Calculate the wave number for the shortest wavelength transition in the Balmer series of atomic hydrogen.
Answer
566.4k+ views
Hint: Substitute the values of highest and lowest principal quantum number possible in the Rydberg formula to find the wave number.
Formula: $\dfrac{1}{\lambda }={{Z}^{2}}{{R}_{\infty }}\left( \dfrac{1}{{{n}_{1}}^{2}}-\dfrac{1}{{{n}_{2}}^{2}} \right)$
where,
$\dfrac{1}{\lambda }$ is the wavenumber,
Z is the atomic number,
${{R}_{\infty }}$ is the Rydberg constant whose value is $1.09677*{{10}^{7}}{{m}^{-1}}$,
${{n}_{1}}$ is the principal quantum number of lower energy level,
${{n}_{2}}$ is the principal quantum number of upper energy level
Complete step by step answer:
We will now try to understand the emission spectrum of Hydrogen.
-When a hydrogen atom absorbs a photon, it causes the electron to experience a transition to a higher energy level, for example, n = 1 to n = 2.
-When a photon is emitted through a hydrogen atom, the electron undergoes a transition from a higher energy level to a lower, for example, n = 3 to n = 2.
-During this transition from a higher level to a lower level, there is the transmission of light.
The series of hydrogen emission spectrums have unique names based on the transition from higher energy to lower energy.
-Lyman Series: Transition of an electron from outer orbit having n>1 to n=1.
-Balmer Series: Transition of an electron from outer orbit having n>1 to n=2.
-Paschen Series: Transition of an electron from outer orbit having n>1 to n=3.
-Brackett Series: Transition of an electron from outer orbit having n>1 to n=4.
-Pfund Series: Transition of an electron from outer orbit having n>1 to n=5.
-Humphrey Series: Transition of an electron from outer orbit having n>1 to n=6.
It is important to remember that the wavelength emitted in the Balmer series alone lies in the visible range of the light spectrum.
The shortest wavelength transition in Balmer series is $n=\infty \to n=2$
Substituting the above values in the Rydberg formula,
$\dfrac{1}{\lambda }=1*1.09677*{{10}^{7}}*\left( \dfrac{1}{4}-0 \right)$
$\dfrac{1}{\lambda }=2741925{{m}^{-1}}$
Therefore, the wavenumber with the shortest wavelength transition is $2741925{{m}^{-1}}$.
Note: Do not get confused between the meaning of ${{n}_{1}}$and ${{n}_{2}}$.${{n}_{2}}$ must always have a larger value than ${{n}_{1}}$for the transition to exist and wavelength to be transmitted.
Formula: $\dfrac{1}{\lambda }={{Z}^{2}}{{R}_{\infty }}\left( \dfrac{1}{{{n}_{1}}^{2}}-\dfrac{1}{{{n}_{2}}^{2}} \right)$
where,
$\dfrac{1}{\lambda }$ is the wavenumber,
Z is the atomic number,
${{R}_{\infty }}$ is the Rydberg constant whose value is $1.09677*{{10}^{7}}{{m}^{-1}}$,
${{n}_{1}}$ is the principal quantum number of lower energy level,
${{n}_{2}}$ is the principal quantum number of upper energy level
Complete step by step answer:
We will now try to understand the emission spectrum of Hydrogen.
-When a hydrogen atom absorbs a photon, it causes the electron to experience a transition to a higher energy level, for example, n = 1 to n = 2.
-When a photon is emitted through a hydrogen atom, the electron undergoes a transition from a higher energy level to a lower, for example, n = 3 to n = 2.
-During this transition from a higher level to a lower level, there is the transmission of light.
The series of hydrogen emission spectrums have unique names based on the transition from higher energy to lower energy.
-Lyman Series: Transition of an electron from outer orbit having n>1 to n=1.
-Balmer Series: Transition of an electron from outer orbit having n>1 to n=2.
-Paschen Series: Transition of an electron from outer orbit having n>1 to n=3.
-Brackett Series: Transition of an electron from outer orbit having n>1 to n=4.
-Pfund Series: Transition of an electron from outer orbit having n>1 to n=5.
-Humphrey Series: Transition of an electron from outer orbit having n>1 to n=6.
It is important to remember that the wavelength emitted in the Balmer series alone lies in the visible range of the light spectrum.
The shortest wavelength transition in Balmer series is $n=\infty \to n=2$
Substituting the above values in the Rydberg formula,
$\dfrac{1}{\lambda }=1*1.09677*{{10}^{7}}*\left( \dfrac{1}{4}-0 \right)$
$\dfrac{1}{\lambda }=2741925{{m}^{-1}}$
Therefore, the wavenumber with the shortest wavelength transition is $2741925{{m}^{-1}}$.
Note: Do not get confused between the meaning of ${{n}_{1}}$and ${{n}_{2}}$.${{n}_{2}}$ must always have a larger value than ${{n}_{1}}$for the transition to exist and wavelength to be transmitted.
Recently Updated Pages
Master Class 11 English: Engaging Questions & Answers for Success

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

Master Class 11 Maths: Engaging Questions & Answers for Success

Master Class 11 Biology: Engaging Questions & Answers for Success

Master Class 11 Physics: Engaging Questions & Answers for Success

Master Class 11 Chemistry: Engaging Questions & Answers for Success

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

Difference Between Prokaryotic Cells and Eukaryotic Cells

Find the value of the expression given below sin 30circ class 11 maths CBSE

Difference between physical and chemical change class 11 chemistry CBSE

Two of the body parts which do not appear in MRI are class 11 biology CBSE

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

