20 · LIGHT AND SPECTROSCOPY
Experimentally, the emission spectrum of the hydrogen atom is obtained by pass-
ing an electric spark through a quartz tube containing hydrogen gas. The energy from
the spark dissociates some of the hydrogen molecules into atoms. Some of the dissoci-
ated hydrogen atoms have so much energy that they are in an excited electronic state.
Although many of these excited atoms lose their excess energy by collisions with
other atoms or molecules, some lose the radiation as light. The emission spectrum is
obtained by passing the emitted light through a spectrometer. Measurements of the
Lyman series must be made in equipment from which air has been evacuated. This is
because the emission lines appear in the range 90–120 nm and both nitrogen and
oxygen gases absorb UV radiation at these wavelengths.
The spectrum of the Lyman series, obtained using a photosensitive emulsion as
detector, is shown at the bottom of Fig. 20.7. For clarity, all emission lines are shown
as being of equal intensity.
Transitions that cause the Lyman series
The hydrogen atom contains only one electron. The electronic energy of a hydrogen
atom depends upon the orbital in which the electron is found. If the electron lies in
the lowest energy orbital (n= 1), the atom is in its ground electronic energy level (its
ground state). The energy of 1 mol of hydrogen atoms in this level is 1310 kJ. (A neg-
ative energy seems strange, but this is just a convention. It means that a stationary
electron just outside the attraction of the hydrogen nucleus will have zero energy.) If
the electron lies in higher orbitals (n> 1), the atom is in an excited electronic state
and its energy becomes bigger (i.e. less negative). At very high values of nthe energy
of 1 mol of hydrogen atoms approaches zero (see Fig. 20.7).
The transitions involved in the Lyman series involve hydrogen atoms in higher
electronic energy levels losing energy by emitting light so that the hydrogen atom ends
up in its ground state. We can represent these transitions as follows:
H(n> 1)→H(n= 1)+h
electronically ground state emitted
excited light
state
wherenin the excited state takes the values 2, 3, 4, 5 etc.
These transitions are shown by downward arrows in Fig. 20.7.
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Fig. 20.7Schematic diagram
of the transitions and the
observed spectral lines in the
Lyman series of the hydrogen
atom.