General Chemistry 202-SN1-RE • CEGEP, Montreal

Corrected exercises: atomic structure and electron configuration (202-SN1-RE)

This is the corrected exercise set on atomic structure and electron configuration for General Chemistry, 202-SN1-RE (formerly 202-NYA). It is the first big chapter of the course, the one that introduces the quantum language: isotopes and average atomic mass, quanta of light, quantum numbers, orbitals, electron configuration, and the link between the energy levels of an atom and the lines of its spectrum. Part A covers the basics: isotopes and the mass spectrum (exercise 1), photon energy and the photoelectric effect (exercise 2), the quantum model and quantum numbers (exercise 3), electron configuration with its exceptions (exercise 4), and wavelengths from the Bohr model (exercise 5). Part B moves up to exam level: periodicity explained by effective nuclear charge (exercise 6), hydrogen-like ions and the three spectral series (exercise 7), wave-particle duality (exercise 8), successive ionization energies (exercise 9) and a complete hydrogen lamp problem (exercise 10).

The set is written for CEGEP students in the Science program (Sciences de la nature) and follows the same course outline as the French-language version. Corrected material at this level is hard to find online: what turns up is mostly paid question banks, or university exercises that cut the chapter differently.

The reflex to keep throughout: an atomic spectrum is not continuous. Each line corresponds to a transition between two precise energy levels, and the energy of the photon is exactly the difference between those two levels. Absorption when the electron goes up, emission when it comes down: the sign of ΔE\Delta E tells the whole story.

10 corrected exercises • 100 points • 150 minutes

This chapter is part of 202-SN1-RE, every chapter with its set and sheet Before you start Revision sheet: the traps and the method for this chapter

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Course recap

  • • Isotopes and average atomic mass: two isotopes of the same element have the same number of protons ZZ but different numbers of neutrons, hence different mass numbers AA. The atomic mass in the periodic table is the average of the isotopic masses weighted by their natural abundances, which is why it is almost never a whole number.
  • • Quanta and the photoelectric effect: E=hν=hcλE=h\nu=\dfrac{hc}{\lambda}. A metal ejects an electron only if the photon energy exceeds the work function W0W_{0}, and then Ek,max=hν−W0E_{k,max}=h\nu-W_{0}. Raising the intensity of light that is not energetic enough ejects nothing: this is the experiment that forced the photon on physics.
  • • The four quantum numbers: nn (principal, n=1,2,3,...n=1,2,3,..., the shell); ll (azimuthal, l=0,1,...,n−1l=0,1,...,n-1, the subshell s, p, d, f); mlm_{l} (magnetic, an integer from −l-l to +l+l, the orbital); msm_{s} (spin, +12+\tfrac{1}{2} or −12-\tfrac{1}{2}). A shell nn holds n2n^{2} orbitals and 2n22n^{2} electrons; a subshell ll holds 2l+12l+1 orbitals and 2(2l+1)2(2l+1) electrons.
  • • Electron configuration: the Aufbau principle (filling in order of increasing energy 1s 2s 2p 3s 3p 4s 3d 4p...1s\,2s\,2p\,3s\,3p\,4s\,3d\,4p...), the Pauli exclusion principle (at most two electrons per orbital, with opposite spins), Hund's rule (occupy each orbital of a subshell with one electron of the same spin before pairing up).
  • • Exceptions in the d block: chromium and copper adopt [Ar]4s13d5[Ar]4s^{1}3d^{5} and [Ar]4s13d10[Ar]4s^{1}3d^{10}, because a half-filled or filled dd subshell is especially stable. An atom with unpaired electrons is paramagnetic; if all its electrons are paired, it is diamagnetic.
  • • Bohr model for hydrogen: the energy of level nn is En=−2.18×10−18n2E_{n}=-\dfrac{2.18\times 10^{-18}}{n^{2}} J. The energy of a photon is E=hν=hcλE=h\nu=\dfrac{hc}{\lambda}, where h=6.626×10−34h=6.626\times 10^{-34} J·s and c=3.00×108c=3.00\times 10^{8} m/s. The energy of the photon exchanged in a transition is ∣ΔE∣=∣Efinal−Einitial∣|\Delta E|=|E_{final}-E_{initial}|.
  • • Periodicity: the effective nuclear charge ZeffZ_{eff} (the attraction felt by a valence electron) increases from left to right across a period. The atomic radius decreases from left to right (ZeffZ_{eff} grows) and increases from top to bottom (one more shell). Ionization energy and electronegativity follow the opposite trend to the radius.
  • • Avogadro constant: NA=6.022×1023N_{A}=6.022\times 10^{23} /mol, to go from an energy per atom to an energy per mole.
  • • Hydrogen-like ions: for an ion with a single electron and atomic number ZZ, En=−2.18×10−18 Z2n2E_{n}=-\dfrac{2.18\times 10^{-18}\,Z^{2}}{n^{2}} J. Spectral series of hydrogen: Lyman (transitions down to n=1n=1, ultraviolet), Balmer (to n=2n=2, visible), Paschen (to n=3n=3, infrared).
  • • Duality and uncertainty: λ=hmv\lambda=\dfrac{h}{mv} (de Broglie) and Δx Δp≥h4π\Delta x\,\Delta p\geq \dfrac{h}{4\pi} (Heisenberg), with Δp=m Δv\Delta p=m\,\Delta v and me=9.109×10−31m_{e}=9.109\times 10^{-31} kg.
  • • Successive ionization energies: they always increase, but a sharp jump appears as soon as the electron core is entered. The position of the jump gives the number of valence electrons, hence the group. Electron affinity is the energy involved when a gaseous atom captures an electron: negative when the capture is favourable.

