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ChemistryOct 7, 2026 · Interim review
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Practice: Electron Configuration LabIsotopes, Ions and Average Atomic MassEmission Spectra LabTrends to BondsInterim QuizInterim Flashcards

Session C5: Chemistry Interim Review — Atomic Structure, Periodic Trends and Bonding

Exam weighting (from the teacher): Unit 1 Atomic Structure 60% · Unit 2 Periodic Trends 20% · Unit 3 Chemical Bonding 20%. This note gives each unit that share of the space, and follows the teacher’s topic lists in order.
Sources: NCERT Class 9 Ch. 4 (Structure of the Atom), NCERT Class 11 Ch. 2 (Structure of Atom: sub-atomic particles, atomic models, Bohr’s model, emission spectra, orbitals and electronic configuration) and Ch. 3 (Periodicity: atomic radius, ionic radius, ionization enthalpy, electronegativity). Unit 3 is the short version of Sessions C1 to C4.
Practice tools (study-tools site, Chemistry): Electron Configuration Lab (electron-config/), Isotopes, Ions and Average Atomic Mass (atom-math/), Emission Spectra Lab (spectra-lab/), Trends to Bonds (trends-to-bonds/), Chemistry Interim Quiz (chem-interim-quiz/) and Interim Flashcards (chem-interim-flashcards/).

Lesson Plan (three 45-minute sessions)

Session Minutes What to do
A. Unit 1, part 1 0–12 Topic 1: atomic models. Student retells the timeline from the picture, then one merit and one limitation of each model.
12–22 Topics 2 and 3: particles, isotopes vs ions. Fill the counting table without notes.
22–37 Topic 4: average atomic mass, including a missing-variable problem.
37–45 Topic 5: fusion, then 5 quick questions from the practice set.
B. Unit 1, part 2 0–20 Topic 6: electron configuration: full, noble gas, orbital diagrams, ground vs excited.
20–32 Topic 7: light emission: excitation, de-excitation, energy and wavelength.
32–45 Topic 8: emission spectra matching, then the Emission Spectra Lab.
C. Units 2 and 3 0–18 Unit 2: the four trends with the “three ideas” explanation.
18–38 Unit 3: bonding in the teacher’s order, at speed.
38–45 Mark Practice Exam 1 together; list the weak topics.

Unit 1 — Atomic Structure (60%)

Topic 1 — Atomic Models: Scientists, Experiments, Merits and Limitations

The five models in order
Scientist, year Experiment or evidence What it showed / the model Merit Limitation
Dalton, 1803 Mass ratios in chemical reactions (conservation of mass, definite proportions) Atoms are tiny, solid, indivisible spheres. Atoms of one element are identical; compounds form in whole-number ratios; reactions rearrange atoms. Explained the laws of conservation of mass and definite proportions. Atoms are divisible (protons, neutrons, electrons). Atoms of one element can differ in mass (isotopes). No charges.
Thomson, 1897 Cathode ray tube: the ray bent toward a positive plate, and was the same for every metal and gas All atoms contain tiny negative particles: electrons. Plum pudding model: electrons embedded in a sphere of positive charge. First model with a subatomic particle; explains why atoms are neutral. No nucleus. Could not explain the gold foil results.
Millikan, 1909 Oil drop experiment Measured the charge of one electron (−1.60 × 10⁻¹⁹ C), which also gave its mass (9.11 × 10⁻³¹ kg). Showed the electron has a fixed charge and a mass about 1/1836 of a proton’s. A measurement, not a model of the atom.
Rutherford, 1911 Gold foil (alpha scattering) experiment Nuclear model: a tiny, dense, positive nucleus with electrons around it; the atom is mostly empty space. Discovered the nucleus; explains the scattering. An orbiting electron should lose energy and spiral into the nucleus, so the atom should collapse. Does not explain line spectra or how electrons are arranged.
Bohr, 1913 Line spectrum of hydrogen Electrons move in fixed energy levels (orbits). An electron in a level does not lose energy. Light is absorbed or emitted only when an electron jumps between levels. Explains why atoms are stable and why hydrogen gives a line spectrum. Works only for one-electron atoms (hydrogen). Cannot explain the spectra of larger atoms. Electrons do not really travel in neat circular paths.
Chadwick, 1932 Bombarded beryllium with alpha particles; a neutral radiation came out Discovered the neutron: no charge, mass about equal to a proton. Explained the “missing” mass of the nucleus and why isotopes exist. —
Quantum mechanical model (Schrödinger, 1926; with de Broglie and Heisenberg) Electrons behave as waves; mathematics of the wave equation Electrons are found in orbitals: regions where there is a high probability of finding an electron (the electron cloud). Energy is still quantized (levels and sublevels s, p, d, f). Works for every atom; explains the periodic table and bonding. Gives only the probability of where an electron is, never its exact path (Heisenberg’s uncertainty principle).
The gold foil experiment

