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Atomic Structure & Periodicity

Subatomic Particles

Atoms consist of three principal subatomic particles. Their properties are summarised below.

PropertyProtonNeutronElectron
Symbolpp or p+p^+nn or n0n^0ee^-
Relative charge+1+1001-1
Charge (C)+1.602×1019+1.602 \times 10^{-19}001.602×1019-1.602 \times 10^{-19}
Relative mass1.007281.007281.008671.008670.000550.00055 (1/1836\approx 1/1836)
LocationNucleusNucleusElectron shells / orbitals
Spin+12+\tfrac{1}{2}+12+\tfrac{1}{2}+12+\tfrac{1}{2}

The atomic number (proton number) ZZ defines the element. The mass number A=Z+NA = Z + N, where NN is the neutron number. The notation is:

ZAX{}^{A}_{Z}\mathrm{X}

Isotopes

Isotopes are atoms of the same element (same ZZ) with different neutron numbers (different AA). Chemical properties are virtually identical because they share the same electron configuration. Physical properties (melting point, density, reaction rate) differ slightly due to mass effects.

Relative Atomic Mass (ArA_r)

The relative atomic mass is the weighted mean of the isotopic masses, weighted by their natural abundances:

Ar(X)=LBimiaiRB◆◆LBiaiRBA_r(\mathrm{X}) = \frac◆LB◆\sum_i m_i \cdot a_i◆RB◆◆LB◆\sum_i a_i◆RB◆

where mim_i is the isotopic mass and aia_i is the relative abundance of isotope ii.

Worked Example. Chlorine has two stable isotopes: 35Cl{}^{35}\mathrm{Cl} (75.77%, m=34.969um = 34.969\,\mathrm{u}) and 37Cl{}^{37}\mathrm{Cl} (24.23%, m=36.966um = 36.966\,\mathrm{u}).

Ar(Cl)=(34.969)(75.77)+(36.966)(24.23)100=2650.4+895.3100=35.45A_r(\mathrm{Cl}) = \frac{(34.969)(75.77) + (36.966)(24.23)}{100} = \frac{2650.4 + 895.3}{100} = 35.45

Relative Molecular Mass (MrM_r)

For a compound with formula XaYb\mathrm{X}_a\mathrm{Y}_b:

Mr=aAr(X)+bAr(Y)M_r = a \cdot A_r(\mathrm{X}) + b \cdot A_r(\mathrm{Y})

Mass Spectrometry

Mass spectrometry separates ions by their mass-to-charge ratio (m/zm/z). The stages are:

  1. Vaporisation -- sample converted to gaseous state.
  2. Ionisation -- typically by electron impact (EI): a high-energy electron beam ejects an electron from the sample molecule, producing a molecular ion M+\mathrm{M}^{+\bullet}.
  3. Acceleration -- ions accelerated through a potential difference VV, gaining kinetic energy 12mv2=zVe\tfrac{1}{2}mv^2 = zVe.
  4. Deflection -- a magnetic field BB deflects ions into a curved path of radius rr:
r=LB2mV/zRB◆◆LBBRBr = \frac◆LB◆\sqrt{2mV/z}◆RB◆◆LB◆B◆RB◆

Lighter ions (lower m/zm/z) are deflected more. The detector records the abundance at each m/zm/z.

  1. Detection -- ions strike the detector, generating a current proportional to their abundance.

Interpreting Mass Spectra

  • The molecular ion peak (M+\mathrm{M}^{+\bullet}) gives the relative molecular mass.
  • Fragmentation produces characteristic peaks. For example, CH4+\mathrm{CH}_4^{+\bullet} at m/z=16m/z = 16; CH3+\mathrm{CH}_3^+ at m/z=15m/z = 15.
  • The base peak is the most intense signal (assigned 100% relative abundance).

Worked Example. A compound shows a molecular ion peak at m/z=78m/z = 78 and a base peak at m/z=77m/z = 77. The M+1 peak at m/z=79m/z = 79 has 6.4% of the molecular ion intensity. This is consistent with benzene (C6H6\mathrm{C}_6\mathrm{H}_6, Mr=78M_r = 78). The M+1 peak intensity (6×1.1%=6.6%\approx 6 \times 1.1\% = 6.6\%) confirms six carbon atoms.

Electron Configuration

Quantum Numbers

Each electron in an atom is described by four quantum numbers:

Quantum NumberSymbolValuesDescribes
Principalnn1,2,3,1, 2, 3, \ldotsEnergy level / shell
Azimuthal\ell0,1,,n10, 1, \ldots, n-1Subshell type (0=s0 = s, 1=p1 = p, 2=d2 = d)
Magneticmm_\ell,+1,,+-\ell, -\ell+1, \ldots, +\ellOrbital orientation
Spinmsm_s+12,12+\tfrac{1}{2}, -\tfrac{1}{2}Electron spin direction

Subshell Capacities

Subshell\ellOrbitalsMax Electrons
ss001122
pp113366
dd22551010
ff33771414

The maximum number of electrons in shell nn is 2n22n^2.

Aufbau Principle

Electrons occupy the lowest energy subshells first. The filling order is:

1s<2s<2p<3s<3p<4s<3d<4p<5s<4d<5p<6s<4f<5d<6p<7s1s \lt 2s \lt 2p \lt 3s \lt 3p \lt 4s \lt 3d \lt 4p \lt 5s \lt 4d \lt 5p \lt 6s \lt 4f \lt 5d \lt 6p \lt 7s

The 4s4s subshell fills before 3d3d because its energy is lower for Z20Z \le 20. For Z>20Z \gt 20, the energies shift and 3d3d becomes lower -- this is important for transition metals (see Transition Metals).

Pauli Exclusion Principle

No two electrons in the same atom can have the same set of four quantum numbers. Consequently, each orbital holds at most two electrons, with opposite spins.

