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Line Emission Spectrum of Hydrogen

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Estimated time: 9 minutes
Maharashtra State Board: Class 12

Key Points: Line Emission Spectrum of Hydrogen

Emission vs. Absorption Spectrum

  • Emission spectrum: Formed when atoms emit radiation upon absorbing energy. Electrons jump to higher levels, then fall back, emitting photons. Arranged in increasing order of wavelength (decreasing frequency). \[\Delta E=E_{n_2}-E_{n_1},\] where n2 > n1​.

  • Absorption spectrum: Formed when atoms absorb specific wavelengths of radiation. Arranged in increasing order of wavelength. \[\Delta E=E_{n_2}-E_{n_1},\] where n2 < n1​.

Spectral Series of Hydrogen

Each series corresponds to electron transitions ending at a particular energy level:

 
Series Electron falls to (n₁) From levels (n₂) Region of Spectrum
Lyman n = 1 2, 3, 4, … Ultraviolet (UV)
Balmer n = 2 3, 4, 5, … Visible
Paschen n = 3 4, 5, 6, … Infrared (IR)
Brackett n = 4 5, 6, 7, … Infrared (IR)
Pfund n = 5 6, 7, 8, … Far Infrared
Maharashtra State Board: Class 12

Formula: Number of Emission Lines

When an electron jumps from level n2​ to level n1​:

\[\text{Number of emission lines}=\frac{(n_2-n_1)(n_2-n_1+1)}{2}\]

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