How to remember the order: Dalton’s ball → Thomson’s pudding → Rutherford’s nucleus → Bohr’s levels → the quantum cloud. Each new model was built to fix the limitation of the one before it.

Orbit vs orbital (a favorite test question). A Bohr orbit is a fixed circular path at a set distance. A quantum orbital is a 3-D region where the electron is probably found. Orbits are a simplification; orbitals are the accepted picture.


Topic 2 — Subatomic Particles

Particle Symbol Relative charge Relative mass (amu) Where Discovered by
Proton p⁺ +1 1 nucleus Rutherford (after Goldstein’s positive rays)
Neutron n⁰ 0 1 nucleus Chadwick, 1932
Electron e⁻ −1 about 1/1836 (≈ 0) electron cloud, outside the nucleus Thomson, 1897

Topic 3 — Isotopes vs Ions (Naming and Notation)

Reading a nuclear symbol
Isotopes Ions
What changes the number of neutrons the number of electrons
What stays the same protons (same element) and, for neutral atoms, electrons protons (same element) and neutrons
Effect different mass number; same chemical behavior a charge; different chemical behavior
Notation hyphen: carbon-14 · symbol: ¹⁴₆C charge at the top right: Mg²⁺, Cl⁻
Naming element name + mass number cation (+): element name + “ion” (sodium ion) · anion (−): ending changes to -ide (chloride ion, oxide ion)

Charge rule: charge = protons − electrons. Lose electrons → positive ion (cation). Gain electrons → negative ion (anion). The protons never change when an ion forms.

Counting practice

Species Protons Neutrons Electrons How
¹⁴₆C (carbon-14) 6 8 6 n = 14 − 6; neutral, so e = p
²³₁₁Na⁺ 11 12 10 1+ means one electron lost
²⁴₁₂Mg²⁺ 12 12 10 2+ means two electrons lost
³⁷₁₇Cl⁻ 17 20 18 1− means one electron gained
¹⁸₈O²⁻ 8 10 10 2− means two electrons gained
⁵⁶₂₆Fe³⁺ 26 30 23 3+ means three electrons lost

Compare two species in three questions: Same protons? (If not, different elements.) Same neutrons? (If not, isotopes.) Same electrons? (If not, one is an ion.) Carbon-12 and carbon-14 are isotopes. Na and Na⁺ are an atom and its ion. ¹⁴₆C and ¹⁴₇N have the same mass number but are different elements.

Hydrogen’s three isotopes have their own names: protium (¹H), deuterium (²H) and tritium (³H).


Topic 4 — Average Atomic Mass (and Solving for a Missing Variable)

Most elements are a mixture of isotopes. The mass on the periodic table is the weighted average of the isotope masses:

average atomic mass = (mass₁ × fraction₁) + (mass₂ × fraction₂) + …, where fraction = percent abundance ÷ 100, and the fractions add to 1.

Why “weighted”? Take 100 chlorine atoms: about 76 are chlorine-35 and 24 are chlorine-37. Total mass ≈ 76 × 35 + 24 × 37 = 3548, so the average is 3548 ÷ 100 = 35.48. Each isotope counts in proportion to how many atoms of it there are. That is all the formula does.