Part A: Isotopes, quanta, configuration and spectrum (/50)

Exercise 1: Isotopes, average atomic mass and the mass spectrum

Natural chlorine is a mixture of two isotopes: 35Cl^{35}Cl (mass 34.9689 u, abundance 75.77%) and 37Cl^{37}Cl (36.9659 u, 24.23%). Natural copper also has two, 63Cu^{63}Cu (62.9296 u) and 65Cu^{65}Cu (64.9278 u), and its tabulated atomic mass is 63.546 u. The figure below shows the mass spectrum of natural chlorine.

343536373820406080100120³⁵Cl75.77%³⁷Cl24.23%mass (u)abundance (%)
  • a) Give the composition of the nucleus and the number of electrons of the 37Cl^{37}Cl atom, then of the 37Cl−^{37}Cl^{-} ion.
  • b) Calculate the average atomic mass of chlorine and explain why the atomic masses in the periodic table are almost never whole numbers.
  • c) Determine the natural abundance of each of the two isotopes of copper.
  • d) The mass spectrum of atomic bromine shows two peaks: 78.9183 u (50.69%) and 80.9163 u (49.31%). Calculate the atomic mass of bromine, then predict the appearance of the mass spectrum of the Br2Br_{2} molecule: how many peaks, at which masses, in what intensity ratio?

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  • a) 17 protons, 20 neutrons; 17 electrons for the atom, 18 for 37Cl−^{37}Cl^{-}
  • b) M=35.45M=35.45 u: a weighted average, so almost never a whole number
  • c) 69.15% 63Cu^{63}Cu and 30.85% 65Cu^{65}Cu
  • d) M(Br)=79.90M(Br)=79.90 u; three peaks at 158, 160 and 162 u, in the ratio 1 : 2 : 1
a)

The mass number is A=37A=37 and the atomic number is Z=17Z=17: the nucleus contains 17 protons and 37−17=2037-17=20 neutrons. The neutral 37Cl^{37}Cl atom has 17 electrons. The 37Cl−^{37}Cl^{-} ion has gained one electron: same nucleus (17 protons, 20 neutrons), but 18 electrons.

b)

M=34.9689×0.7577+36.9659×0.2423=26.497+8.956=35.45M=34.9689\times 0.7577+36.9659\times 0.2423=26.497+8.956=35.45 u. The tabulated value is not a whole number because it is not the mass of any one atom, but the average of the isotopic masses weighted by their natural abundances. It falls between 35 and 37, closer to 35 since 35Cl^{35}Cl is three times as abundant.

c)

Let xx be the abundance of 63Cu^{63}Cu; then 62.9296x+64.9278(1−x)=63.54662.9296x+64.9278(1-x)=63.546. Solving: x=64.9278−63.54664.9278−62.9296=1.38181.9982=0.6915x=\dfrac{64.9278-63.546}{64.9278-62.9296}=\dfrac{1.3818}{1.9982}=0.6915. Natural copper is therefore 69.15% 63Cu^{63}Cu and 30.85% 65Cu^{65}Cu.

d)

M(Br)=78.9183×0.5069+80.9163×0.4931=79.90M(Br)=78.9183\times 0.5069+80.9163\times 0.4931=79.90 u. For Br2Br_{2}, each atom is independently 79Br^{79}Br (probability p=0.5069p=0.5069) or 81Br^{81}Br (q=0.4931q=0.4931), which gives three peaks: 79Br2^{79}Br_{2} at 158 u with probability p2=0.257p^{2}=0.257, 79Br81Br^{79}Br^{81}Br at 160 u with 2pq=0.5002pq=0.500 (there are two ways to form the mixed molecule, hence the factor 2), and 81Br2^{81}Br_{2} at 162 u with q2=0.243q^{2}=0.243. The intensities are therefore in a ratio close to 1 : 2 : 1, with the central peak twice as tall as the other two. This is the classic signature of bromine in mass spectrometry.

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Exercise 2: Light, quanta and the photoelectric effect

The sodium lamps used for street lighting emit yellow light of wavelength 589 nm. Potassium has a work function (threshold energy) W0=3.68×10−19W_{0}=3.68\times 10^{-19} J. Use h=6.626×10−34h=6.626\times 10^{-34} J·s, c=3.00×108c=3.00\times 10^{8} m/s, NA=6.022×1023N_{A}=6.022\times 10^{23} /mol and me=9.109×10−31m_{e}=9.109\times 10^{-31} kg. The diagram below shows the plate and the three kinds of illumination studied.

potassium plate: W₀ = 3.68 × 10⁻¹⁹ Ja) 589 nmc) 400 nmd) 700 nm100 times more intense
  • a) Calculate the frequency and the energy of a 589 nm photon, then the energy of one mole of these photons in kJ/mol.
  • b) Calculate the threshold wavelength of potassium, that is, the longest wavelength able to eject an electron. What colour does it correspond to?
  • c) Potassium is illuminated with violet light of 400 nm. Calculate the maximum kinetic energy of the ejected electrons, then their speed.
  • d) The same metal is now illuminated with red light of 700 nm, but one hundred times more intense. Predict the result by calculation, then explain why it is incompatible with a purely wave model of light.