Hund's Rule

Within a given subshell, electrons occupy degenerate orbitals singly first, with parallel spins, before pairing. This minimises electron-electron repulsion and maximises total spin.

Writing Electron Configurations

Use the notation nxn\ell^x where xx is the number of electrons in that subshell.

ElementZZConfigurationShorthand
H11s11s^11s11s^1
C61s22s22p21s^2 2s^2 2p^2[He]2s22p2[\mathrm{He}]\,2s^2 2p^2
Na111s22s22p63s11s^2 2s^2 2p^6 3s^1[Ne]3s1[\mathrm{Ne}]\,3s^1
Fe261s22s22p63s23p64s23d61s^2 2s^2 2p^6 3s^2 3p^6 4s^2 3d^6[Ar]4s23d6[\mathrm{Ar}]\,4s^2 3d^6
Cu291s22s22p63s23p64s13d101s^2 2s^2 2p^6 3s^2 3p^6 4s^1 3d^{10}[Ar]4s13d10[\mathrm{Ar}]\,4s^1 3d^{10}

Note on Cr and Cu. Chromium (Z=24Z = 24) is [Ar]4s13d5[\mathrm{Ar}]\,4s^1 3d^5 and copper (Z=29Z = 29) is [Ar]4s13d10[\mathrm{Ar}]\,4s^1 3d^{10}. The half-filled d5d^5 and fully-filled d10d^{10} configurations are stabilised by exchange energy -- the extra stability gained from maximising parallel spins outweighs the energy cost of promoting an electron from 4s4s to 3d3d.

d-block Electron Configurations

For transition metals, when forming cations, the 4s4s electrons are removed before the 3d3d electrons. For example:

  • Fe\mathrm{Fe}: [Ar]4s23d6[\mathrm{Ar}]\,4s^2 3d^6
  • Fe2+\mathrm{Fe}^{2+}: [Ar]3d6[\mathrm{Ar}]\,3d^6
  • Fe3+\mathrm{Fe}^{3+}: [Ar]3d5[\mathrm{Ar}]\,3d^5

This is because once the 3d3d subshell begins to populate, it drops below 4s4s in energy.

Ionisation Energy

Definition

The first ionisation energy of an element is the enthalpy change when one mole of gaseous atoms each loses one electron to form one mole of gaseous 1+1+ ions:

X(g)X+(g)+eΔH=IE1\mathrm{X}(g) \to \mathrm{X}^+(g) + e^- \quad \Delta H = \mathrm{IE}_1

The second ionisation energy is:

X+(g)X2+(g)+eΔH=IE2\mathrm{X}^+(g) \to \mathrm{X}^{2+}(g) + e^- \quad \Delta H = \mathrm{IE}_2

Ionisation energies are always endothermic (positive ΔH\Delta H).

General Trend Across a Period

Ionisation energy generally increases across a period (left to right) because:

  1. Nuclear charge increases -- each successive element adds one proton to the nucleus.
  2. Shielding increases negligibly -- additional electrons enter the same shell, so the shielding effect of inner electrons remains approximately constant.
  3. Atomic radius decreases -- the increased effective nuclear charge pulls electron shells closer.
  4. Net effect -- the outer electron is held more tightly, requiring more energy to remove.
ElementZZConfigurationIE1\mathrm{IE}_1 (kJ/mol)
Na11[Ne]3s1[\mathrm{Ne}]\,3s^1496
Mg12[Ne]3s2[\mathrm{Ne}]\,3s^2738
Al13[Ne]3s23p1[\mathrm{Ne}]\,3s^2 3p^1578
Si14[Ne]3s23p2[\mathrm{Ne}]\,3s^2 3p^2786
P15[Ne]3s23p3[\mathrm{Ne}]\,3s^2 3p^31012
S16[Ne]3s23p4[\mathrm{Ne}]\,3s^2 3p^41000
Cl17[Ne]3s23p5[\mathrm{Ne}]\,3s^2 3p^51251
Ar18[Ne]3s23p6[\mathrm{Ne}]\,3s^2 3p^61521

Anomalies: Al vs Mg and S vs P

Al (578) < Mg (738). The electron removed from Al is a 3p3p electron, which is in a higher energy subshell than the 3s3s electrons of Mg. The 3p3p electron is further from the nucleus on average and experiences greater shielding from the 3s3s electrons.

S (1000) < P (1012). In P (3p33p^3), each 3p3p orbital contains one electron. In S (3p43p^4), one orbital must contain two paired electrons. Pairing introduces electron-electron repulsion within the same orbital, which slightly reduces the energy required to remove one of the paired electrons.

Trend Down a Group

Ionisation energy decreases down a group because:

  1. Principal quantum number increases -- outer electrons occupy shells further from the nucleus.
  2. Shielding increases -- additional inner shells screen the nuclear charge.
  3. Atomic radius increases -- the outer electron is further from the nucleus.
  4. Net effect -- despite increasing nuclear charge, the increased distance and shielding dominate, making electron removal easier.

| Element | IE1\mathrm{IE}_1 (kJ/mol) | |---| | Li | 520 | | Na | 496 | | K | 419 | | Rb | 403 |

Successive Ionisation Energies

Plotting successive ionisation energies (IE1\mathrm{IE}_1, IE2\mathrm{IE}_2, IE3\mathrm{IE}_3, ...) against ionisation number reveals the electron configuration. Large jumps occur when electrons are removed from a new inner shell.

Worked Example. For aluminium (Z=13Z = 13), successive ionisation energies are:

nnIEn\mathrm{IE}_n (kJ/mol)Shell
1578n=3n = 3
21817n=3n = 3
32745n=3n = 3
411577n=2n = 2 (jump)

The large jump between IE3\mathrm{IE}_3 and IE4\mathrm{IE}_4 indicates that the first three electrons were removed from the third shell (valence), and the fourth is removed from the second shell (core).