Quick check without a calculator: the average is always between the isotope masses and closest to the most abundant isotope.

Type A: find the average

Chlorine: Cl-35 has mass 34.969 amu (75.78%); Cl-37 has mass 36.966 amu (24.22%).

Magnesium (three isotopes): 23.985 × 0.7899 + 24.986 × 0.1000 + 25.983 × 0.1101 = 18.946 + 2.499 + 2.861 = 24.31 amu.

Type B: find the missing percent abundances

Boron has two isotopes: B-10 (10.013 amu) and B-11 (11.009 amu). Its average atomic mass is 10.811 amu. Find the percent of each.

  1. Let x = fraction of B-10. Then the fraction of B-11 is (1 − x), because the fractions add to 1.
  2. 10.013x + 11.009(1 − x) = 10.811
  3. 10.013x + 11.009 − 11.009x = 10.811
  4. −0.996x = −0.198, so x = 0.1988
  5. B-10 is 19.9% and B-11 is 80.1%. Check: the average (10.811) is closer to 11, so B-11 should be the larger share. It is.

Type C: find a missing isotope mass

Copper has two isotopes. Cu-63 has mass 62.930 amu and is 69.15% of copper. The average atomic mass is 63.546 amu. Find the mass of Cu-65.

  1. Percent of Cu-65 = 100 − 69.15 = 30.85%
  2. 62.930 × 0.6915 + m × 0.3085 = 63.546
  3. 43.516 + 0.3085m = 63.546
  4. m = 20.030 ÷ 0.3085 = 64.93 amu

Common slips: using percents instead of fractions (75.78 instead of 0.7578); using mass numbers when exact masses are given; forgetting that the two fractions are x and (1 − x), not x and x.


Topic 5 — Nuclear Fusion

Fusion: two light nuclei join to form one heavier nucleus, releasing a very large amount of energy.

Deuterium-tritium fusion

Balancing a nuclear equation. The mass numbers (top) and the atomic numbers (bottom) must each add up to the same total on both sides.

Equation Check
²₁H + ³₁H → ⁴₂He + ¹₀n top: 2 + 3 = 4 + 1 · bottom: 1 + 1 = 2 + 0
²₁H + ²₁H → ³₂He + ? top: 4 = 3 + 1 · bottom: 2 = 2 + 0, so the particle is a neutron, ¹₀n
⁴₂He + ⁴₂He → ? top 8, bottom 4: element 4 is beryllium, so ⁸₄Be
Fusion Fission
What happens small nuclei join a large nucleus splits (for example uranium-235 hit by a neutron)
Where Sun and stars; hydrogen bomb nuclear power plants; atomic bomb
Conditions extremely high temperature and pressure can run at ordinary temperatures once started (chain reaction)
Products helium; little long-lived waste radioactive waste
Both change the nucleus, form new elements, release far more energy than chemical reactions

Topic 6 — Electron Configuration

The address system

Energy level (n) Sublevels Orbitals Maximum electrons (2n²)
1 1s 1 2
2 2s, 2p 1 + 3 = 4 8
3 3s, 3p, 3d 1 + 3 + 5 = 9 18
4 4s, 4p, 4d, 4f 1 + 3 + 5 + 7 = 16 32

Every orbital holds at most 2 electrons. So an s sublevel holds 2, p holds 6, d holds 10 and f holds 14.

The three rules

  1. Aufbau principle: fill the lowest-energy sublevel first.
  2. Pauli exclusion principle: an orbital holds at most 2 electrons, and they must have opposite spins (one ↑, one ↓).
  3. Hund’s rule: within a sublevel, put one electron in each orbital first (all with the same spin), and only then start pairing.
The diagonal rule and the blocks of the periodic table

Filling order: 1s → 2s → 2p → 3s → 3p → 4s → 3d → 4p → 5s → 4d → 5p. The surprise is that 4s fills before 3d.

