The wavelength of light emitted in a transition from the first excited state in which the ionization energy is 126 kJ/mol to the ground state in which the ionization energy is 412 kJ/mol should be calculated using the concept of Bohr’s theory. Concept Introduction: The emission of radiation given by an energized hydrogen atom to the electron falling from a higher-energy orbit to a lower orbit give a quantum of energy in the form of light. Based on electrostatic interaction and law of motion, Bohr derived the following equation. E n = − 2 .18 × 10 − 18 J ( 1 n 2 ) where n gets an integer values such as n = 1, 2, 3 and so on. This is the energy of electron in n th orbital. The electrons are excited thermally when the light is used by an object. As a result, an emission spectrum comes. Line spectra consist of light only at specific, discrete wavelengths. In emission, the electron returns to a lower energy state from n f (the i and f subscripts denote the initial and final energy states). In most cases, the lower energy state corresponds to the ground state but it may be any energy state which is lower than the initial excited state. The difference in the energies between the initial and final states is ΔE = E f − E i This transition results in the photon’s emission with frequency v and energy hv . The following equation is resulted. ΔE = hν = − 2 .18 × 10 − 18 J ( 1 n f 2 − 1 n i 2 ) When n i > n f , a photon is emitted. The term in parentheses is positive, making ΔE negative . As a result, energy is lost to the surroundings. When n i < n f , a photon is absorbed. The term in parentheses is negative, so ΔE is positive. As a result, energy is absorbed from the surroundings. To find: The wavelength of light emitted in a transition from the first excited state in which the ionization energy is 126 kJ/mol to the ground state in which the ionization energy is 412 kJ/mol
The wavelength of light emitted in a transition from the first excited state in which the ionization energy is 126 kJ/mol to the ground state in which the ionization energy is 412 kJ/mol should be calculated using the concept of Bohr’s theory. Concept Introduction: The emission of radiation given by an energized hydrogen atom to the electron falling from a higher-energy orbit to a lower orbit give a quantum of energy in the form of light. Based on electrostatic interaction and law of motion, Bohr derived the following equation. E n = − 2 .18 × 10 − 18 J ( 1 n 2 ) where n gets an integer values such as n = 1, 2, 3 and so on. This is the energy of electron in n th orbital. The electrons are excited thermally when the light is used by an object. As a result, an emission spectrum comes. Line spectra consist of light only at specific, discrete wavelengths. In emission, the electron returns to a lower energy state from n f (the i and f subscripts denote the initial and final energy states). In most cases, the lower energy state corresponds to the ground state but it may be any energy state which is lower than the initial excited state. The difference in the energies between the initial and final states is ΔE = E f − E i This transition results in the photon’s emission with frequency v and energy hv . The following equation is resulted. ΔE = hν = − 2 .18 × 10 − 18 J ( 1 n f 2 − 1 n i 2 ) When n i > n f , a photon is emitted. The term in parentheses is positive, making ΔE negative . As a result, energy is lost to the surroundings. When n i < n f , a photon is absorbed. The term in parentheses is negative, so ΔE is positive. As a result, energy is absorbed from the surroundings. To find: The wavelength of light emitted in a transition from the first excited state in which the ionization energy is 126 kJ/mol to the ground state in which the ionization energy is 412 kJ/mol
Solution Summary: The author explains that the wavelength of light emitted in a transition from the first excited state to the ground state should be calculated using the concept of Bohr's theory.
The wavelength of light emitted in a transition from the first excited state in which the ionization energy is 126 kJ/mol to the ground state in which the ionization energy is 412 kJ/mol should be calculated using the concept of Bohr’s theory.
Concept Introduction:
The emission of radiation given by an energized hydrogen atom to the electron falling from a higher-energy orbit to a lower orbit give a quantum of energy in the form of light. Based on electrostatic interaction and law of motion, Bohr derived the following equation.
En=−2.18 × 10−18 J (1n2)
where n gets an integer values such as n = 1, 2, 3 and so on. This is the energy of electron in nth orbital.
The electrons are excited thermally when the light is used by an object. As a result, an emission spectrum comes. Line spectra consist of light only at specific, discrete wavelengths. In emission, the electron returns to a lower energy state from nf (the i and f subscripts denote the initial and final energy states). In most cases, the lower energy state corresponds to the ground state but it may be any energy state which is lower than the initial excited state. The difference in the energies between the initial and final states is
ΔE = Ef− Ei
This transition results in the photon’s emission with frequency v and energy hv. The following equation is resulted.
ΔE = hν =−2.18 × 10−18 J (1nf2−1ni2)
When ni > nf, a photon is emitted. The term in parentheses is positive, making ΔE negative. As a result, energy is lost to the surroundings. When ni < nf, a photon is absorbed. The term in parentheses is negative, so ΔE is positive. As a result, energy is absorbed from the surroundings.
To find: The wavelength of light emitted in a transition from the first excited state in which the ionization energy is 126 kJ/mol to the ground state in which the ionization energy is 412 kJ/mol
Г
C-RSA CHROMATOPAC CH=1
DATA 1: @CHRM1.C00
ATTEN=10 SPEED= 10.0
0.0 b.092
0.797
1.088
1.813
C-RSA CHROMATOPAC CH=1 Report No. =13
** CALCULATION REPORT **
DATA=1: @CHRM1.000 11/03/05 08:09:52
CH PKNO
TIME
1
2
0.797
3
1.088
4
1.813
AREA
1508566
4625442
2180060
HEIGHT
207739
701206 V
287554 V
MK IDNO
CONC
NAME
18.1447
55.6339
26.2213
TOTAL
8314067 1196500
100
C-R8A CHROMATOPAC CH=1
DATA 1: @CHRM1.C00
ATTEN=10 SPEED= 10.0
0. 0
087
337.
0.841
1.150
C-R8A CHROMATOPAC CH=1 Report No. =14
DATA=1: @CHRM1.000 11/03/05 08:12:40
** CALCULATION REPORT **
CH PKNO
TIME
AREA
1
3 0.841
1099933
41.15
4039778
HEIGHT MK IDNO
170372
649997¯¯¯
CONC
NAME
21.4007
78.5993
TOTAL
5139711 820369
100
3
C-R8A CHROMATOPAC
CH=1
DATA 1: @CHRM1.C00
ATTEN=10 SPEED= 10.0
0.100
0:652
5.856
3
1.165
C-RSA CHROMATOPAC CH-1 Report No. =15
DATA=1: @CHRM1.000 11/03/05 08:15:26
** CALCULATION REPORT **
CH PKNO TIME
AREA
HEIGHT MK IDNO CONC
NAME
1 3 3 0.856
4
1.165
TOTAL
1253386
4838738
175481
708024 V
20.5739
79.4261
6092124…
Draw the product of the reaction shown below. Ignore small byproducts that would evaporate please.
Relative Abundance
20-
Problems
501
(b) The infrared spectrum has a medium-intensity peak at about 1650 cm. There is also a
C-H out-of-plane bending peak near 880 cm.
100-
80-
56
41
69
M(84)
LL
15 20 25
30
35
55 60 65 70
75
80
85 90
m/z
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