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  • a) ν=5.09×1014\nu=5.09\times 10^{14} Hz, E=3.37×10−19E=3.37\times 10^{-19} J, that is 203 kJ/mol
  • b) λ0=540\lambda_{0}=540 nm, green light
  • c) Ek=1.29×10−19E_{k}=1.29\times 10^{-19} J and v=5.32×105v=5.32\times 10^{5} m/s
  • d) E=2.84×10−19E=2.84\times 10^{-19} J <W0<W_{0}: no electron, whatever the intensity
a)

ν=cλ=3.00×108589×10−9=5.09×1014\nu=\dfrac{c}{\lambda}=\dfrac{3.00\times 10^{8}}{589\times 10^{-9}}=5.09\times 10^{14} Hz. The photon energy is E=hν=(6.626×10−34)(5.09×1014)=3.37×10−19E=h\nu=(6.626\times 10^{-34})(5.09\times 10^{14})=3.37\times 10^{-19} J. For one mole: 3.37×10−19×6.022×1023=2.03×1053.37\times 10^{-19}\times 6.022\times 10^{23}=2.03\times 10^{5} J/mol, that is 203 kJ/mol.

b)

At the threshold, all of the photon energy goes exactly into extracting the electron: hcλ0=W0\dfrac{hc}{\lambda_{0}}=W_{0}, so λ0=hcW0=(6.626×10−34)(3.00×108)3.68×10−19=5.40×10−7\lambda_{0}=\dfrac{hc}{W_{0}}=\dfrac{(6.626\times 10^{-34})(3.00\times 10^{8})}{3.68\times 10^{-19}}=5.40\times 10^{-7} m, that is 540 nm: green light. Any light with a wavelength below 540 nm (hence more energetic) ejects electrons; any light beyond it ejects none.

c)

E=hcλ=(6.626×10−34)(3.00×108)400×10−9=4.97×10−19E=\dfrac{hc}{\lambda}=\dfrac{(6.626\times 10^{-34})(3.00\times 10^{8})}{400\times 10^{-9}}=4.97\times 10^{-19} J. The maximum kinetic energy is the excess: Ek=E−W0=4.97×10−19−3.68×10−19=1.29×10−19E_{k}=E-W_{0}=4.97\times 10^{-19}-3.68\times 10^{-19}=1.29\times 10^{-19} J. Then v=2Ekme=2(1.29×10−19)9.109×10−31=5.32×105v=\sqrt{\dfrac{2E_{k}}{m_{e}}}=\sqrt{\dfrac{2(1.29\times 10^{-19})}{9.109\times 10^{-31}}}=5.32\times 10^{5} m/s.

d)

At 700 nm, E=hcλ=2.84×10−19E=\dfrac{hc}{\lambda}=2.84\times 10^{-19} J, which is below W0=3.68×10−19W_{0}=3.68\times 10^{-19} J: no electron is ejected, and the intensity changes nothing. In the wave model, the energy carried by a wave depends on its amplitude, hence on its intensity: with light strong enough, or shone long enough, the required energy should eventually build up. Experiment says the opposite, and instantly: what counts is the energy of a single photon, hνh\nu. Raising the intensity raises the number of photons, not the energy of each one. This is exactly Einstein's argument of 1905.

12345678910−4−3−2−1123ν₀ = 5.55400 nm: 1.29700 and 589 nm: no electron−W₀ν (10¹⁴ Hz)slope hEk max (10⁻¹⁹ J)

Exercise 3: The quantum model and quantum numbers

This exercise is about the four quantum numbers (n, l, ml, ms)(n,\ l,\ m_{l},\ m_{s}) that describe the state of an electron in an atom.

  • a) Give the physical meaning of each of the four quantum numbers and the set of values each may take.
  • b) How many orbitals and how many electrons at most can the n=4n=4 level hold? Justify using the rules.
  • c) How many electrons at most can occupy the 3d3d subshell?
  • d) Which of the following sets (n, l, ml, ms)(n,\ l,\ m_{l},\ m_{s}) are allowed? For the others, explain why they are forbidden:(i)(3, 2, −1, +12)(3,\ 2,\ -1,\ +\tfrac{1}{2})(ii)(2, 2, 0, −12)(2,\ 2,\ 0,\ -\tfrac{1}{2})(iii)(4, 3, −4, +12)(4,\ 3,\ -4,\ +\tfrac{1}{2})(iv)(1, 0, 0, +1)(1,\ 0,\ 0,\ +1).

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  • a) nn the energy, ll the shape (00 to n−1n-1), mlm_{l} the orientation (−l-l to +l+l), ms=±12m_{s}=\pm\tfrac{1}{2}
  • b) 16 orbitals and 32 electrons, that is n2n^{2} and 2n22n^{2}
  • c) 5 orbitals and 10 electrons
  • d) Only (i) is allowed; (ii) violates l≤n−1l\leq n-1, (iii) violates −l≤ml≤l-l\leq m_{l}\leq l, (iv) violates ms=±12m_{s}=\pm\tfrac{1}{2}
a)

nn (principal): the energy level and the size of the orbital; n=1, 2, 3,...n=1,\ 2,\ 3,... ll (azimuthal): the shape of the orbital and the subshell (l=0l=0 for s, 1 for p, 2 for d, 3 for f); ll runs from 00 to n−1n-1. mlm_{l} (magnetic): the orientation of the orbital, that is, the particular orbital; mlm_{l} takes the integers from −l-l to +l+l. msm_{s} (spin): the direction of the electron's spin; ms=+12m_{s}=+\tfrac{1}{2} or −12-\tfrac{1}{2}.

b)

The n=4n=4 level contains n2=16n^{2}=16 orbitals and at most 2n2=322n^{2}=32 electrons.

c)

The 3d3d subshell has l=2l=2, hence 2l+1=52l+1=5 orbitals and at most 2(2l+1)=102(2l+1)=10 electrons.

d)

(i) Allowed: l=2<n=3l=2<n=3, ml=−1m_{l}=-1 lies in [−2,2][-2, 2], ms=+12m_{s}=+\tfrac{1}{2}. (ii) Forbidden: ll must be strictly less than nn (at most n−1=1n-1=1); here l=2l=2 with n=2n=2 is impossible. (iii) Forbidden: mlm_{l} must lie between −l-l and +l+l, that is, between −3-3 and +3+3; ml=−4m_{l}=-4 is outside that interval. (iv) Forbidden: msm_{s} can only be +12+\tfrac{1}{2} or −12-\tfrac{1}{2}, never +1+1.

