The Rydberg formula is a powerful tool for calculating the wavelengths of spectral lines in hydrogen. The formula is given by:
Rydberg Formula
The formula is expressed as:
1/λ = R_H (1/n1² - 1/n2²)
Where:
- λ = wavelength of the emitted light
- R_H = Rydberg constant (approximately 1.097 x 10^7 m^-1)
- n1 = lower energy level (for Lyman series, n1 = 1)
- n2 = higher energy level (n2 = 2, 3, 4, ...)
Calculating Wavelengths for the Lyman Series
For the Lyman series, the transitions occur from higher energy levels down to n1 = 1. The first four lines correspond to:
- Transition from n2 = 2 to n1 = 1
- Transition from n2 = 3 to n1 = 1
- Transition from n2 = 4 to n1 = 1
- Transition from n2 = 5 to n1 = 1
Calculations
Now, let’s calculate the wavelengths:
1. For n2 = 2
1/λ = R_H (1/1² - 1/2²)
1/λ = 1.097 x 10^7 (1 - 1/4) = 1.097 x 10^7 (3/4)
λ = 4.86 x 10^-7 m or 486 nm
2. For n2 = 3
1/λ = R_H (1/1² - 1/3²)
1/λ = 1.097 x 10^7 (1 - 1/9) = 1.097 x 10^7 (8/9)
λ = 3.66 x 10^-7 m or 366 nm
3. For n2 = 4
1/λ = R_H (1/1² - 1/4²)
1/λ = 1.097 x 10^7 (1 - 1/16) = 1.097 x 10^7 (15/16)
λ = 2.73 x 10^-7 m or 273 nm
4. For n2 = 5
1/λ = R_H (1/1² - 1/5²)
1/λ = 1.097 x 10^7 (1 - 1/25) = 1.097 x 10^7 (24/25)
λ = 2.18 x 10^-7 m or 218 nm
Summary of Wavelengths
The wavelengths of the first four spectral lines in the Lyman series are:
- n2 = 2: 486 nm
- n2 = 3: 366 nm
- n2 = 4: 273 nm
- n2 = 5: 218 nm
These wavelengths correspond to the ultraviolet region of the electromagnetic spectrum.