Atomic and Ionic Radii

Atomic Radius

The atomic radius is the distance from the nucleus to the outermost electrons. It cannot be measured directly; instead, half the internuclear distance in a covalent bond or metallic lattice is used (covalent radius or metallic radius).

Trend across a period: Atomic radius decreases. Increasing nuclear charge pulls electrons closer without a compensating increase in shielding (same shell).

Trend down a group: Atomic radius increases. Each successive element adds a new electron shell.

Ionic Radius

Cations are smaller than their parent atoms because removing electrons reduces electron-electron repulsion and the remaining electrons are drawn closer by the unchanged nuclear charge. Higher charge cations are even smaller: Fe3+<Fe2+<Fe\mathrm{Fe}^{3+} \lt \mathrm{Fe}^{2+} \lt \mathrm{Fe}.

Anions are larger than their parent atoms because adding electrons increases electron-electron repulsion, causing the electron cloud to expand. For isoelectronic species (same number of electrons), the ionic radius decreases with increasing nuclear charge:

O2>F>Na+>Mg2+>Al3+\mathrm{O}^{2-} \gt \mathrm{F}^- \gt \mathrm{Na}^+ \gt \mathrm{Mg}^{2+} \gt \mathrm{Al}^{3+}

All have the neon electron configuration (1s22s22p61s^2 2s^2 2p^6), but nuclear charge increases from 8 to 13.

Shielding and Effective Nuclear Charge

Shielding Constant (σ\sigma)

The shielding constant σ\sigma quantifies the extent to which inner electrons screen the nuclear charge from a valence electron. A simplified model (Slater's rules) assigns:

  • Electrons in the same group (ns,npns, np): shield with efficiency 0.350.35 each (except 1s1s: 0.300.30).
  • Electrons in the (n1)(n-1) shell: shield with efficiency 0.850.85.
  • Electrons in shells (n2)\le (n-2): shield with efficiency 1.001.00.

Effective Nuclear Charge (ZeffZ_\mathrm{eff})

Zeff=ZσZ_\mathrm{eff} = Z - \sigma

Worked Example. For potassium (Z=19Z = 19, configuration 1s22s22p63s23p64s11s^2 2s^2 2p^6 3s^2 3p^6 4s^1), the shielding experienced by the 4s4s electron:

σ=(8×0.85)+(10×1.00)=6.8+10.0=16.8\sigma = (8 \times 0.85) + (10 \times 1.00) = 6.8 + 10.0 = 16.8 Zeff=1916.8=2.2Z_\mathrm{eff} = 19 - 16.8 = 2.2

This low effective nuclear charge explains why the 4s4s electron is so easily lost (low first ionisation energy of K).

For calcium (Z=20Z = 20, 4s24s^2), each 4s4s electron experiences:

σ=(1×0.35)+(8×0.85)+(10×1.00)=0.35+6.8+10.0=17.15\sigma = (1 \times 0.35) + (8 \times 0.85) + (10 \times 1.00) = 0.35 + 6.8 + 10.0 = 17.15 Zeff=2017.15=2.85Z_\mathrm{eff} = 20 - 17.15 = 2.85

The higher ZeffZ_\mathrm{eff} for Ca compared to K explains the higher first ionisation energy of Ca (590 vs 419 kJ/mol).

PropertyAcross a periodDown a group
Atomic radiusDecreasesIncreases
Ionic radius (same charge)DecreasesIncreases
First ionisation energyGenerally increasesDecreases
ElectronegativityIncreasesDecreases
Metallic characterDecreasesIncreases
Melting point (metals)IncreasesDecreases
Melting point (non-metals)VariableVariable

Practice Problems

Problem 1

Bromine has two stable isotopes: 79Br{}^{79}\mathrm{Br} (50.69%) and 81Br{}^{81}\mathrm{Br} (49.31%). Calculate the relative atomic mass of bromine.

Solution:

Ar(Br)=LB(79×50.69)+(81×49.31)RB◆◆LB100RB=4004.5+3994.1100=79.9980.0A_r(\mathrm{Br}) = \frac◆LB◆(79 \times 50.69) + (81 \times 49.31)◆RB◆◆LB◆100◆RB◆ = \frac{4004.5 + 3994.1}{100} = 79.99 \approx 80.0
Problem 2

The first five ionisation energies of an element XX are (in kJ/mol): 590, 1145, 4912, 6491, 8153. Identify the group of element XX.

Solution:

The large jump between IE2\mathrm{IE}_2 (1145) and IE3\mathrm{IE}_3 (4912) indicates that the third electron is being removed from a new, inner shell. This means XX has two valence electrons and belongs to Group 2. The first ionisation energy (590 kJ/mol) is consistent with calcium.

Problem 3

Write the electron configuration of Cr3+\mathrm{Cr}^{3+} and explain why it has a d3d^3 configuration.

Solution:

Chromium (Z=24Z = 24) has the ground-state configuration [Ar]4s13d5[\mathrm{Ar}]\,4s^1 3d^5. When forming Cr3+\mathrm{Cr}^{3+}, the 4s4s electrons are removed first (as they are higher in energy once the 3d3d subshell is populated), followed by one 3d3d electron:

Cr3+:[Ar]3d3\mathrm{Cr}^{3+}: [\mathrm{Ar}]\,3d^3

The d3d^3 configuration has one electron in each of three dd orbitals with parallel spins, which is stabilised by exchange energy (Hund's rule). This half-filled-like arrangement is relatively stable.

Problem 4

Explain why the first ionisation energy of oxygen is less than that of nitrogen.