Exercise 4: Electron configuration and exceptions

Recall the atomic numbers: phosphorus Z=15Z=15, calcium Z=20Z=20, chromium Z=24Z=24, iron Z=26Z=26, copper Z=29Z=29. The periodic table extract below locates these five elements.

NaMgAlSiPSClArKCaScTiVCrMnFeCoNiCuZnGaGeAsSeBrKr123456789101112131415161718period 3period 4group
  • a) Write the full and the abbreviated electron configuration of phosphorus PP, then of the Ca2+Ca^{2+} ion.
  • b) Give the number of valence electrons of phosphorus and the number of unpaired electrons of phosphorus.
  • c) Chromium and copper are exceptions to the Aufbau principle. Give their actual electron configuration and briefly explain why.
  • d) Write the configuration of iron, then determine whether it is paramagnetic or diamagnetic. Justify.

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  • a) P=[Ne]3s23p3P=[Ne]3s^{2}3p^{3} and Ca2+=[Ar]Ca^{2+}=[Ar], 18 electrons
  • b) 5 valence electrons, 3 unpaired
  • c) Cr=[Ar]4s13d5Cr=[Ar]4s^{1}3d^{5} and Cu=[Ar]4s13d10Cu=[Ar]4s^{1}3d^{10}: d5d^{5} and d10d^{10} are stable
  • d) Fe=[Ar]4s23d6Fe=[Ar]4s^{2}3d^{6}, 4 unpaired, hence paramagnetic
a)

Phosphorus (Z=15Z=15): 1s22s22p63s23p31s^{2}2s^{2}2p^{6}3s^{2}3p^{3}, that is [Ne]3s23p3[Ne]3s^{2}3p^{3}. The Ca2+Ca^{2+} ion: neutral calcium is [Ar]4s2[Ar]4s^{2}; by losing its two 4s4s electrons, the ion becomes [Ar][Ar], that is 1s22s22p63s23p61s^{2}2s^{2}2p^{6}3s^{2}3p^{6} (18 electrons).

b)

Phosphorus has 5 valence electrons (the n=3n=3 shell: 3s23p33s^{2}3p^{3}). By Hund's rule, the three 3p3p electrons each occupy a separate orbital with the same spin: phosphorus therefore has 3 unpaired electrons.

c)

Chromium: [Ar]4s13d5[Ar]4s^{1}3d^{5} (not 4s23d44s^{2}3d^{4}); copper: [Ar]4s13d10[Ar]4s^{1}3d^{10} (not 4s23d94s^{2}3d^{9}). One 4s4s electron moves into 3d3d because a half-filled (3d53d^{5}) or completely filled (3d103d^{10}) dd subshell is especially stable.

d)

Iron (Z=26Z=26): [Ar]4s23d6[Ar]4s^{2}3d^{6}. The six 3d3d electrons are spread over the five dd orbitals: five occupy one orbital each (Hund), the sixth pairs up, which leaves 4 unpaired electrons. Since it has unpaired electrons, iron is paramagnetic.

P : [Ne]3s3p3 unpairedCr : [Ar]4s3d6 unpairedFe : [Ar]4s3d4 unpairedfilling order: 1s 2s 2p 3s 3p 4s 3d 4p ...Cr and Cu: one 4s electron moves to 3d (3d⁵, 3d¹⁰)

Exercise 5: The hydrogen spectrum and photon energy

In the hydrogen atom, the energy of level nn is En=−2.18×10−18n2E_{n}=-\dfrac{2.18\times 10^{-18}}{n^{2}} J. Use h=6.626×10−34h=6.626\times 10^{-34} J·s and c=3.00×108c=3.00\times 10^{8} m/s. The diagram below shows the first levels to scale.

n = 1E₁ = −2.18 × 10⁻¹⁸ Jn = 2n = 3n = ∞0 Jenergy
  • a) Calculate the energy of the electron at levels n=2n=2 and n=3n=3.
  • b) An electron goes from level n=3n=3 to level n=2n=2. Does the atom absorb or emit energy? Calculate the energy of the photon exchanged.
  • c) Calculate the wavelength of the photon. In which region of the spectrum (ultraviolet, visible, infrared) does it lie?

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  • a) E2=−5.45×10−19E_{2}=-5.45\times 10^{-19} J and E3=−2.42×10−19E_{3}=-2.42\times 10^{-19} J
  • b) Emission of 3.03×10−193.03\times 10^{-19} J
  • c) λ=657\lambda=657 nm, the red line in the visible
a)

E2=−2.18×10−184=−5.45×10−19E_{2}=-\dfrac{2.18\times 10^{-18}}{4}=-5.45\times 10^{-19} J and E3=−2.18×10−189=−2.42×10−19E_{3}=-\dfrac{2.18\times 10^{-18}}{9}=-2.42\times 10^{-19} J.

b)

The electron drops from a higher level to a lower one: the atom emits energy. ΔE=E2−E3=−5.45×10−19−(−2.42×10−19)=−3.03×10−19\Delta E=E_{2}-E_{3}=-5.45\times 10^{-19}-(-2.42\times 10^{-19})=-3.03\times 10^{-19} J. The negative sign confirms emission; the energy of the emitted photon is ∣ΔE∣=3.03×10−19|\Delta E|=3.03\times 10^{-19} J.

