The Balmer series of hydrogen refers to the set of spectral lines corresponding to electron transitions from higher energy levels to the second energy level (n=2). The longest wavelength in this series occurs when the electron transitions from the third energy level (n=3) to the second energy level (n=2).
Calculating the Longest Wavelength
The formula to find the wavelength (λ) of the emitted light in the Balmer series is given by the Rydberg formula:
1/λ = R_H (1/n1² - 1/n2²)
Where:
- R_H is the Rydberg constant (approximately 1.097 x 107 m-1).
- n1 is the lower energy level (for Balmer series, n1 = 2).
- n2 is the higher energy level (for the longest wavelength, n2 = 3).
Plugging in the Values
Substituting the values into the formula:
1/λ = R_H (1/2² - 1/3²)
1/λ = 1.097 x 107 (1/4 - 1/9)
Calculating the fractions:
1/4 - 1/9 = 9/36 - 4/36 = 5/36
Now substituting back:
1/λ = 1.097 x 107 (5/36)
Finding the Wavelength
Now, calculate λ:
λ = 36/(1.097 x 107 x 5)
After performing the calculations, you will find:
λ ≈ 656.3 nm
Summary
The longest wavelength in the Balmer series of hydrogen is approximately 656.3 nanometers, which corresponds to the red color in the visible spectrum.