\lambda_{\text{H}, 1}} = R (1)^2 \left( \frac{1}{2^2} - \frac{1}{3^2} \right)

16561=R(14−19)=R(536)\frac{1}{6561} = R \left( \frac{1}{4} - \frac{1}{9} \right) = R \left( \frac{5}{36} \right)

Solving for RR:
R=365×6561 A˚−1R = \frac{36}{5 \times 6561} \text{ \AA}^{-1}


Step 2: Second spectral line in the Balmer series of singly-ionized Helium (He+\text{He}^+)

For singly-ionized helium, the atomic number is ZHe=2Z_{\text{He}} = 2. The second line in the Balmer series corresponds to a transition from n2=4n_2 = 4 to n1=2n_1 = 2.

Applying the Rydberg formula:
1λHe,2=R(2)2(122−142)\frac{1}{\lambda_{\text{He}, 2}} = R (2)^2 \left( \frac{1}{2^2} - \frac{1}{4^2} \right)

1λHe,2=4R(14−116)=4R(316)=3R4\frac{1}{\lambda_{\text{He}, 2}} = 4R \left( \frac{1}{4} - \frac{1}{16} \right) = 4R \left( \frac{3}{16} \right) = \frac{3R}{4}

Taking the reciprocal gives:
λHe,2=43R\lambda_{\text{He}, 2} = \frac{4}{3R}


Step 3: Calculation

Substitute the value of RR into the expression for λHe,2\lambda_{\text{He}, 2}:

λHe,2=43×(365×6561)=4×5×65613×36\lambda_{\text{He}, 2} = \frac{4}{3 \times \left( \frac{36}{5 \times 6561} \right)} = \frac{4 \times 5 \times 6561}{3 \times 36}

λHe,2=20×6561108\lambda_{\text{He}, 2} = \frac{20 \times 6561}{108}

Simplifying the fraction:
6561108=2434=60.75\frac{6561}{108} = \frac{243}{4} = 60.75

λHe,2=20×60.75=1215 A˚\lambda_{\text{He}, 2} = 20 \times 60.75 = 1215 \text{ \AA}

Thus, the wavelength of the second spectral line in the Balmer series of a singly-ionized helium atom is 1215 A˚1215\text{ \AA}.

Correct Answer: A