c)

λ=hc∣ΔE∣=(6.626×10−34)(3.00×108)3.03×10−19=6.57×10−7\lambda=\dfrac{hc}{|\Delta E|}=\dfrac{(6.626\times 10^{-34})(3.00\times 10^{8})}{3.03\times 10^{-19}}=6.57\times 10^{-7} m, about 657 nm. This wavelength lies in the visible range (red light): it is the characteristic red line of the hydrogen spectrum. Every visible line, in fact, ends on level n=2n=2, that of the Balmer series; those that land on n=1n=1, the Lyman series, belong to the ultraviolet.

n = 1n = 2n = 3n = ∞0 eV (ionization)−13.6 eV(ground state)Lyman(ultraviolet)Balmer (visible)

Part B: Exam level (/50)

Exercise 6: Periodic properties and their anomalies

This exercise is about periodic trends and two famous exceptions to the ionization energy trend. The periodic table extract below locates the elements mentioned.

LiBeBCNOFNeNaMgAlSiPSClArKCaGaGeAsSeBrKr12131415161718234periodgroup
  • a) Using the effective nuclear charge ZeffZ_{eff} and the number of shells, explain why the atomic radius decreases from left to right across a period and increases from top to bottom down a group.
  • b) Rank the atoms NaNa, MgMg, KK and ClCl by increasing atomic radius.
  • c) The first ionization energy increases overall from left to right across a period. Yet Ei(Al)<Ei(Mg)E_{i}(Al)<E_{i}(Mg) and Ei(S)<Ei(P)E_{i}(S)<E_{i}(P) are measured. Explain these two anomalies from the electron configurations.
  • d) The ions O2−O^{2-}, F−F^{-}, Na+Na^{+} and Mg2+Mg^{2+} are isoelectronic (10 electrons each). Rank them by decreasing radius and justify.

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  • a) Period: ZeffZ_{eff} grows with the same number of shells; group: one more shell, shielded
  • b) Cl<Mg<Na<KCl<Mg<Na<K
  • c) AlAl loses a 3p3p above the full 3s23s^{2}; SS has a doubly occupied 3p3p orbital
  • d) O2−>F−>Na+>Mg2+O^{2-}>F^{-}>Na^{+}>Mg^{2+}: with 10 electrons, it is the number of protons that contracts
a)

Across a period, the number of shells does not change but the number of protons increases: the effective nuclear charge felt by the valence electrons grows, pulls them in harder, and the radius decreases. Down a group, one shell is added on each row: the valence electrons are farther and farther from the nucleus and shielded by the inner shells, so the radius increases.

b)

By increasing radius: Cl<Mg<Na<KCl<Mg<Na<K. Chlorine is farthest to the right (maximum ZeffZ_{eff}, smallest); MgMg then NaNa are in the same period but NaNa is farther left and so larger; potassium has one more shell and is the largest.

c)

The Al<MgAl<Mg anomaly: magnesium has the configuration [Ne]3s2[Ne]3s^{2}, a full and stable 3s3s subshell that is hard to ionize; aluminum [Ne]3s23p1[Ne]3s^{2}3p^{1} easily loses its single 3p3p electron, which is higher in energy. The S<PS<P anomaly: phosphorus has 3p33p^{3}, a stable half-filled subshell (one electron per orbital); sulfur 3p43p^{4} has one doubly occupied orbital, and the repulsion between those two paired electrons makes removal easier, hence a lower ionization energy.

d)

All have 10 electrons, so it is the number of protons that sets them apart. Nuclear charges: OO 8, FF 9, NaNa 11, MgMg 12. The more protons for the same cloud of 10 electrons, the more contracted the ion. By decreasing radius: O2−>F−>Na+>Mg2+O^{2-}>F^{-}>Na^{+}>Mg^{2+}.

Exercise 7: Hydrogen-like ions and the spectral series

The Bohr model remains exact for any ion with a single electron, called hydrogen-like: En=−2.18×10−18 Z2n2E_{n}=-\dfrac{2.18\times 10^{-18}\,Z^{2}}{n^{2}} J, where ZZ is the atomic number. Keep h=6.626×10−34h=6.626\times 10^{-34} J·s, c=3.00×108c=3.00\times 10^{8} m/s and NA=6.022×1023N_{A}=6.022\times 10^{23} /mol.

  • a) Calculate the energy of the electron of He+He^{+} (Z=2Z=2) in the ground state, then the ionization energy of He+He^{+} in kJ/mol. Compare it with the 1313 kJ/mol of hydrogen and justify the ratio obtained.
  • b) The Lyman series groups the transitions of hydrogen down to n=1n=1. Calculate the wavelength of the n=2→n=1n=2\rightarrow n=1 line and locate it in the spectrum.
  • c) Calculate the wavelength of the n=4→n=3n=4\rightarrow n=3 line of hydrogen (Paschen series) and locate it. Then rank the Lyman, Balmer and Paschen series by decreasing energy of the emitted photons, and explain the ranking without any new calculation.
  • d) Show by calculation that the n=4→n=2n=4\rightarrow n=2 transition of He+He^{+} emits exactly the same wavelength as the n=2→n=1n=2\rightarrow n=1 transition of hydrogen. Generalize: what condition on ZZ, nin_{i} and nfn_{f} makes a line of a hydrogen-like ion coincide with a line of hydrogen?

