The order of wavelength \(\left(\lambda\right)\) of the emitted photons from longest to shortest is,
\(\boxed{{\lambda _1}\left( {4 \to 3}\right)>{\lambda _2}\left( {4\to2}\right)>{\lambda _3}\left( {2\to1}\right)>{\lambda _4}\left( {3\to1}\right)}\)
Further explanation:
Concept:
According to the equation of photon energy, the energy of the photon is inversely proportional to the wavelength.
\(E=\dfrac{{hc}}{\lambda }\)
Here, E is the photon energy, h is the Planck constant,\(\left(\lambda\right)\) is the wavelength of photon, and c is the speed of light.
The formula to calculate the energy of the emitted photon in the hydrogen atom is,
\(E=\left({-13.6{\text{ eV}}}\right)\left({\dfrac{1}{{{{\left({{{\text{n}}_{\text{i}}}} \right)}^2}}}-\dfrac{1}{{{{\left( {{{\text{n}}_{\text{f}}}}\right)}^2}}}}\right)\)
Where,
E is the energy of emitted photon.
\({{\text{n}}_{\text{i}}}\) is the initial energy level of transition.
\({{\text{n}}_{\text{f}}}\) is the final energy level of transition.
Solution:
Finding the energy of emitted photons in each transition.
1. For the first transition, from initial energy level n=4 to final energy level n=3.
\(\begin{aligned}{E_1}&=\left({-13.6{\text{ eV}}}\right)\left({\dfrac{1}{{{{\left({{{\text{n}}_{\text{i}}}} \right)}^2}}}-\frac{1}{{{{\left({{{\text{n}}_{\text{f}}}} \right)}^2}}}}\right)\\&=\left( { - 13.6{\text{ eV}}} \right)\left( {\frac{1}{{{{\left( {\text{4}}\right)}^2}}}-\dfrac{1}{{{{\left( {\text{3}}\right)}^2}}}}\right)\\&=0.6611\,{\text{eV}}\\\end{aligned}\)
2. For the second transition, from initial energy level n=4 to final energy level n=2.
\(\begin{aligned}{E_1}&=\left({-13.6{\text{ eV}}}\right)\left({\dfrac{1}{{{{\left({{{\text{n}}_{\text{i}}}} \right)}^2}}}-\frac{1}{{{{\left({{{\text{n}}_{\text{f}}}} \right)}^2}}}}\right)\\&=\left( { - 13.6{\text{ eV}}} \right)\left( {\frac{1}{{{{\left( {\text{4}}\right)}^2}}}-\dfrac{1}{{{{\left( {\text{2}}\right)}^2}}}}\right)\\&=2.55\,{\text{eV}}\\\end{aligned}\)
3. For the third transition, from initial energy level n=2 to final energy level n=1.
\(\begin{aligned}{E_1}&=\left({-13.6{\text{ eV}}}\right)\left({\dfrac{1}{{{{\left({{{\text{n}}_{\text{i}}}} \right)}^2}}}-\frac{1}{{{{\left({{{\text{n}}_{\text{f}}}} \right)}^2}}}}\right)\\&=\left( { - 13.6{\text{ eV}}} \right)\left( {\frac{1}{{{{\left( {\text{2}}\right)}^2}}}-\dfrac{1}{{{{\left( {\text{1}}\right)}^2}}}}\right)\\&=10.2\,{\text{eV}}\\\end{aligned}\)
4. For the fourth transition, from initial energy level n=3 to final energy level n=1.
\(\begin{aligned}{E_1}&=\left({-13.6{\text{ eV}}}\right)\left({\dfrac{1}{{{{\left({{{\text{n}}_{\text{i}}}} \right)}^2}}}-\frac{1}{{{{\left({{{\text{n}}_{\text{f}}}} \right)}^2}}}}\right)\\&=\left( { - 13.6{\text{ eV}}} \right)\left( {\frac{1}{{{{\left( {\text{3}}\right)}^2}}}-\dfrac{1}{{{{\left( {\text{1}}\right)}^2}}}}\right)\\&=12.09\,{\text{eV}}\\\end{aligned}\)
The energy of emitted photons in increasing order are,
\({E_1}\left({4 \to 3} \right)<{E_2}\left({4 \to 2}\right)<{E_3}\left({2 \to 1} \right)<{E_4}\left( {3 \to 1}\right)\)
Since the wavelength is inversely proportional to the energy of emitted photons, therefore, corresponding order of wavelength \(\left(\lambda\right)\) of the emitted photons from longest to shortest is,
\(\boxed{{\lambda _1}\left( {4 \to 3}\right)>{\lambda _2}\left( {4\to2}\right)>{\lambda _3}\left( {2\to1}\right)>{\lambda _4}\left( {3\to1}\right)}\)
Learn more:
1. Ranking of elements according to their first ionization energy.:https://brainly.com/question/1550767
2.Chemical equation representing the first ionization energy for lithium.:https://brainly.com/question/5880605
Answer details:
Grade: Senior School
Subject: Chemistry
Chapter: Atomic structure
Keywords: transition, hydrogen atom, energy difference, transition from n=4 to n=3, transition from n=4 to n=2, transition from n=2 to n=1, transition from n=3 to n=1, greatest, emitted photons.