Solution:

Nitrogen (1s22s22p31s^2 2s^2 2p^3) has three unpaired 2p2p electrons, one in each 2p2p orbital (Hund's rule). Oxygen (1s22s22p41s^2 2s^2 2p^4) has four 2p2p electrons, so one orbital must contain a pair. Removing an electron from oxygen means removing one of the paired electrons from the doubly-occupied orbital. The pairing repulsion in that orbital makes the electron less tightly held than a nitrogen 2p2p electron, so oxygen has a lower first ionisation energy.

Problem 5

The mass spectrum of an element shows three peaks at m/z=52m/z = 52, 54, and 56 with relative abundances 17.4%, 67.8%, and 14.8% respectively. (a) Identify the element. (b) Explain the pattern.

Solution:

(a) The element is chromium (Cr\mathrm{Cr}, Z=24Z = 24, Ar52A_r \approx 52). The peaks correspond to 52Cr{}^{52}\mathrm{Cr}, 54Cr{}^{54}\mathrm{Cr}, and 56Cr{}^{56}\mathrm{Cr}.

(b) Chromium has four stable isotopes: 50Cr{}^{50}\mathrm{Cr} (4.3%), 52Cr{}^{52}\mathrm{Cr} (83.8%), 53Cr{}^{53}\mathrm{Cr} (9.5%), and 54Cr{}^{54}\mathrm{Cr} (2.4%). However, the data shows three peaks at 52, 54, and 56, which is more consistent with iron (Fe\mathrm{Fe}, Z=26Z = 26): 54Fe{}^{54}\mathrm{Fe} (5.8%), 56Fe{}^{56}\mathrm{Fe} (91.7%), 57Fe{}^{57}\mathrm{Fe} (2.1%), and 58Fe{}^{58}\mathrm{Fe} (0.3%).

Re-examining: the m/zm/z values of 52, 54, 56 with the given abundances most closely match chromium: 52Cr{}^{52}\mathrm{Cr} (Ar=51.94A_r = 51.94, abundance 83.8%\approx 83.8\%), 53Cr{}^{53}\mathrm{Cr} (Ar=52.94A_r = 52.94, 9.5%\approx 9.5\%), 54Cr{}^{54}\mathrm{Cr} (Ar=53.94A_r = 53.94, 2.4%\approx 2.4\%). However, the relative abundances in the problem (17.4%, 67.8%, 14.8%) do not match chromium's known isotope pattern.

The correct identification requires the data to be internally consistent: Ar=52×0.174+54×0.678+56×0.148=9.05+36.61+8.29=53.95A_r = 52 \times 0.174 + 54 \times 0.678 + 56 \times 0.148 = 9.05 + 36.61 + 8.29 = 53.95. This value (54\approx 54) is closest to chromium, but the isotope pattern does not match natural abundance. The element is therefore most likely chromium with the mass spectrum showing a simplified or experimental dataset.

Mass Spectrometry in Detail

High-Resolution Mass Spectrometry

Low-resolution mass spectrometry gives m/zm/z to the nearest integer. High-resolution MS gives m/zm/z to several decimal places, allowing distinction between species with the same nominal mass:

SpeciesExact mass (m/zm/z)Nominal mass
C3H8\mathrm{C}_3\mathrm{H}_844.06344
CO2\mathrm{CO}_243.99044
N2O\mathrm{N}_2\mathrm{O}44.00144
C2H4O\mathrm{C}_2\mathrm{H}_4\mathrm{O}44.02644

High-resolution MS can distinguish C3H8\mathrm{C}_3\mathrm{H}_8 (44.06344.063) from CO2\mathrm{CO}_2 (43.99043.990) -- a difference of 0.073amu0.073\,\mathrm{amu}, easily resolved by modern instruments.

The Rule of 13

The rule of 13 provides possible molecular formulas from the molecular ion peak:

Mr=13n+rM_r = 13n + r

where nn is the number of carbon atoms and rr is the number of hydrogen atoms (plus halogens counted as hydrogen equivalents: F = H, Cl = H + 35, Br = H + 79, I = H + 127).

Example. For Mr=92M_r = 92: 92=13×7+192 = 13 \times 7 + 1. Base formula: C7H1\mathrm{C}_7\mathrm{H}_1. This is unrealistic (too few H for 7 C), so subtract 6 H and add one degree of unsaturation: C7H8\mathrm{C}_7\mathrm{H}_8. Possible structures: toluene (C6H5CH3\mathrm{C}_6\mathrm{H}_5\mathrm{CH}_3) or methylcyclohexene.

Isotope Peaks in Mass Spectrometry

The M+1 peak provides a way to estimate the number of carbon atoms:

Number of carbonsLB%intensity of M+1◆RB◆◆LB1.1RB\text{Number of carbons} \approx \frac◆LB◆\%\,\text{intensity of M+1}◆RB◆◆LB◆1.1◆RB◆

Worked Example. A compound has a molecular ion at m/z=150m/z = 150 (100%) and M+1 at m/z=151m/z = 151 (9.9%). Estimate the number of carbons.

n(C)9.91.1=9n(\mathrm{C}) \approx \frac{9.9}{1.1} = 9

The compound likely contains 9 carbon atoms. 12×9=10812 \times 9 = 108. Remaining mass = 150108=42150 - 108 = 42. This could correspond to C2H2O\mathrm{C}_2\mathrm{H}_2\mathrm{O} (or other combinations). The rule of 13 confirms: 150=13×11+7150 = 13 \times 11 + 7, so the base formula is C11H7\mathrm{C}_{11}\mathrm{H}_7. With 9 carbons, the formula becomes C9H10O\mathrm{C}_9\mathrm{H}_{10}\mathrm{O} (Mr=9×12+10+16=138M_r = 9 \times 12 + 10 + 16 = 138, which does not match). The calculation illustrates the method but requires additional information (like the M+2 peak for halogens) for unambiguous determination.

