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Exercises · 12.5

Q.A difference of 2.3 eV2.3\ \text{eV} separates two energy levels in an atom. What is the frequency of radiation emitted when the atom makes a transition from the upper level to the lower level?

Puducherry CbseNCERTSubjective· 2mImportance★★★★★
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The energy difference between two atomic levels is directly proportional to the frequency of the emitted photon via E=hνE = h\nu. For ΔE=2.3 eV\Delta E = 2.3\ \text{eV}, the frequency is ν=5.56×1014 Hz\nu = 5.56 \times 10^{14}\ \text{Hz}.

When an electron in an atom jumps from a higher energy level to a lower one, the atom loses energy. That energy doesn't vanish — it leaves the atom as a single packet of light, a photon. The photon’s energy is exactly equal to the difference between the two atomic energy levels.

This is the core idea behind atomic spectra: each spectral line corresponds to a specific transition, and the photon’s frequency is locked to the energy gap by Planck’s constant hh.

Ephoton=hν=ΔEE_{\text{photon}} = h \nu = \Delta E

Here h=6.626×10−34 J⋅sh = 6.626 \times 10^{-34}\ \text{J·s} is Planck’s constant, and ν\nu is the frequency in hertz. The problem gives ΔE=2.3 eV\Delta E = 2.3\ \text{eV}, but hh is in joules — so we must convert the energy to joules first.

  1. Convert the energy from eV to joules. The conversion factor is 1 eV=1.602×10−19 J1\ \text{eV} = 1.602 \times 10^{-19}\ \text{J}. So:

ΔE=2.3×1.602×10−19=3.6846×10−19 J\Delta E = 2.3 \times 1.602 \times 10^{-19} = 3.6846 \times 10^{-19}\ \text{J}

  1. Apply the photon energy relation. From E=hνE = h\nu, we solve for frequency:

ν=ΔEh\nu = \frac{\Delta E}{h}

  1. Plug in the numbers.

ν=3.6846×10−196.626×10−34\nu = \frac{3.6846 \times 10^{-19}}{6.626 \times 10^{-34}}

Divide:

ν=5.56×1014 Hz\nu = 5.56 \times 10^{14}\ \text{Hz} …

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