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Find the wavelenght of the first line of...

Find the wavelenght of the first line of `He^(+)`ion sepectral series whose interval between extreme line is
`[(1)/(lambda)-(1)/(lambda)=2.745xx10^(4)cm^(1)]`

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To find the wavelength of the first line of the `He^(+)` ion spectral series, we can use the formula for the wavelength of spectral lines in hydrogen-like atoms, which is given by the Rydberg formula: \[ \frac{1}{\lambda} = RZ^2 \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right) \] Where: - \( R \) is the Rydberg constant (\( R = 1.097 \times 10^7 \, \text{m}^{-1} \)) - \( Z \) is the atomic number (for He, \( Z = 2 \)) - \( n_1 \) is the lower energy level - \( n_2 \) is the higher energy level ### Step 1: Identify the values of \( n_1 \) and \( n_2 \) For the first line of the spectral series, we typically take \( n_1 = 1 \) (ground state) and \( n_2 = 2 \) (first excited state). ### Step 2: Substitute the values into the Rydberg formula Now, substituting \( R \), \( Z \), \( n_1 \), and \( n_2 \) into the Rydberg formula: \[ \frac{1}{\lambda} = RZ^2 \left( \frac{1}{1^2} - \frac{1}{2^2} \right) \] Calculating the right-hand side: \[ \frac{1}{\lambda} = (1.097 \times 10^7) \cdot (2^2) \left( 1 - \frac{1}{4} \right) \] \[ = (1.097 \times 10^7) \cdot 4 \left( \frac{3}{4} \right) \] \[ = (1.097 \times 10^7) \cdot 3 \] \[ = 3.291 \times 10^7 \, \text{m}^{-1} \] ### Step 3: Calculate \( \lambda \) Now, we can find \( \lambda \) by taking the reciprocal: \[ \lambda = \frac{1}{3.291 \times 10^7} \, \text{m} \] Calculating \( \lambda \): \[ \lambda \approx 3.04 \times 10^{-8} \, \text{m} \] To convert this to centimeters: \[ \lambda \approx 3.04 \times 10^{-8} \, \text{m} \times 100 \, \text{cm/m} = 3.04 \times 10^{-6} \, \text{cm} \] ### Step 4: Final Result Thus, the wavelength of the first line of the `He^(+)` ion spectral series is approximately: \[ \lambda \approx 3.04 \times 10^{-6} \, \text{cm} \]

To find the wavelength of the first line of the `He^(+)` ion spectral series, we can use the formula for the wavelength of spectral lines in hydrogen-like atoms, which is given by the Rydberg formula: \[ \frac{1}{\lambda} = RZ^2 \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right) \] Where: - \( R \) is the Rydberg constant (\( R = 1.097 \times 10^7 \, \text{m}^{-1} \)) ...
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