Exceptions to the Aufbau Principle

The following elements have ground-state configurations that deviate from the simple Aufbau prediction:

ElementExpectedActualReason
Cr (Z=24Z=24)[Ar]4s23d4[\mathrm{Ar}]\,4s^2 3d^4[Ar]4s13d5[\mathrm{Ar}]\,4s^1 3d^5Half-filled dd subshell is stabilised by exchange energy
Cu (Z=29Z=29)[Ar]4s23d9[\mathrm{Ar}]\,4s^2 3d^9[Ar]4s13d10[\mathrm{Ar}]\,4s^1 3d^{10}Fully-filled dd subshell is stabilised

The exchange energy arises because electrons with parallel spins (Hund's rule) cannot occupy the same region of space (Pauli exclusion), which reduces electron-electron repulsion. The energy gained from exchange stabilisation can exceed the energy difference between 4s4s and 3d3d orbitals.

Across a period: IE generally increases because:

  1. Nuclear charge increases (stronger attraction to electrons).
  2. Atomic radius decreases (electrons are closer to the nucleus).
  3. Shielding increases only slightly (inner electrons screen imperfectly).

Down a group: IE decreases because:

  1. Atomic radius increases significantly (outermost electron is further from the nucleus).
  2. Shielding increases (more inner electron shells).

Exceptions across Period 2:

  • Be (IE>B\mathrm{IE} \gt \mathrm{B}): Be has a filled 2s2s subshell (2s22s^2), which is relatively stable. B has 2s22p12s^2 2p^1, and the 2p2p electron is higher in energy and easier to remove.
  • N (IE>O\mathrm{IE} \gt \mathrm{O}): N has a half-filled 2p2p subshell (2p32p^3), which is stabilised by exchange energy. O has 2p42p^4 with pairing repulsion in one orbital.

Successive Ionisation Energies

Successive ionisation energies (IE1\mathrm{IE}_1, IE2\mathrm{IE}_2, IE3\mathrm{IE}_3, ...) always increase because each electron is removed from an increasingly positive ion. Large jumps indicate that the electron is being removed from a new, inner shell closer to the nucleus.

Worked Example. The first five ionisation energies of an element are (in kJ/mol\mathrm{kJ/mol}): 578578, 18171817, 27452745, 1157811578, 1484214842.

The large jump between IE3\mathrm{IE}_3 and IE4\mathrm{IE}_4 indicates that the first three electrons are removed from the outer shell, and the fourth is removed from an inner shell. The element is in Group 13 (three valence electrons). This is aluminium.

Using Ionisation Energy Data to Identify Elements

A plot of log(IE)\log(\mathrm{IE}) vs ionisation number shows clear steps corresponding to the removal of electrons from different shells. The number of electrons in each step gives the group number.

ElementIE1\mathrm{IE}_1 (kJ/mol\mathrm{kJ/mol})GroupEvidence
Na496496, 45624562, ...1Large jump after 1st
Mg738738, 14511451, 77337733, ...2Large jump after 2nd
Al578578, 18171817, 27452745, 1157811578, ...13Large jump after 3rd
Si789789, 15771577, 32283228, 43564356, 1609116091, ...14Large jump after 4th
PropertyNaMgAlSiPSClAr
IE1\mathrm{IE}_1 (kJ/mol\mathrm{kJ/mol})4967385787891012100012511521
Atomic radius (pm\mathrm{pm})18616014311811010499--
Melting point (C^\circ\mathrm{C})98650661141444115101-101189-189
Electrical conductivityGoodGoodGoodPoor (semiconductor)PoorPoorPoorPoor

Melting point anomaly: Silicon has the highest melting point because it has a giant covalent (macromolecular) structure with strong covalent bonds throughout. Sulphur has a higher melting point than phosphorus because S8S_8 molecules are larger and have more London forces than P4P_4 molecules.

Metallic vs Non-Metallic Character

Metallic character decreases across a period (increasing nuclear charge pulls electrons closer, making them harder to lose) and increases down a group (increasing atomic radius makes electron loss easier).

Non-metallic character follows the opposite trend: it increases across a period and decreases down a group.

The diagonal relationship: Elements diagonally adjacent in the periodic table (e.g. Li and Mg, Be and Al) show similar properties due to similar charge-to-radius ratios.

Additional Practice Problems

Problem 4

The first four ionisation energies of an element X are: 738738, 14511451, 77337733, and 10540kJ/mol10540\,\mathrm{kJ/mol}. Identify the element and explain the pattern.

Solution:

The large jump between the second (14511451) and third (77337733) ionisation energies indicates that removing the third electron requires breaking into a new, inner electron shell. The element has two valence electrons and is in Group 2.

The element is magnesium (Mg\mathrm{Mg}, Z=12Z = 12, electron configuration [Ne]3s2[\mathrm{Ne}]\,3s^2). The first two electrons are removed from the 3s3s subshell (valence); the third must be removed from the 2p2p subshell (core), which is much closer to the nucleus and more tightly held.

Problem 5

A mass spectrum shows the following peaks for an organic compound: m/z=78m/z = 78 (M+, base peak), 79 (M+1, 6.7% of M+), 80 (M+2, 0.5% of M+). No significant peaks at m/z>80m/z > 80.

(a) Suggest the molecular formula. (b) Identify the compound.

Solution:

(a) M+1 = 6.7% suggests approximately 6.7/1.1=66.7/1.1 = 6 carbons. C6H6\mathrm{C}_6\mathrm{H}_6: M=72M = 72 (too low). C6H6\mathrm{C}_6\mathrm{H}_6... M=6(12)+6(1)=78M = 6(12) + 6(1) = 78. Check: M+2 = 0.5%, consistent with approximately 6 carbons (each 13C^{13}\mathrm{C} contributes 1.1%, and 6×1.1=6.6%6 \times 1.1 = 6.6\%; M+2 from two 13C^{13}\mathrm{C} atoms: C(6,2)×(0.011)215×0.000121=0.18%C(6,2) \times (0.011)^2 \approx 15 \times 0.000121 = 0.18\%, plus other contributions). The data are consistent with C6H6\mathrm{C}_6\mathrm{H}_6.

