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9 - N u m e r i c a l   4

Problem

The series limit wavelength of the Balmer series is emitted as the electron in the hydrogen atom falls from n=n = \infty to n=2n = 2. What is the wavelength of this line if ΔE=3.040eV\Delta E = 3.040 \, \mathrm{eV}?

Data

  • Energy Difference ΔE\Delta E: 3.040eV3.040 \, \mathrm{eV}
  • Energy Level nn: \infty
  • Energy Level pp: 22
  • Rydberg Constant RHR_H: 1.0974×107m11.0974 \times 10^{7} \, \mathrm{m}^{-1}

To find:

  • Wavelength λ\lambda

Prerequisite Concepts

  1. Balmer Series Formula:
    The wavelength of emitted photons in the Balmer series is given by:
1λ=RH(1p21n2) \frac{1}{\lambda} = R_H \left( \frac{1}{p^2} - \frac{1}{n^2} \right)

Where:

  • RHR_H: Rydberg constant
  • pp: Lower energy level
  • nn: Higher energy level (n>pn > p)
  1. Series Limit Wavelength:
    The shortest wavelength in the Balmer series corresponds to n=n = \infty, where 1n20\frac{1}{n^2} \to 0.

  2. Units Conversion:
    Convert the result to nanometers (nm\mathrm{nm}) for standard interpretation.

Solution

Step 1: Write the general formula

1λ=RH(1p21n2)\frac{1}{\lambda} = R_H \left( \frac{1}{p^2} - \frac{1}{n^2} \right)

Step 2: Substitute the given values

Substitute RH=1.0974×107m1R_H = 1.0974 \times 10^{7} \, \mathrm{m}^{-1}, p=2p = 2, and n=n = \infty:

1λ=1.0974×107(12212)\frac{1}{\lambda} = 1.0974 \times 10^{7} \left( \frac{1}{2^2} - \frac{1}{\infty^2} \right)

Step 3: Simplify the expression

Since 12=0\frac{1}{\infty^2} = 0:

1λ=1.0974×107(140)\frac{1}{\lambda} = 1.0974 \times 10^{7} \left( \frac{1}{4} - 0 \right) 1λ=1.0974×1070.25\frac{1}{\lambda} = 1.0974 \times 10^{7} \cdot 0.25 1λ=0.27435×107m1\frac{1}{\lambda} = 0.27435 \times 10^{7} \, \mathrm{m}^{-1}

Step 4: Calculate λ\lambda

λ=10.27435×107m\lambda = \frac{1}{0.27435 \times 10^{7}} \, \mathrm{m} λ=3.644979×107m\lambda = 3.644979 \times 10^{-7} \, \mathrm{m}

Step 5: Convert to nanometers

λ=364.49nm\lambda = 364.49 \, \mathrm{nm}

Answer

The wavelength of the Balmer series limit line is:

λ=364.49nm\lambda = 364.49 \, \mathrm{nm}