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Hydrogen Spectra

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Hydrogen Spectra

Hydrogen, the simplest but the most abundant element in the universe is also the most studied element. During the early development of science, people have been investigating light emitted by a heated tubes of hydrogen gas. When these lights passes prisms, they saw some lines in the visible region.

The picture shown here is a brilliant star taken by the Hubble telescope exploring the universe. This brilliant star may be one of the largest mass of hydrogen.

Hydrogen spectrum in the visible region

When a hydrogen gas is heated or excited by electric means, the visible spectrum consists of lines. The wavelengths (wl) of these lines are given below: wl     656 486 434 410 397 nm These lines are shown here together with lines emitted by hot gases of Hg and He. These lines are called the Balmer Series, because Balmer saw some regularity in their wavelength, and he has given a formula to show the regularity.

The Balmer Series

Do you see any regularity in the wavelength? Well, J.J. Balmer analyzed these lines and he gave the following relationship:

                n2
wl = 364.56 -------- nm
             n2 - 22
for the regularity in terms of integers n. For some integers of n, you can confirm the wl to be

  n =  3     4    5     6     7    8   9    10...
 wl = 656   486  434   410   397  389 383  380... nm
      red green blue indigo violet (not visible)

As the n increase, the lines are getting closer together. If you plot the lines according to their wl on a linear scale, you will get the apparence of a spectrum as observed by experimentalists.

For this reason, these lines are called the Balmer series.

The Rydberg Formula

Rydberg inverted both sides of Balmer's formula and gave

  1        1     1
 --- = RH (--  - --)
 wl        22    n2
This is known as the Rydberg formula, and R is known as the Rydberg constant, its numerical values depends on the units used RH = 0.010972 nm-1
  = 10972 mm-1
  = 109721 cm-1
  = 10972130 m-1

This formula shows that if you plot 1/wl as a function of 1/n2, you will get a straight line. The reciprocal of wl (1/wl) is the number of waves per unit length, and it is called the wavenumber.

Other Series

The results given by Balmer and Rydberg for the spectrum in the visible region of the electromagnetic radiation start with n = 3, and the other integer is 2.

Is there a series with the following formula?


  1        1     1
 --- = RH (--  - --)
 wl        12    n2
If the law of nature is simple and regular, a series should exist, and the values for n and wavenumber (wn) should be:

  n =   2      3      4     5    ...
 wl =  121    102     97    94      nm
 wn = 82291  97530 102864 105332 ...cm-1
Do you know in what region of the electromagnetic radiation these lines are? Of course, these lines are in the UV region, and they are not visible, but they are detected by instruments. These lines form a Lyman series.

A Generalized Rydberg Formula

Existences of the Lyman series and Balmer's series sugest the existance of more series, and a generalized formula is suggested.

           1       1
 wn = RH (---  -  ---)
          nf2      ni2
Actually, the series with nf2 = 3, and ni2 = 4, 5, 6, 7, ... is called Pashen series.

A SciTech Presentation of Hands-On-Atom provides some fun things to do regarding the hydrogen spectra. Click it to try out if you wish.

Confidence Building Questions

Spectra of Elements shows the spectra of elements in the periodic table.

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