(b) C6H6\mathrm{C}_6\mathrm{H}_6 is benzene (M=78M = 78). The mass spectrum of benzene characteristically shows the molecular ion as the base peak (highly stable aromatic ring).

Problem 6

Explain why the first ionisation energy of oxygen is lower than that of nitrogen, even though oxygen has a higher nuclear charge.

Solution:

Nitrogen has the electron configuration 1s22s22p31s^2 2s^2 2p^3 with a half-filled 2p2p subshell. Half-filled subshells are stabilised by exchange energy (electrons with parallel spins minimise repulsion due to the Pauli exclusion principle). Removing an electron from this stable configuration requires extra energy.

Oxygen has 1s22s22p41s^2 2s^2 2p^4. The fourth electron in the 2p2p subshell must pair with another electron in one of the pp orbitals. The pairing repulsion between the two electrons in the same orbital partially offsets the increased nuclear charge. This makes the electron easier to remove from oxygen than from nitrogen, despite the higher nuclear charge.

Data: IE1(N)=1402kJ/mol\mathrm{IE}_1(\mathrm{N}) = 1402\,\mathrm{kJ/mol}, IE1(O)=1314kJ/mol\mathrm{IE}_1(\mathrm{O}) = 1314\,\mathrm{kJ/mol}.

Advanced Ionisation Energy Problems

Problem 7

The successive ionisation energies of element X are shown below:

nn1234567891011
IE (kJ/mol\mathrm{kJ/mol})578181727451157814842183772332727466318623721642640

(a) In which group of the periodic table is element X? (1 mark)

(b) Identify element X. (1 mark)

(c) Explain the large jump between the third and fourth ionisation energies. (2 marks)

(d) Predict the formula of the oxide formed by element X. (1 mark)

Solution:

(a) Group 13. The large jump between the 3rd and 4th ionisation energies indicates that the first three electrons are in the outer shell (valence electrons), and the 4th electron is removed from an inner shell.

(b) Aluminium (Al\mathrm{Al}, Z=13Z = 13). The first ionisation energy (578 kJ/mol) matches the known value for aluminium.

(c) The first three electrons are removed from the n=3n = 3 shell (3s23p13s^2 3p^1). The fourth electron must be removed from the n=2n = 2 shell (2p62p^6), which is much closer to the nucleus and more strongly held. The large increase in ionisation energy reflects the transition from valence to core electrons (1 mark for identifying the shell transition, 1 mark for explaining that inner shell electrons experience less shielding and are closer to the nucleus).

(d) Al2O3\mathrm{Al}_2\mathrm{O}_3. Aluminium is in Group 13 and forms a 3+3+ ion. Oxygen forms a 22- ion. The formula requires charge balance: 2×3+=3×22 \times 3+ = 3 \times 2-, giving Al2O3\mathrm{Al}_2\mathrm{O}_3.

Problem 8

A mass spectrum of an organic compound shows the following peaks:

  • m/z=92m/z = 92 (M+, 100% relative intensity)
  • m/z=93m/z = 93 (M+1, 7.7% relative intensity)
  • m/z=94m/z = 94 (M+2, 0.3% relative intensity)
  • m/z=65m/z = 65 (base fragment)
  • m/z=91m/z = 91 (major fragment, tropylium ion)

(a) Determine the molecular formula. (3 marks)

(b) Suggest the identity of the compound. (1 mark)

(c) Explain the origin of the peak at m/z=91m/z = 91. (2 marks)

Solution:

(a) M+1 = 7.7% suggests approximately 7.7/1.1=77.7/1.1 = 7 carbon atoms. 7×12=847 \times 12 = 84. Remaining mass = 9284=892 - 84 = 8, which corresponds to 8 hydrogen atoms. The molecular formula is C7H8\mathrm{C}_7\mathrm{H}_8. Verification: DoU=2(7)+282=4\text{DoU} = \frac{2(7) + 2 - 8}{2} = 4. This is consistent with a benzene ring (4 degrees of unsaturation: one ring + three double bonds in the aromatic system).

M+2 = 0.3% is consistent with two 13C^{13}\mathrm{C} atoms: C(7,2)×(0.011)2=21×0.000121=0.25%C(7,2) \times (0.011)^2 = 21 \times 0.000121 = 0.25\%, close to the observed value.

(b) C7H8\mathrm{C}_7\mathrm{H}_8 is consistent with toluene (C6H5CH3\mathrm{C}_6\mathrm{H}_5\mathrm{CH}_3).

(c) The peak at m/z=91m/z = 91 corresponds to the tropylium ion (C7H7+\mathrm{C}_7\mathrm{H}_7^+), formed by loss of one hydrogen atom from the methyl group followed by ring expansion of the resulting benzyl cation. The tropylium ion has a cyclic, aromatic structure (C7H7+\mathrm{C}_7\mathrm{H}_7^+, 6π6\,\pi electrons satisfying Huckel's rule) that makes it exceptionally stable, explaining its high intensity in the mass spectrum.

Electron Configuration and Periodicity in Detail

Shielding and Penetration Effects

Not all electrons in the same principal shell shield equally. The ss orbital penetrates closer to the nucleus than the pp orbital, and pp penetrates closer than dd. This means:

  • ss electrons experience less shielding (higher ZeffZ_\mathrm{eff}) than pp electrons in the same shell.
  • The 4s4s orbital is lower in energy than 3d3d for Z20Z \le 20 because the 4s4s electron penetrates through the inner shell electron cloud more effectively.
  • For Z>20Z > 20, the increasing nuclear charge pulls the 3d3d electrons closer, and 3d3d drops below 4s4s in energy.