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  • a) E1=−8.72×10−18E_{1}=-8.72\times 10^{-18} J, that is 5251 kJ/mol, exactly 4 times hydrogen
  • b) λ=122\lambda=122 nm, far ultraviolet
  • c) λ=1876\lambda=1876 nm, infrared; Lyman, Balmer then Paschen by decreasing energy
  • d) Same λ\lambda of 122 nm; the coincidence occurs for nf→Znfn_{f}\rightarrow Zn_{f} and ni→Znin_{i}\rightarrow Zn_{i}
a)

E1=−(2.18×10−18)(22)12=−8.72×10−18E_{1}=-\dfrac{(2.18\times 10^{-18})(2^{2})}{1^{2}}=-8.72\times 10^{-18} J. To ionize is to bring the electron to n=∞n=\infty, where E=0E=0: 8.72×10−188.72\times 10^{-18} J must be supplied per ion, that is 8.72×10−18×6.022×1023=5.25×1068.72\times 10^{-18}\times 6.022\times 10^{23}=5.25\times 10^{6} J/mol, or 5251 kJ/mol. This is exactly 4 times the value for hydrogen, because the energy is proportional to Z2Z^{2} and ZZ goes from 1 to 2. Physically, the helium nucleus attracts its single electron twice as strongly, and the electron is much harder to remove.

b)

∣ΔE∣=2.18×10−18(112−122)=2.18×10−18×0.75=1.635×10−18|\Delta E|=2.18\times 10^{-18}\left(\dfrac{1}{1^{2}}-\dfrac{1}{2^{2}}\right)=2.18\times 10^{-18}\times 0.75=1.635\times 10^{-18} J. Then λ=hc∣ΔE∣=1.988×10−251.635×10−18=1.22×10−7\lambda=\dfrac{hc}{|\Delta E|}=\dfrac{1.988\times 10^{-25}}{1.635\times 10^{-18}}=1.22\times 10^{-7} m, that is 122 nm: in the far ultraviolet. The whole Lyman series is invisible to the eye.

c)

∣ΔE∣=2.18×10−18(19−116)=2.18×10−18×0.0486=1.06×10−19|\Delta E|=2.18\times 10^{-18}\left(\dfrac{1}{9}-\dfrac{1}{16}\right)=2.18\times 10^{-18}\times 0.0486=1.06\times 10^{-19} J, so λ=1.988×10−251.06×10−19=1.88×10−6\lambda=\dfrac{1.988\times 10^{-25}}{1.06\times 10^{-19}}=1.88\times 10^{-6} m, that is 1876 nm: in the infrared. By decreasing energy: Lyman, then Balmer, then Paschen. The reason is that the levels crowd together as nn increases: the drop to n=1n=1 crosses the largest energy gap, the drop to n=3n=3 the smallest. Ultraviolet, visible, infrared: the order of the series is also the order of the spectrum. Each series is named after its final level: Lyman falls to n=1n=1 (ultraviolet), Balmer to n=2n=2 (visible), Paschen to n=3n=3 (infrared).

d)

For He+He^{+}, ∣ΔE∣=2.18×10−18×22(122−142)=2.18×10−18×4×316=2.18×10−18×0.75|\Delta E|=2.18\times 10^{-18}\times 2^{2}\left(\dfrac{1}{2^{2}}-\dfrac{1}{4^{2}}\right)=2.18\times 10^{-18}\times 4\times \dfrac{3}{16}=2.18\times 10^{-18}\times 0.75, which is the same value 1.635×10−181.635\times 10^{-18} J as in b), hence the same wavelength of 122 nm. In general, ∣ΔE∣=2.18×10−18Z2(1nf2−1ni2)|\Delta E|=2.18\times 10^{-18}Z^{2}\left(\dfrac{1}{n_{f}^{2}}-\dfrac{1}{n_{i}^{2}}\right): if nfn_{f} and nin_{i} are replaced by ZnfZn_{f} and ZniZn_{i}, the factor Z2Z^{2} cancels exactly against the squares in the denominators. In other words, every line of hydrogen has a twin in He+He^{+} (levels doubled), in Li2+Li^{2+} (levels tripled), and so on. This is why some stellar lines attributed to hydrogen were at first misidentified.

n = 1n = 2n = 3n = 4n → ∞LymanBalmerPaschen

Exercise 8: Wave-particle duality: de Broglie and Heisenberg

The wavelength associated with a particle of mass mm and speed vv is λ=hmv\lambda=\dfrac{h}{mv} (de Broglie), and the uncertainty in its position and momentum obeys Δx Δp≥h4π\Delta x\,\Delta p\geq \dfrac{h}{4\pi} (Heisenberg), with Δp=m Δv\Delta p=m\,\Delta v. Use h=6.626×10−34h=6.626\times 10^{-34} J·s and me=9.109×10−31m_{e}=9.109\times 10^{-31} kg.

  • a) Calculate the de Broglie wavelength of an electron moving at 5.00×1065.00\times 10^{6} m/s. Compare it with the diameter of an atom, of the order of 1×10−101\times 10^{-10} m, and say which experimental technique this coincidence makes possible.
  • b) Calculate the de Broglie wavelength of a 145 g baseball thrown at 40.0 m/s. Why is the wave character of everyday objects never observed?
  • c) An electron is confined within an atom, so Δx≈1.0×10−10\Delta x\approx 1.0\times 10^{-10} m. Calculate the minimum uncertainty in its speed and compare it with the speed in part a). Repeat the calculation for the baseball located to within a millimetre.
  • d) Explain how these results condemn the notion of a Bohr orbit and justify speaking instead of an orbital, that is, a region of probability of presence.

