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This value is exactly the Rydberg constant R H in the Rydberg heuristic formula [link] . In fact, [link] is identical to the Rydberg formula, because for a given m , we have n = m + 1 , m + 2 , . . . . In this way, the Bohr quantum model of the hydrogen atom allows us to derive the experimental Rydberg constant from first principles and to express it in terms of fundamental constants. Transitions between the allowed electron orbits are illustrated in [link] .

We can repeat the same steps that led to [link] to obtain the wavelength of the absorbed radiation; this again gives [link] but this time for the positions of absorption lines in the absorption spectrum of hydrogen. The only difference is that for absorption, the quantum number m is the index of the orbit occupied by the electron before the transition (lower-energy orbit) and the quantum number n is the index of the orbit to which the electron makes the transition (higher-energy orbit). The difference between the electron energies in these two orbits is the energy of the absorbed photon.

Size and ionization energy of the hydrogen atom in an excited state

If a hydrogen atom in the ground state absorbs a 93.7-nm photon, corresponding to a transition line in the Lyman series, how does this affect the atom’s energy and size? How much energy is needed to ionize the atom when it is in this excited state? Give your answers in absolute units, and relative to the ground state.

Strategy

Before the absorption, the atom is in its ground state. This means that the electron transition takes place from the orbit m = 1 to some higher n th orbit. First, we must determine n for the absorbed wavelength λ = 93.7 nm . Then, we can use [link] to find the energy E n of the excited state and its ionization energy E , n , and use [link] to find the radius r n of the atom in the excited state. To estimate n , we use [link] .

Solution

Substitute m = 1 and λ = 93.7 nm in [link] and solve for n . You should not expect to obtain a perfect integer answer because of rounding errors, but your answer will be close to an integer, and you can estimate n by taking the integral part of your answer:

1 λ = R H ( 1 1 2 1 n 2 ) n = 1 1 1 λ R H = 1 1 1 ( 93.7 × 10 −9 m ) ( 1.097 × 10 7 m −1 ) = 6.07 n = 6 .

The radius of the n = 6 orbit is

r n = a 0 n 2 = a 0 6 2 = 36 a 0 = 36 ( 0.529 × 10 −10 m ) = 19.04 × 10 −10 m 19.0 Å .

Thus, after absorbing the 93.7-nm photon, the size of the hydrogen atom in the excited n = 6 state is 36 times larger than before the absorption, when the atom was in the ground state. The energy of the fifth excited state ( n = 6 ) is:

E n = E 0 n 2 = E 0 6 2 = E 0 36 = 13.6 eV 36 0.378 eV .

After absorbing the 93.7-nm photon, the energy of the hydrogen atom is larger than it was before the absorption. Ionization of the atom when it is in the fifth excited state ( n = 6 ) requites 36 times less energy than is needed when the atom is in the ground state:

E , 6 = E 6 = ( −0.378 eV ) = 0.378 eV .

Significance

We can analyze any spectral line in the spectrum of hydrogen in the same way. Thus, the experimental measurements of spectral lines provide us with information about the atomic structure of the hydrogen atom.

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Check Your Understanding When an electron in a hydrogen atom is in the first excited state, what prediction does the Bohr model give about its orbital speed and kinetic energy? What is the magnitude of its orbital angular momentum?

v 2 = 1.1 × 10 6 m / s 0.0036 c ; L 2 = 2 K 2 = 3.4 eV

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Source:  OpenStax, University physics volume 3. OpenStax CNX. Nov 04, 2016 Download for free at http://cnx.org/content/col12067/1.4
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