Effective Nuclear Charge Calculations for Period 3

ElementZZConfigurationσ\sigmaZeffZ_\mathrm{eff} (valence)
Na11[Ne]3s1[\mathrm{Ne}]3s^110×0.85=8.510 \times 0.85 = 8.5118.5=2.511 - 8.5 = 2.5
Mg12[Ne]3s2[\mathrm{Ne}]3s^21×0.35+10×0.85=8.851 \times 0.35 + 10 \times 0.85 = 8.85128.85=3.1512 - 8.85 = 3.15
Al13[Ne]3s23p1[\mathrm{Ne}]3s^2 3p^12×0.35+10×0.85=9.202 \times 0.35 + 10 \times 0.85 = 9.20139.20=3.8013 - 9.20 = 3.80
Si14[Ne]3s23p2[\mathrm{Ne}]3s^2 3p^23×0.35+10×0.85=9.553 \times 0.35 + 10 \times 0.85 = 9.55149.55=4.4514 - 9.55 = 4.45
P15[Ne]3s23p3[\mathrm{Ne}]3s^2 3p^34×0.35+10×0.85=9.904 \times 0.35 + 10 \times 0.85 = 9.90159.90=5.1015 - 9.90 = 5.10
S16[Ne]3s23p4[\mathrm{Ne}]3s^2 3p^45×0.35+10×0.85=10.255 \times 0.35 + 10 \times 0.85 = 10.251610.25=5.7516 - 10.25 = 5.75
Cl17[Ne]3s23p5[\mathrm{Ne}]3s^2 3p^56×0.35+10×0.85=10.606 \times 0.35 + 10 \times 0.85 = 10.601710.60=6.4017 - 10.60 = 6.40
Ar18[Ne]3s23p6[\mathrm{Ne}]3s^2 3p^67×0.35+10×0.85=10.957 \times 0.35 + 10 \times 0.85 = 10.951810.95=7.0518 - 10.95 = 7.05

The steady increase in ZeffZ_\mathrm{eff} across the period explains the general increase in first ionisation energy.

The drop from Be to B:

  • IE1(Be)=899kJ/mol\mathrm{IE}_1(\mathrm{Be}) = 899\,\mathrm{kJ/mol} (2s22s^2, filled subshell)
  • IE1(B)=801kJ/mol\mathrm{IE}_1(\mathrm{B}) = 801\,\mathrm{kJ/mol} (2s22p12s^2 2p^1)

The 2p2p electron in boron is shielded by the two 2s2s electrons (which have the same nn value but different \ell). The 2s2s orbital penetrates more effectively than 2p2p, so the 2s2s electrons are held more tightly and shield the 2p2p electron more effectively than 2p2p electrons shield each other. This reduces ZeffZ_\mathrm{eff} for the 2p2p electron, making it easier to remove.

The drop from N to P:

  • IE1(N)=1402kJ/mol\mathrm{IE}_1(\mathrm{N}) = 1402\,\mathrm{kJ/mol} (2p32p^3, half-filled)
  • IE1(O)=1314kJ/mol\mathrm{IE}_1(\mathrm{O}) = 1314\,\mathrm{kJ/mol} (2p42p^4)

In nitrogen (2p32p^3), each pp orbital has one electron (Hund's rule). In oxygen (2p42p^4), one orbital must contain two paired electrons. The pairing energy (exchange energy lost + Coulombic repulsion between paired electrons) makes the fourth electron less tightly held.

Exchange energy stabilisation for half-filled subshells: A half-filled p3p^3 configuration has three electrons with parallel spins. The number of exchange interactions is (32)=3\binom{3}{2} = 3. For p4p^4, the number of parallel spin pairs is (32)=3\binom{3}{2} = 3 (among the three unpaired electrons) plus the exchange between one of the unpaired electrons and the paired electron if spins are parallel. The net exchange stabilisation decreases slightly when the subshell goes from half-filled to more-than-half-filled.

Mass Spectrometry: Fragmentation Patterns

Understanding fragmentation patterns is essential for identifying organic compounds from mass spectra.

Common fragmentation pathways:

Fragmentm/zm/zOrigin
CH3+\mathrm{CH}_3^+15Loss of alkyl group
OH+\mathrm{OH}^+17Alcohols, carboxylic acids
C2H5+\mathrm{C}_2\mathrm{H}_5^+29Ethyl group
CHO+\mathrm{CHO}^+29Aldehydes
CH3CO+\mathrm{CH}_3\mathrm{CO}^+43Methyl ketones
COOH+\mathrm{COOH}^+45Carboxylic acids
C6H5+\mathrm{C}_6\mathrm{H}_5^+77Aromatic compounds
C7H7+\mathrm{C}_7\mathrm{H}_7^+91Benzyl/tropylium ion

Alpha cleavage: The bond adjacent to the carbonyl group breaks, producing an acylium ion. For example, in propanone (CH3COCH3\mathrm{CH}_3\mathrm{COCH}_3), alpha cleavage gives CH3CO+\mathrm{CH}_3\mathrm{CO}^+ at m/z=43m/z = 43 (base peak) and CH3+\mathrm{CH}_3^+ at m/z=15m/z = 15.

McLafferty rearrangement: A hydrogen atom six atoms away from a carbonyl group transfers to the carbonyl oxygen, with simultaneous cleavage of the bond between the α\alpha- and β\beta-carbons. This produces an enol radical cation and a neutral alkene. For butanal (CH3CH2CH2CHO\mathrm{CH}_3\mathrm{CH}_2\mathrm{CH}_2\mathrm{CHO}), McLafferty rearrangement gives C2H4O+\mathrm{C}_2\mathrm{H}_4\mathrm{O}^{+\bullet} at m/z=44m/z = 44.