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  • a) λ=1.45×10−10\lambda=1.45\times 10^{-10} m, the order of the spacing in a crystal: electron diffraction
  • b) λ=1.14×10−34\lambda=1.14\times 10^{-34} m, out of reach of any slit
  • c) Δv≥5.8×105\Delta v\geq 5.8\times 10^{5} m/s for the electron, 3.6×10−313.6\times 10^{-31} m/s for the ball
  • d) An orbit assumes a trajectory; only the probability of presence remains, the orbital
a)

λ=hmev=6.626×10−34(9.109×10−31)(5.00×106)=6.626×10−344.554×10−24=1.45×10−10\lambda=\dfrac{h}{m_{e}v}=\dfrac{6.626\times 10^{-34}}{(9.109\times 10^{-31})(5.00\times 10^{6})}=\dfrac{6.626\times 10^{-34}}{4.554\times 10^{-24}}=1.45\times 10^{-10} m. This is the same order of magnitude as the diameter of an atom and as the spacing between two planes of a crystal: the electron can therefore be diffracted by a crystal, exactly like X-rays. This is the principle of electron diffraction and, further on, of the electron microscope, whose resolving power far exceeds that of the optical microscope.

b)

λ=hmv=6.626×10−34(0.145)(40.0)=6.626×10−345.80=1.14×10−34\lambda=\dfrac{h}{mv}=\dfrac{6.626\times 10^{-34}}{(0.145)(40.0)}=\dfrac{6.626\times 10^{-34}}{5.80}=1.14\times 10^{-34} m. This wavelength is about 102410^{24} times smaller than that of the electron, and incomparably smaller than any object or slit one could make. No diffraction phenomenon can therefore be observed: the wave nature exists in principle for the ball, but it is experimentally out of reach. It is the mass in the denominator that crushes everything.

c)

Δv≥h4πmeΔx=6.626×10−344π(9.109×10−31)(1.0×10−10)=5.8×105\Delta v\geq \dfrac{h}{4\pi m_{e}\Delta x}=\dfrac{6.626\times 10^{-34}}{4\pi (9.109\times 10^{-31})(1.0\times 10^{-10})}=5.8\times 10^{5} m/s. This uncertainty is more than a tenth of the speed in part a): we do not even know the order of magnitude of the electron's speed once we know it is in the atom. For the ball: Δv≥6.626×10−344π(0.145)(1.0×10−3)=3.6×10−31\Delta v\geq \dfrac{6.626\times 10^{-34}}{4\pi (0.145)(1.0\times 10^{-3})}=3.6\times 10^{-31} m/s, a perfectly negligible uncertainty.

d)

A Bohr orbit assumes that the position and the speed of the electron are known at every instant: it is a trajectory. But part c) shows that locating the electron within the atom makes its speed totally undetermined, and the reverse is true too. The trajectory therefore has no meaning at this scale, not for lack of instruments, but by nature. What remains computable is the probability of finding the electron at a point: it is the square of the wave function, and the region where this probability is significant is called an orbital. The Bohr model keeps its energies EnE_{n}, which are correct for hydrogen, but loses its circular orbits. For the baseball, the uncertainty is so small that the classical trajectory remains perfectly valid: quantum mechanics does not contradict Newtonian mechanics, it contains it.

Exercise 9: Successive ionization energies and electron affinity

The first four successive ionization energies, in kJ/mol, of three elements of the third period are measured:

element XX: I1=496I_{1}=496, I2=4562I_{2}=4562, I3=6910I_{3}=6910, I4=9543I_{4}=9543;

element YY: I1=738I_{1}=738, I2=1451I_{2}=1451, I3=7733I_{3}=7733, I4=10540I_{4}=10540;

element ZZ: I1=578I_{1}=578, I2=1817I_{2}=1817, I3=2745I_{3}=2745, I4=11577I_{4}=11577. The figure below shows these three sequences of values.

123452000400060008000100001200014000XYZionization numberionization energy (kJ/mol)
  • a) For each of the three elements, locate the sharp jump in the sequence of ionization energies and deduce the number of valence electrons, hence the group.
  • b) Identify XX, YY and ZZ, give their abbreviated electron configuration, and check the consistency with the charge of the most stable ion of each.
  • c) The ratio I2/I1I_{2}/I_{1} is greater than 9 for XX but only about 2 for YY. Explain this difference.
  • d) The electron affinity of chlorine is −349-349 kJ/mol, that of magnesium is positive, and the second electron affinity of oxygen (O−+e−→O2−O^{-}+e^{-}\rightarrow O^{2-}) is always positive. Explain these three facts, then say how the O2−O^{2-} ion can nevertheless exist in solid MgOMgO.

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  • a) XX: 1 valence electron, YY: 2, ZZ: 3, so groups 1, 2 and 13
  • b) X=NaX=Na, Y=MgY=Mg, Z=AlZ=Al, ions Na+Na^{+}, Mg2+Mg^{2+} and Al3+Al^{3+}, all [Ne][Ne]
  • c) 9.2 against 1.97: for XX the second electron comes from the core, for YY from the valence shell
  • d) ClCl completes the octet, MgMg must open a 3p3p, O−O^{-} repels; O2−O^{2-} is held by the lattice energy
a)

Element XX: the jump occurs between I1I_{1} and I2I_{2} (from 496 to 4562, a factor of 9.2), so there is only one valence electron: group 1 (alkali metals). Element YY: the jump is between I2I_{2} and I3I_{3} (1451 then 7733, a factor of 5.3), so two valence electrons: group 2 (alkaline earth metals). Element ZZ: the jump is between I3I_{3} and I4I_{4} (2745 then 11577, a factor of 4.2), so three valence electrons: group 13.

b)

