Calculate the wavelength in angstrom of the photon that is emitted when an electron in Bohr orbit n=2 returns to the orbit n=1 in the hydrogen atom. The ionization potential of the ground state of the hydrogen atom is \[2.17\times {{10}^{-11}}ergato{{m}^{-1}}\].
Answer
614.7k+ views
Hint: Bohr produces a set of postulates to explain the hydrogen atom. We know the energy difference between two energy levels is equal to the energy of a photon and its equation is given as $\Delta E=h\nu $ , where $\Delta E$ is the energy difference between two energy levels, h is the Planck’s constant and $\nu $ is the frequency.
Complete step by step solution:
In the question, we have to find the difference between two energy levels, which give the wavelength of the photon that is emitted. This is explained by using a formula called Rydberg formula.
\[E=R(\dfrac{1}{n_{f}^{2}}-\dfrac{1}{n_{i}^{2}})\] Here, \[n_{f}^{{}}\] is the final energy level, that is\[n_{f}^{{}}=2\]. And \[n_{i}^{{}}\]is the initial energy level, that is \[n_{i}^{{}}=1\] and E is the energy level and R is the Rydberg constant. So, For 2 energy levels${{E}_{2}}$ and ${{E}_{2}}$ .
\[{{E}_{2}}-{{E}_{1}}=-2.17\times {{10}^{-11}}(\dfrac{1}{4}-\dfrac{1}{1})\]=\[2.17\times {{10}^{-11}}\dfrac{3}{4}\]
Here, \[n_{f}^{{}}\]is the final energy level, that is \[n_{f}^{{}}=2\]. And \[n_{i}^{{}}\]is the initial energy level, that is \[n_{i}^{{}}=1\]
\[{{E}_{2}}-{{E}_{1}} = \Delta E=hv=\dfrac{c}{\lambda }h\]
We can write the above equation in another manner too based on wavelength.
\[\lambda = \dfrac{hc}{\Delta E}\]
Where, \[\lambda \]is the wavelength, h is the Planck’s constant, c is the velocity of light and \[\Delta E\] difference in energy levels. We know, \[h=6.62\times {{10}^{-27}}erg\], \[c=3\times {{10}^{10}}cm\] and \[\Delta E\] is given as\[2.17\times {{10}^{-11}}\dfrac{3}{4}\].
\[\lambda =\dfrac{6.62\times {{10}^{-27}}erg\times 3\times {{10}^{10}}cm}{2.17\times {{10}^{-11}}\dfrac{3}{4}} = \dfrac{2.648}{2.17}{{10}^{-5}}cm\]
$=1.22\times { 10 }^{ -5 }cm = 1220\mathring { A } $
Additional Information:
Niels Bohr produces the atomic Hydrogen model. In it he describes, a positively charged nucleus consists of protons and neutrons and is surrounded by negatively charged electron clouds. The atom is held together by electrostatic forces between the positively charged nucleus and negatively charged surrounding, that is electrons. The structure of hydrogen in Bohr’s model has energy levels.
Note: In the question, wavelength in angstrom is asked. We are calculating wavelength in centimetres. We should always see to it that it is converted to angstrom units. 1 Armstrong =${{10}^{-8}}$ centimetres.
Complete step by step solution:
In the question, we have to find the difference between two energy levels, which give the wavelength of the photon that is emitted. This is explained by using a formula called Rydberg formula.
\[E=R(\dfrac{1}{n_{f}^{2}}-\dfrac{1}{n_{i}^{2}})\] Here, \[n_{f}^{{}}\] is the final energy level, that is\[n_{f}^{{}}=2\]. And \[n_{i}^{{}}\]is the initial energy level, that is \[n_{i}^{{}}=1\] and E is the energy level and R is the Rydberg constant. So, For 2 energy levels${{E}_{2}}$ and ${{E}_{2}}$ .
\[{{E}_{2}}-{{E}_{1}}=-2.17\times {{10}^{-11}}(\dfrac{1}{4}-\dfrac{1}{1})\]=\[2.17\times {{10}^{-11}}\dfrac{3}{4}\]
Here, \[n_{f}^{{}}\]is the final energy level, that is \[n_{f}^{{}}=2\]. And \[n_{i}^{{}}\]is the initial energy level, that is \[n_{i}^{{}}=1\]
\[{{E}_{2}}-{{E}_{1}} = \Delta E=hv=\dfrac{c}{\lambda }h\]
We can write the above equation in another manner too based on wavelength.
\[\lambda = \dfrac{hc}{\Delta E}\]
Where, \[\lambda \]is the wavelength, h is the Planck’s constant, c is the velocity of light and \[\Delta E\] difference in energy levels. We know, \[h=6.62\times {{10}^{-27}}erg\], \[c=3\times {{10}^{10}}cm\] and \[\Delta E\] is given as\[2.17\times {{10}^{-11}}\dfrac{3}{4}\].
\[\lambda =\dfrac{6.62\times {{10}^{-27}}erg\times 3\times {{10}^{10}}cm}{2.17\times {{10}^{-11}}\dfrac{3}{4}} = \dfrac{2.648}{2.17}{{10}^{-5}}cm\]
$=1.22\times { 10 }^{ -5 }cm = 1220\mathring { A } $
Additional Information:
Niels Bohr produces the atomic Hydrogen model. In it he describes, a positively charged nucleus consists of protons and neutrons and is surrounded by negatively charged electron clouds. The atom is held together by electrostatic forces between the positively charged nucleus and negatively charged surrounding, that is electrons. The structure of hydrogen in Bohr’s model has energy levels.
Note: In the question, wavelength in angstrom is asked. We are calculating wavelength in centimetres. We should always see to it that it is converted to angstrom units. 1 Armstrong =${{10}^{-8}}$ centimetres.
Recently Updated Pages
Three beakers labelled as A B and C each containing 25 mL of water were taken A small amount of NaOH anhydrous CuSO4 and NaCl were added to the beakers A B and C respectively It was observed that there was an increase in the temperature of the solutions contained in beakers A and B whereas in case of beaker C the temperature of the solution falls Which one of the following statements isarecorrect i In beakers A and B exothermic process has occurred ii In beakers A and B endothermic process has occurred iii In beaker C exothermic process has occurred iv In beaker C endothermic process has occurred

Master Class 11 Social Science: Engaging Questions & Answers for Success

Master Class 11 Physics: Engaging Questions & Answers for Success

Master Class 11 Maths: Engaging Questions & Answers for Success

Master Class 11 Economics: Engaging Questions & Answers for Success

Master Class 11 Computer Science: Engaging Questions & Answers for Success

Trending doubts
One Metric ton is equal to kg A 10000 B 1000 C 100 class 11 physics CBSE

There are 720 permutations of the digits 1 2 3 4 5 class 11 maths CBSE

State and prove Bernoullis theorem class 11 physics CBSE

Draw a diagram of a plant cell and label at least eight class 11 biology CBSE

Difference Between Prokaryotic Cells and Eukaryotic Cells

1 Quintal is equal to a 110 kg b 10 kg c 100kg d 1000 class 11 physics CBSE