Exam-Style Questions with Full Mark Schemes

Q1 (4 marks)

Explain why the first ionisation energy of sodium is lower than that of magnesium, and why the first ionisation energy of aluminium is lower than that of magnesium.

Mark Scheme:

Na < Mg (2 marks): Both have electrons in the 3s3s subshell. Magnesium has a higher nuclear charge (Z=12Z = 12 vs Z=11Z = 11) with similar shielding, so the outer electrons are held more tightly, giving a higher ionisation energy (1 mark). The 3s23s^2 configuration of Mg also has the added stability of a filled subshell (1 mark).

Al < Mg (2 marks): The electron removed from Al is a 3p3p electron, which is higher in energy than the 3s3s electrons of Mg (1 mark). The 3p3p electron is further from the nucleus on average and is shielded by the 3s23s^2 electrons, making it easier to remove (1 mark).

Q2 (5 marks)

The mass spectrum of a compound shows a molecular ion peak at m/z=78m/z = 78 (100%) and a base peak at m/z=77m/z = 77 (M-1). The M+1 peak at m/z=79m/z = 79 has 6.7% relative intensity. A significant peak also appears at m/z=51m/z = 51.

(a) Suggest the molecular formula. (2 marks)

(b) Identify the compound. (1 mark)

(c) Explain the peak at m/z=77m/z = 77. (1 mark)

(d) Suggest the identity of the fragment at m/z=51m/z = 51. (1 mark)

Mark Scheme:

(a) M+1 = 6.7% gives approximately 6.7/1.166.7/1.1 \approx 6 carbon atoms (1 mark). C6H6\mathrm{C}_6\mathrm{H}_6: M=72+6=78M = 72 + 6 = 78. Molecular formula: C6H6\mathrm{C}_6\mathrm{H}_6 (1 mark).

(b) Benzene (C6H6\mathrm{C}_6\mathrm{H}_6) (1 mark).

(c) The peak at m/z=77m/z = 77 is C6H5+\mathrm{C}_6\mathrm{H}_5^+ (phenyl cation), formed by loss of one hydrogen atom from the molecular ion (1 mark).

(d) The peak at m/z=51m/z = 51 is C4H3+\mathrm{C}_4\mathrm{H}_3^+, formed by further fragmentation of the phenyl cation (loss of C2H2\mathrm{C}_2\mathrm{H}_2 from C6H5+\mathrm{C}_6\mathrm{H}_5^+: 7726=5177 - 26 = 51) (1 mark).

Q3 (6 marks)

Define the term first ionisation energy. The first five ionisation energies of an element are shown below:

nn12345
IE (kJ/mol\mathrm{kJ/mol})738145177331054013630

(a) Identify the element. (1 mark)

(b) Explain why there is a large increase between the second and third ionisation energies. (2 marks)

(c) Write the electron configuration of the ion formed after the second ionisation. (1 mark)

(d) Explain why the ion in part (c) has a smaller ionic radius than the atom. (2 marks)

Mark Scheme:

(a) Magnesium (Mg\mathrm{Mg}, Z=12Z = 12) (1 mark).

(b) The first two electrons are removed from the 3s3s subshell (valence electrons) (1 mark). The third electron is removed from the 2p2p subshell (core electrons), which is closer to the nucleus and experiences less shielding, so much more energy is required (1 mark).

(c) Mg2+\mathrm{Mg}^{2+}: 1s22s22p61s^2 2s^2 2p^6 or [Ne][\mathrm{Ne}] (1 mark).

(d) When electrons are removed, the remaining electrons experience less electron-electron repulsion and are pulled closer to the nucleus by the unchanged nuclear charge (1 mark). The increased effective nuclear charge per electron reduces the ionic radius (1 mark).

Q4 (5 marks)

High-resolution mass spectrometry gives the molecular ion peak of a compound at m/z=60.0575m/z = 60.0575. Two possible molecular formulas are C3H8O\mathrm{C}_3\mathrm{H}_8\mathrm{O} and C2H4O2\mathrm{C}_2\mathrm{H}_4\mathrm{O}_2.

(a) Calculate the exact mass of each formula. (2 marks)

(b) Identify the correct formula. (1 mark)

(c) The compound gives a positive iodoform test. Suggest the identity of the compound. (2 marks)

Mark Scheme:

(a) C3H8O\mathrm{C}_3\mathrm{H}_8\mathrm{O}: 3(12.0000)+8(1.0078)+15.9949=36.0000+8.0625+15.9949=60.05743(12.0000) + 8(1.0078) + 15.9949 = 36.0000 + 8.0625 + 15.9949 = 60.0574 (1 mark).

C2H4O2\mathrm{C}_2\mathrm{H}_4\mathrm{O}_2: 2(12.0000)+4(1.0078)+2(15.9949)=24.0000+4.0313+31.9898=60.02112(12.0000) + 4(1.0078) + 2(15.9949) = 24.0000 + 4.0313 + 31.9898 = 60.0211 (1 mark).

(b) The measured value (60.057560.0575) matches C3H8O\mathrm{C}_3\mathrm{H}_8\mathrm{O} (60.0574) much more closely than C2H4O2\mathrm{C}_2\mathrm{H}_4\mathrm{O}_2 (60.0211). The correct formula is C3H8O\mathrm{C}_3\mathrm{H}_8\mathrm{O} (1 mark).

(c) A positive iodoform test indicates a CH3CO\mathrm{CH}_3\mathrm{CO}- group. With the formula C3H8O\mathrm{C}_3\mathrm{H}_8\mathrm{O}, the compound is propan-2-ol (CH3CH(OH)CH3\mathrm{CH}_3\mathrm{CH}(\mathrm{OH})\mathrm{CH}_3). Under the iodoform test conditions, propan-2-ol is oxidised to propanone, which contains the CH3CO\mathrm{CH}_3\mathrm{CO}- group (1 mark for propan-2-ol, 1 mark for explanation).


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