In the third period, this gives X=NaX=Na with configuration [Ne]3s1[Ne]3s^{1}, Y=MgY=Mg with configuration [Ne]3s2[Ne]3s^{2}, and Z=AlZ=Al with configuration [Ne]3s23p1[Ne]3s^{2}3p^{1}. Each ionizes until it recovers the [Ne][Ne] core and no further, hence the ions Na+Na^{+}, Mg2+Mg^{2+} and Al3+Al^{3+}, all isoelectronic with neon. The measured values confirm what the configuration predicts: the number of electrons that are easy to remove is exactly the number of valence electrons.

c)

For XX, removing the first electron empties the valence shell: the Na+Na^{+} ion is already [Ne][Ne]. The second electron must then be taken from the n=2n=2 shell, much closer to the nucleus, far less shielded, and part of an especially stable noble gas configuration: the cost explodes. For YY, the second electron is still a 3s3s electron, from the same valence shell. Only the charge of the ion has changed, going from 0 to +1+1, which increases the attraction without changing shell: the cost only roughly doubles. The rule to remember is that the sharp jump does not measure the charge, it signals the passage into the electron core.

d)

Chlorine [Ne]3s23p5[Ne]3s^{2}3p^{5} needs only one electron to reach the argon configuration: capture is very favourable, strongly exothermic, so the electron affinity is very negative. Magnesium [Ne]3s2[Ne]3s^{2} has its 3s3s subshell complete; the extra electron would have to enter a 3p3p orbital, higher in energy and well shielded by the 3s3s electrons: the process costs energy, and the electron affinity is positive. For oxygen, the second capture requires bringing an electron up to an O−O^{-} ion that is already negative: the electrostatic repulsion must be overcome, and that always costs energy, whatever the element. The O2−O^{2-} ion is therefore never stable in isolation. It nevertheless exists in MgOMgO because the energy balance does not stop at the free ion: the lattice energy released when Mg2+Mg^{2+} and O2−O^{2-} ions stack into a crystal lattice is enormous, precisely because both ions carry a double charge, and it more than compensates for the cost of the second capture. The stability of O2−O^{2-} comes from the solid, not from the ion.

123456−40004000800012000160002000073814517733example: magnesiumthe JUMP between the 2nd and 3rd reveals2 valence electronsionization numberE (kJ/mol)

Exercise 10: Problem: the hydrogen lamp and the ionization energy

A discharge lamp filled with hydrogen emits the Balmer series, that is, the photons produced when an electron falls back to level n=2n=2. Keep En=−2.18×10−18n2E_{n}=-\dfrac{2.18\times 10^{-18}}{n^{2}} J, h=6.626×10−34h=6.626\times 10^{-34} J·s, c=3.00×108c=3.00\times 10^{8} m/s and NA=6.022×1023N_{A}=6.022\times 10^{23} /mol. The diagram below shows the setup.

H₂discharge tubehigh voltageprismscreen
  • a) Calculate the wavelength of the line emitted in the n=4→n=2n=4\rightarrow n=2 transition. What colour does it correspond to?
  • b) Calculate the energy needed to completely ionize a hydrogen atom from its ground state (n=1→n=∞n=1\rightarrow n=\infty), first in joules per atom, then in kilojoules per mole.
  • c) The limit of the Balmer series corresponds to the n=∞→n=2n=\infty\rightarrow n=2 transition. Calculate its wavelength and explain what it represents physically.

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  • a) λ=486\lambda=486 nm, the blue-green Balmer line
  • b) 2.18×10−182.18\times 10^{-18} J per atom, that is 1313 kJ/mol
  • c) λ=365\lambda=365 nm: the series limit, the most energetic photon, in the ultraviolet
a)

∣ΔE∣=2.18×10−18(122−142)=2.18×10−18(0.25−0.0625)=4.09×10−19|\Delta E|=2.18\times 10^{-18}\left(\dfrac{1}{2^{2}}-\dfrac{1}{4^{2}}\right)=2.18\times 10^{-18}(0.25-0.0625)=4.09\times 10^{-19} J. Then λ=hc∣ΔE∣=(6.626×10−34)(3.00×108)4.09×10−19=4.86×10−7\lambda=\dfrac{hc}{|\Delta E|}=\dfrac{(6.626\times 10^{-34})(3.00\times 10^{8})}{4.09\times 10^{-19}}=4.86\times 10^{-7} m, that is 486 nm: a blue-green (cyan) line in the visible.

b)

To ionize from the ground state is to bring the electron from n=1n=1 to n=∞n=\infty: ∣ΔE∣=E∞−E1=0−(−2.18×10−18)=2.18×10−18|\Delta E|=E_{\infty}-E_{1}=0-(-2.18\times 10^{-18})=2.18\times 10^{-18} J per atom. Per mole: 2.18×10−18×6.022×1023=1.31×1062.18\times 10^{-18}\times 6.022\times 10^{23}=1.31\times 10^{6} J/mol, or about 1313 kJ/mol. This is the well-known value of the ionization energy of hydrogen.

c)

∣ΔE∣=2.18×10−18(122−0)=5.45×10−19|\Delta E|=2.18\times 10^{-18}\left(\dfrac{1}{2^{2}}-0\right)=5.45\times 10^{-19} J, so λ=hc∣ΔE∣=(6.626×10−34)(3.00×108)5.45×10−19=3.65×10−7\lambda=\dfrac{hc}{|\Delta E|}=\dfrac{(6.626\times 10^{-34})(3.00\times 10^{8})}{5.45\times 10^{-19}}=3.65\times 10^{-7} m, that is 365 nm, in the ultraviolet. This wavelength is the shortest of the whole Balmer series: it corresponds to the most energetic photon, emitted when the electron falls from an infinitely high level (just at the ionization threshold) to n=2n=2. All the other lines of the series have a longer wavelength and converge toward this limit.

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