CHEM.PRINC.W/OWL2+REBATE+2 SUPPL.>IP<
CHEM.PRINC.W/OWL2+REBATE+2 SUPPL.>IP<
8th Edition
ISBN: 9781337496162
Author: ZUMDAHL
Publisher: CENGAGE L
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Chapter 12, Problem 39E

a)

Interpretation Introduction

Interpretation: The reason behind closer energy levels with higher states should be explained with mathematical concept.

Concept introduction: Salient characteristics of Bohr’s model are as follows:

Electron revolved in certain discrete circular orbits that were associated with fixed angular momentum.

Such discrete orbits are termed non-radiating or stationary orbits. The quantized energy for each of such discrete orbit can be obtained from the expression as follows:

  En=(RH)Z2n2

Where

  • RH is constant that has value of 2.178×1018 J .
  • Z represent atomic number.
  • n denotes particular stationary state.
  • En denotes energy associated with particular stationary state.

Energy absorption or emission only occurred when electron jumped from one energy sate to another hence each such probable unique transition gave rise to specific lines in emission spectrum of hydrogen atom. This was based on the relation as follows:

  ΔE=hΔv

Where

  • Δv is difference in frequency of two stationary states involved in transition.
  • ΔE denotes energy absorbed or emitted in transition.

a)

Expert Solution
Check Mark

Explanation of Solution

The quantized energy for each of such discrete orbit can be obtained from the expression as follows:

  En=(RH)Z2n2

This expression suggests En is inversely related to square of n . So higher the value of particular stationary state more is the energy associated with it. Hence for consecutive energy levels, the energy difference is almost minimal. So they begin to appear as continuum.

(b)

Interpretation Introduction

Interpretation: The colors depicted for transition between various energy levels should be verified.

Concept introduction: Salient characteristics of Bohr’s model are as follows:

Electron revolved in certain discrete circular orbits that were associated with fixed angular momentum.

Such discrete orbits are termed non-radiating or stationary orbits. The quantized energy for each of such discrete orbit can be obtained from the expression as follows:

  En=(RH)Z2n2

Where

  • RH is constant that has value of 2.178×1018 J .
  • Z represent atomic number.
  • n denotes particular stationary state.
  • En denotes energy associated with particular stationary state.

Hydrogen emission spectrum that shows characteristics lines could be accounted by the assumption made in Bohr’s model. Since energy absorption or emission only occurred when electron jumped from one energy sate to another hence each such probable unique transition gave rise to specific lines in emission spectrum of hydrogen atom. This was based on the relation as follows:

  ΔE=hΔv

Where

  • Δv is difference in frequency of two stationary states involved in transition.
  • ΔE denotes energy absorbed or emitted in transition.

(b)

Expert Solution
Check Mark

Explanation of Solution

The quantized energy for each of such discrete orbit can be obtained from the expression as follows:

  En=(RH)Z2n2

For n=3

Value of RH is 2.178×1018 J .

Value of Z for hydrogen atom is 1.

Substitute the values in above formula.

  E3=(RH)Z2n2=(2.178×1018 J)1(3)2

For n=2

Substitute the values in above formula.

  E2=(RH)Z2n2=(2.178×1018 J)1(2)2

Difference in theses energies gives energy for red color transition is calculated as follows:

  E3E2=(2.178×1018 J)[1(3)21(2)2]=3.025×1019 J

Similarly, energy for green color transition as follows:

  E4E2=(2.178×1018 J)[1(4)21(2)2]=4.083×1019 J

Likewise, energy for blue color transition as follows:

  E5E2=(2.178×1018 J)[1(5)21(2)2]=5.445×1019 J

Formula to compute wavelength from energy difference is given as follow:

  λ=hcΔE

Value of ΔE is 3.025×1019 J .

Value of h is 6.626×1034 J s .

Value of c is 3×108 m/s .

Substitute the value in above equation to calculate wavelength for red color.

  λ=hcΔE=(6.626×1034 J s)(3×108 m/s)(3.025×1019 J)=(6.571×107 m)(1 nm109 m)=657.1 nm

Corresponding wavelength is calculated as follows;

Value of ΔE is 3.025×1019 J .

Substitute the value in above equation to calculate wavelength for green color.

  λ=hcΔE=(6.626×1034 J s)(3×108 m/s)(4.083×1019 J)=(4.868×107 m)(1 nm109 m)=486.8 nm

Value of ΔE is 5.445×1019 J .

Substitute the value in above equation to calculate wavelength for blue color.

  λ=hcΔE=(6.626×1034 J s)(3×108 m/s)(5.445×1019 J)=(1.6528×107 m)(1 nm109 m)=165.28 nm

Since the wavelength for red, green and blue light also correspond to wavelength values of 657.1 nm

  486.8 nm and 165.28 nm therefore the colored lines depicted are correct.

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Chapter 12 Solutions

CHEM.PRINC.W/OWL2+REBATE+2 SUPPL.>IP<

Ch. 12 - Prob. 11DQCh. 12 - Prob. 12DQCh. 12 - Prob. 13DQCh. 12 - Prob. 14DQCh. 12 - Prob. 15DQCh. 12 - Prob. 16DQCh. 12 - Prob. 17DQCh. 12 - Is the following statement true or false: The...Ch. 12 - Which is higher in energy: the 2s or 2p orbital in...Ch. 12 - Prove mathematically that it is more energetically...Ch. 12 - Microwave radiation has a wavelength on the order...Ch. 12 - Consider the following waves representing...Ch. 12 - Prob. 23ECh. 12 - Human color vision is “produced” by the nervous...Ch. 12 - One type of electromagnetic radiation has a...Ch. 12 - Carbon absorbs energy at a wavelength of 150. nm....Ch. 12 - Prob. 27ECh. 12 - X rays have wavelengths on the order of 110-10m...Ch. 12 - The work function of an element is the energy...Ch. 12 - Ionization energy is the energy required to remove...Ch. 12 - It takes 208.4 kJ of energy to remove 1 mole of...Ch. 12 - What experimental evidence supports the quantum...Ch. 12 - Explain the photoelectric effect.Ch. 12 - Calculate the de Broglie wavelength for each of...Ch. 12 - Neutron diffraction is used in determining the...Ch. 12 - Calculate the velocities of electrons with de...Ch. 12 - An atom of a particular element is traveling at 1%...Ch. 12 - Characterize the Bohr model of the atom. 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The Bohr Model of the atom and Atomic Emission Spectra: Atomic Structure tutorial | Crash Chemistry; Author: Crash Chemistry Academy;https://www.youtube.com/watch?v=apuWi_Fbtys;License: Standard YouTube License, CC-BY