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Calculate the wavelength of the first line in the Balmer series of hydrogen spectrum.

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To calculate the wavelength of the first line in the Balmer series of the hydrogen spectrum, we can follow these steps: ### Step 1: Understand the Balmer Series The Balmer series corresponds to electron transitions in hydrogen where the final energy level (n_l) is 2. The first line in this series corresponds to the transition from n_h = 3 to n_l = 2. ### Step 2: Use the Rydberg Formula The Rydberg formula for calculating the wavelength (λ) of the emitted light is given by: \[ \frac{1}{\lambda} = R \cdot Z^2 \left( \frac{1}{n_l^2} - \frac{1}{n_h^2} \right) \] Where: - \( R \) is the Rydberg constant (approximately \( 1.097 \times 10^7 \, \text{m}^{-1} \) or \( 109678 \, \text{cm}^{-1} \)) - \( Z \) is the atomic number (for hydrogen, \( Z = 1 \)) - \( n_l \) is the lower energy level (2 for the Balmer series) - \( n_h \) is the higher energy level (3 for the first line in the Balmer series) ### Step 3: Substitute Values into the Formula Substituting the values into the Rydberg formula: \[ \frac{1}{\lambda} = 109678 \cdot 1^2 \left( \frac{1}{2^2} - \frac{1}{3^2} \right) \] Calculating the fractions: \[ \frac{1}{2^2} = \frac{1}{4} = 0.25 \] \[ \frac{1}{3^2} = \frac{1}{9} \approx 0.1111 \] Now, substituting these values back into the equation: \[ \frac{1}{\lambda} = 109678 \left( 0.25 - 0.1111 \right) \] \[ \frac{1}{\lambda} = 109678 \left( 0.1389 \right) \] \[ \frac{1}{\lambda} \approx 15287.78 \, \text{cm}^{-1} \] ### Step 4: Calculate Wavelength (λ) Now, take the reciprocal to find λ: \[ \lambda = \frac{1}{15287.78} \approx 0.0000654 \, \text{cm} \] ### Step 5: Convert to Angstroms To convert centimeters to angstroms (1 cm = \( 10^{10} \) angstroms): \[ \lambda \approx 0.0000654 \, \text{cm} \times 10^{10} \, \text{angstroms/cm} = 654 \, \text{angstroms} \] ### Final Answer The wavelength of the first line in the Balmer series of the hydrogen spectrum is approximately **6564 angstroms**. ---

To calculate the wavelength of the first line in the Balmer series of the hydrogen spectrum, we can follow these steps: ### Step 1: Understand the Balmer Series The Balmer series corresponds to electron transitions in hydrogen where the final energy level (n_l) is 2. The first line in this series corresponds to the transition from n_h = 3 to n_l = 2. ### Step 2: Use the Rydberg Formula The Rydberg formula for calculating the wavelength (λ) of the emitted light is given by: ...
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