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Question: What is the wavelength of a photon emitted during a transition from \(n = 5\) state to \(n = 2\) sta...

What is the wavelength of a photon emitted during a transition from n=5n = 5 state to n=2n = 2 state in the hydrogen atom?
A. 434  nm434\;nm
B. 450  nm450\;nm
C. 350  nm350\;nm
D. 525  nm525\;nm

Explanation

Solution

Hint: The photon emitted during the transition from any state to n=2n = 2 state lies on Balmer series of transition. When there is a transition between the two states in a hydrogen atom, the relation between the number of the states and the wavelength is given by the Rydberg equation for hydrogen atom. By using that relation, the wavelength of the photon can be calculated.

Useful formula:
The Rydberg equation for hydrogen atom is given by,
1λ=RH[1n121n22]\dfrac{1}{\lambda } = {R_H}\left[ {\dfrac{1}{{{n_1}^2}} - \dfrac{1}{{{n_2}^2}}} \right]
Where, λ\lambda is the wavelength of the emitted photon, RH{R_H} is the Rydberg constant of hydrogen, n2{n_2} is the initial state of transition and n1{n_1} is the final state of transition.

Complete step by step solution:
Given, The final state of transition, n1=2{n_1} = 2
The initial state of transition, n2=5{n_2} = 5
The Rydberg constant of hydrogen, RH=10973731.6  m1{R_H} = 10973731.6\;{m^{ - 1}}

The Rydberg equation for hydrogen atom is given by,
1λ=RH[1n121n22]  .....................................(1)\dfrac{1}{\lambda } = {R_H}\left[ {\dfrac{1}{{{n_1}^2}} - \dfrac{1}{{{n_2}^2}}} \right]\;.....................................\left( 1 \right)
Substitute the given values of n1{n_1}, n2{n_2} and RH{R_H} in the equation (1),
1λ=10973731.6  m1[122152] 1λ=10973731.6[14125] 1λ=10973731.6[0.250.04] 1λ=10973731.6[0.21] 1λ=2304483.636  m1   \dfrac{1}{\lambda } = 10973731.6\;{m^{ - 1}}\left[ {\dfrac{1}{{{2^2}}} - \dfrac{1}{{{5^2}}}} \right] \\\ \dfrac{1}{\lambda } = 10973731.6\left[ {\dfrac{1}{4} - \dfrac{1}{{25}}} \right] \\\ \dfrac{1}{\lambda } = 10973731.6\left[ {0.25 - 0.04} \right] \\\ \dfrac{1}{\lambda } = 10973731.6\left[ {0.21} \right] \\\ \dfrac{1}{\lambda } = 2304483.636\;{m^{ - 1}} \\\ \\\
Taking reciprocal on both sides,
λ=12304483.636  m1 λ=4.3393×107  m  \lambda = \dfrac{1}{{2304483.636\;{m^{ - 1}}}} \\\ \lambda = 4.3393 \times {10^{ - 7}}\;m \\\
Convert unit from mm to nmnm,
1  m=109  nm1\;m = {10^9}\;nm
Hence,
λ=4.3393×107  m  ×109  nm1  m λ=4.3393×102  nm λ=433.93  nm λ434  nm  \lambda = 4.3393 \times {10^{ - 7}}\;m\; \times \dfrac{{{{10}^9}\;nm}}{{1\;m}} \\\ \lambda = 4.3393 \times {10^2}\;nm \\\ \lambda = 433.93\;nm \\\ \lambda \simeq 434\;nm \\\
Hence, the wavelength of photon emitted during transition, λ=434  nm\lambda = 434\;nm

Thus, the option (A) is correct.

NOTE:
Alternative method:
Hint: The energy level of photons in each level are calculated by using the energy formula for each state. Then the difference in the energy is obtained by taking the difference between two energies. And by using the Planck-Einstein relation the frequency of the emitted photon can be calculated and with the help of the relation between speed of light, wavelength and frequency of light, the wavelength can be obtained.

Useful formula:
The energy of hydrogen in each state is given by,
En=13.6  eVn2  Joules{E_n} = - \dfrac{{13.6\;eV}}{{{n^2}}}\;Joules
Where, 13.6  eV - 13.6\;eV is the approximate ground state energy of the hydrogen atom and nn is the state.
The Planck-Einstein relation is given by,
E=h×υE = h \times \upsilon
Where, EE is the energy difference, hh is the Planck’s constant and υ\upsilon is the frequency of the photon.
The relation between speed of light, wavelength and frequency of light is given by,
c=λ×υc = \lambda \times \upsilon
Where, cc is the speed of photon or light, λ\lambda is the wavelength of photon and υ\upsilon is the frequency of photon.

