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Hydrogen Atom and Hydrogen Molecule Th...

Hydrogen Atom and Hydrogen Molecule
The observed wavelengths in the line spectrum of hydrogen atom were first expressed in terms of a series by johann Jakob Balmer, a Swiss teacher. Balmer's empirical empirical formula is
`1/lambda=R_(H)(1/2^(2)-1/n^(2))," " N=3, 4, 5`
`R_(H)=(Me e^(4))/(8 epsilon_(0)^(2)h^(3) c)=109. 678 cm^(-1)`
Here,
`R_(H)` is the Rydberg Constant, `m_(e)` is the mass of electron. Niels Bohr derived this expression theoretically in 1913. The formula is easily generalized to any one electron atom//ion.
Calculate the iongest wavelength in `A (1 Å=10^(-10) m)` in the 'Balmer series of singly ionized helium `(He^(+))` Ignore nuclear motion in your calculation.

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To solve the problem of calculating the longest wavelength in the Balmer series of singly ionized helium (He⁺), we will follow these steps: ### Step 1: Understand the Formula The formula given for the wavelength (λ) in the Balmer series is: \[ \frac{1}{\lambda} = R_H \cdot Z^2 \left( \frac{1}{2^2} - \frac{1}{n^2} \right) \] Where: - \( R_H \) is the Rydberg constant for hydrogen, which is \( 109.678 \, \text{cm}^{-1} \). - \( Z \) is the atomic number of the ion (for He⁺, \( Z = 2 \)). - \( n \) is the principal quantum number, which takes values \( n = 3, 4, 5, \ldots \) for the Balmer series. ### Step 2: Identify the Longest Wavelength To find the longest wavelength, we need to minimize the term \( \frac{1}{n^2} \). The smallest value of \( n \) in the Balmer series is \( n = 3 \). ### Step 3: Substitute Values into the Formula Now we substitute \( Z = 2 \) and \( n = 3 \) into the formula: \[ \frac{1}{\lambda} = R_H \cdot Z^2 \left( \frac{1}{2^2} - \frac{1}{3^2} \right) \] Calculating the terms: - \( R_H = 109.678 \, \text{cm}^{-1} \) - \( Z^2 = 2^2 = 4 \) - \( \frac{1}{2^2} = \frac{1}{4} \) - \( \frac{1}{3^2} = \frac{1}{9} \) Now, calculate \( \frac{1}{4} - \frac{1}{9} \): \[ \frac{1}{4} - \frac{1}{9} = \frac{9 - 4}{36} = \frac{5}{36} \] ### Step 4: Plug in the Values Now substituting back into the equation: \[ \frac{1}{\lambda} = 109.678 \cdot 4 \cdot \frac{5}{36} \] Calculating this step-by-step: 1. \( 4 \cdot \frac{5}{36} = \frac{20}{36} = \frac{5}{9} \) 2. Now multiply by \( R_H \): \[ \frac{1}{\lambda} = 109.678 \cdot \frac{5}{9} \] 3. Calculate \( 109.678 \cdot \frac{5}{9} \): \[ \frac{1}{\lambda} \approx 60.932 \, \text{cm}^{-1} \] ### Step 5: Calculate λ Now, take the reciprocal to find λ: \[ \lambda = \frac{1}{60.932} \approx 0.0164 \, \text{cm} \] ### Step 6: Convert to Angstroms Since \( 1 \, \text{cm} = 10^{10} \, \text{Å} \): \[ \lambda \approx 0.0164 \, \text{cm} \times 10^{10} \, \text{Å/cm} = 1641.6 \, \text{Å} \] ### Final Answer The longest wavelength in the Balmer series of singly ionized helium (He⁺) is approximately: \[ \lambda \approx 1641.6 \, \text{Å} \] ---
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