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  1. Problems
  2. /In the Bohr model, the orbit n of a hydrogen-like ion has radius rn = 52.9 n²/Z pm, the angular…
HardChemistryHigh School (11–12)Structure of the Atom › Quantum Mechanical Model of the AtomNumericalJEE MainJEE AdvancedNEET

In the Bohr model, the orbit n of a hydrogen-like ion has radius rn = 52.9 n²/Z pm, the angular…

StemPy LabContributed by StemPy Lab

Try it on paper first. A hint, the key idea and the worked solution are here when you need them.

In the Bohr model, the orbit nnn of a hydrogen-like ion has radius rn=52.9 n2Z pmr_n = 52.9\,\dfrac{n^2}{Z}\ \text{pm}rn​=52.9Zn2​ pm, the angular momentum of the electron is mevr=nh2πm_e v r = \dfrac{nh}{2\pi}me​vr=2πnh​, and its energy is En=−2.18×10−18 Z2n2 JE_n = -2.18 \times 10^{-18}\,\dfrac{Z^2}{n^2}\ \text{J}En​=−2.18×10−18n2Z2​ J. Consider the electron of a He+\text{He}^{+}He+ ion (Z=2Z = 2Z=2) in the orbit n=3n = 3n=3. Take h=6.626×10−34 J sh = 6.626 \times 10^{-34}\ \text{J s}h=6.626×10−34 J s, me=9.109×10−31 kgm_e = 9.109 \times 10^{-31}\ \text{kg}me​=9.109×10−31 kg, 1 eV=1.602×10−19 J1\ \text{eV} = 1.602 \times 10^{-19}\ \text{J}1 eV=1.602×10−19 J and c=3.0×108 m s−1c = 3.0 \times 10^{8}\ \text{m s}^{-1}c=3.0×108 m s−1.

  1. What is the radius of this orbit?
  2. How fast does the electron move in it?
  3. What is its de Broglie wavelength?
  4. What is its kinetic energy, in electronvolts?
  5. The electron now falls straight to n=1n = 1n=1. What is the wavelength of the light given out?

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The worked solution

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Work it out on paper first. It is fine to get stuck or make a mistake: that is how we learn. When you are ready, go through the solution one step at a time, and check each step against your own.

Plan. Radius from the formula, speed from the angular momentum, then the wavelength and the energy.

(a) Radius. r3=52.9×92 pm=238.05 pmr_3 = 52.9 \times \dfrac{9}{2}\ \text{pm} = 238.05\ \text{pm}r3​=52.9×29​ pm=238.05 pm.

(b) Speed.

v=nh2πmer=3×6.626×10−342π×9.109×10−31×2.3805×10−10 m s−1=1.459×106 m s−1\displaystyle v = \frac{nh}{2\pi m_e r} = \frac{3 \times 6.626 \times 10^{-34}}{2\pi \times 9.109 \times 10^{-31} \times 2.3805 \times 10^{-10}}\ \text{m s}^{-1} = 1.459 \times 10^{6}\ \text{m s}^{-1}v=2πme​rnh​=2π×9.109×10−31×2.3805×10−103×6.626×10−34​ m s−1=1.459×106 m s−1

(c) de Broglie wavelength.

λ=hmev=6.626×10−349.109×10−31×1.459×106 m=498.6 pm\displaystyle \lambda = \frac{h}{m_e v} = \frac{6.626 \times 10^{-34}}{9.109 \times 10^{-31} \times 1.459 \times 10^{6}}\ \text{m} = 498.6\ \text{pm}λ=me​vh​=9.109×10−31×1.459×1066.626×10−34​ m=498.6 pm

The orbit is 2πr=1495.7 pm2\pi r = 1495.7\ \text{pm}2πr=1495.7 pm long, exactly three wavelengths. This is Bohr's rule seen as a standing wave: nnn whole waves fit round orbit nnn.

(d) Kinetic energy. 12mev2=9.695×10−19 J=6.05 eV\tfrac12 m_e v^2 = 9.695 \times 10^{-19}\ \text{J} = 6.05\ \text{eV}21​me​v2=9.695×10−19 J=6.05 eV. It equals the size of the orbit's energy, 2.18×10−18×49 J=9.689×10−19 J2.18 \times 10^{-18} \times \tfrac49\ \text{J} = 9.689 \times 10^{-19}\ \text{J}2.18×10−18×94​ J=9.689×10−19 J, as the Bohr model says it must.

(e) The light. ΔE=2.18×10−18×4×(1−19) J=7.751×10−18 J\Delta E = 2.18 \times 10^{-18} \times 4 \times \left(1 - \dfrac19\right)\ \text{J} = 7.751 \times 10^{-18}\ \text{J}ΔE=2.18×10−18×4×(1−91​) J=7.751×10−18 J, so

λ=hcΔE=6.626×10−34×3.0×1087.751×10−18 m=25.6 nm\displaystyle \lambda = \frac{hc}{\Delta E} = \frac{6.626 \times 10^{-34} \times 3.0 \times 10^{8}}{7.751 \times 10^{-18}}\ \text{m} = 25.6\ \text{nm}λ=ΔEhc​=7.751×10−186.626×10−34×3.0×108​ m=25.6 nm

This is far in the ultraviolet.

Watch out. The de Broglie wavelength is not the wavelength of the light. One belongs to the moving electron, the other to the photon it gives out.

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