Complete step by step solution:
Given, The final state of transition, n1=2{n_1} = 2
The initial state of transition, n2=5{n_2} = 5
Planck’s constant, h=6.626×1034  J.sh = 6.626 \times {10^{ - 34}}\;J.s
Speed of photon, c=3×108  msc = 3 \times {10^8}\;\dfrac{m}{s}
Step by step solution:
The energy of hydrogen in n=5n = 5 state,
E5=13.6  eV52 E5=13.625 E5=0.544  eV  {E_5} = - \dfrac{{13.6\;eV}}{{{5^2}}} \\\ {E_5} = - \dfrac{{13.6}}{{25}} \\\ {E_5} = - 0.544\;eV \\\
Convert eVeV to JJ,
1  eV=1.602×1019  J1\;eV = 1.602 \times {10^{ - 19}}\;J
Hence,
E5=0.544×1.602×1019  J E5=0.871×1019  J E5=8.71×1020  J  {E_5} = - 0.544 \times 1.602 \times {10^{ - 19}}\;J \\\ {E_5} = - 0.871 \times {10^{ - 19}}\;J \\\ {E_5} = - 8.71 \times {10^{ - 20}}\;J \\\
The energy of hydrogen in n=2n = 2 state,
E2=13.6  eV22 E2=13.64 E2=3.4  eV  {E_2} = - \dfrac{{13.6\;eV}}{{{2^2}}} \\\ {E_2} = - \dfrac{{13.6}}{4} \\\ {E_2} = - 3.4\;eV \\\
Convert eVeV to JJ,
1  eV=1.602×1019  J1\;eV = 1.602 \times {10^{ - 19}}\;J
Hence,
E2=3.4×1.602×1019  J E2=5.44×1019  J  {E_2} = - 3.4 \times 1.602 \times {10^{ - 19}}\;J \\\ {E_2} = - 5.44 \times {10^{ - 19}}\;J \\\
Difference in energy between n=5n = 5 state and n=2n = 2 state,
ΔE=E2E5  ...............................(2)\Delta E = {E_2} - {E_5}\;...............................\left( 2 \right)
Substitute the values of E2{E_2} and E5{E_5} in equation (2),
ΔE=(5.44×1019  J)(8.71×1020  J) ΔE=4.57×1019  J  \Delta E = \left( { - 5.44 \times {{10}^{ - 19}}\;J} \right) - \left( { - 8.71 \times {{10}^{ - 20}}\;J} \right) \\\ \Delta E = 4.57 \times {10^{ - 19}}\;J \\\
The Planck-Einstein relation is given by,
ΔE=h×υ  ...........................(3)\Delta E = h \times \upsilon \;...........................\left( 3 \right)
Substitute the values of ΔE\Delta E, hh and υ\upsilon in equation (3),
4.57×1019  J=6.626×1034  Js  ×υ υ=4.57×1019  J6.626×1034  Js υ=6.897×1014  s1  4.57 \times {10^{ - 19}}\;J = 6.626 \times {10^{ - 34}}\;Js\; \times \upsilon \\\ \upsilon = \dfrac{{4.57 \times {{10}^{ - 19}}\;J}}{{6.626 \times {{10}^{ - 34}}\;Js}} \\\ \upsilon = 6.897 \times {10^{14}}\;{s^{ - 1}} \\\
The relation between speed of light, wavelength and frequency of light is given by,
c=λ×υ  .................................(4)c = \lambda \times \upsilon \;.................................\left( 4 \right)
Substitute the values of ccand υ\upsilon in equation (4),
3×108  ms1=λ×6.897×1014  s1 λ=3.8×108  ms16.897×1014  s1 λ=4.354×107  m  3 \times {10^8}\;m{s^{ - 1}} = \lambda \times 6.897 \times {10^{14}}\;{s^{ - 1}} \\\ \lambda = \dfrac{{3.8 \times {{10}^8}\;m{s^1}}}{{6.897 \times {{10}^{14}}\;{s^{ - 1}}}} \\\ \lambda = 4.354 \times {10^{ - 7}}\;m \\\
Convert unit from mm to nmnm,
1  m=109  nm1\;m = {10^9}\;nm
Hence,
λ=4.35×107  m  ×109  nm1  m λ=4.35×102  nm λ=435  nm λ434  nm  \lambda = 4.35 \times {10^{ - 7}}\;m\; \times \dfrac{{{{10}^9}\;nm}}{{1\;m}} \\\ \lambda = 4.35 \times {10^2}\;nm \\\ \lambda = 435\;nm \\\ \lambda \simeq 434\;nm \\\

Hence, the option (A) is correct.

These two methods are used to find the wavelength of the photon emitted from one state to another state. In the first method the Rydberg equation is directly used to find the wavelength and in the second method, the energy equation, Planck-Einstein equation and relation between speed, wavelength and frequency of photon are used. Bothe these methods give the approximate answer of wavelength.