Shortcut: read the periodic table left to right like a book. Groups 1–2 are the s block, groups 13–18 are the p block, groups 3–12 are the d block. In period 4 you pass 4s (K, Ca), then 3d (Sc to Zn), then 4p (Ga to Kr).

Writing a neutral ground-state configuration

  1. Find the number of electrons (= atomic number for a neutral atom).
  2. Fill sublevels in order until the electrons run out.
  3. Check: the superscripts must add up to the atomic number.
Element Z Full configuration Noble gas configuration
N 7 1s² 2s² 2p³ [He] 2s² 2p³
O 8 1s² 2s² 2p⁴ [He] 2s² 2p⁴
Na 11 1s² 2s² 2p⁶ 3s¹ [Ne] 3s¹
P 15 1s² 2s² 2p⁶ 3s² 3p³ [Ne] 3s² 3p³
Cl 17 1s² 2s² 2p⁶ 3s² 3p⁵ [Ne] 3s² 3p⁵
Ca 20 1s² 2s² 2p⁶ 3s² 3p⁶ 4s² [Ar] 4s²
Fe 26 1s² 2s² 2p⁶ 3s² 3p⁶ 4s² 3d⁶ [Ar] 4s² 3d⁶
Br 35 1s² 2s² 2p⁶ 3s² 3p⁶ 4s² 3d¹⁰ 4p⁵ [Ar] 4s² 3d¹⁰ 4p⁵

Noble gas configuration: write the symbol of the previous noble gas (the one at the end of the row above) in brackets, then only the electrons after it. [He] = 2 electrons, [Ne] = 10, [Ar] = 18, [Kr] = 36.

Two exceptions to know: chromium is [Ar] 4s¹ 3d⁵ and copper is [Ar] 4s¹ 3d¹⁰. A half-filled or completely filled d sublevel is extra stable.

Reading a configuration backwards. The highest n is the period. The electrons in the highest n are the valence electrons (for main-group elements). 1s² 2s² 2p⁶ 3s² 3p⁴ has 16 electrons (sulfur), is in period 3, and has 6 valence electrons.

Orbital filling diagrams

One box per orbital, one arrow per electron. Label each sublevel.

Orbital diagrams: right, wrong and excited

Ground state vs excited state

How to decide (three steps):

  1. Check the limits. Any sublevel over its capacity (2p⁷, 1s³, 3d¹¹) is not possible.
  2. Count the electrons. The total is the atomic number, which names the element.
  3. Compare with the ground state. Same as the filling order → ground state. An electron skipped ahead → excited state.
Configuration Electrons Verdict
1s² 2s² 2p⁶ 3s¹ 11 sodium, ground state
1s² 2s² 2p⁶ 3p¹ 11 sodium, excited (3s is empty but 3p is used)
1s² 2s¹ 2p³ 6 carbon, excited (2s is not full)
1s² 2s² 2p⁵ 3s¹ 10 neon, excited
1s² 2s² 2p⁷ — not possible (2p holds 6)

Topic 7 — Light Emission: Excitation and De-excitation

Hydrogen: excitation, de-excitation and the lines it makes

The story in four steps

  1. Ground state. The electron is in its lowest energy level.
  2. Excitation. The atom absorbs energy (heat from a flame, electricity, or light). The electron jumps to a higher level. The atom is now in an excited state, which is unstable.
  3. De-excitation. The electron falls back to a lower level.
  4. Emission. As it falls, it gives out the energy as one photon of light. The photon’s energy is exactly the difference between the two levels.

Absorb energy → jump up. Fall down → emit light. Light comes out on the way down, never on the way up.

Energy, frequency and wavelength

So a bigger drop releases more energy, which means a higher frequency and a shorter wavelength (toward violet). A smaller drop gives lower energy and a longer wavelength (toward red).

Color Wavelength Frequency Photon energy
red long (about 700 nm) low low
violet short (about 400 nm) high high

Order of visible light by increasing energy: red, orange, yellow, green, blue, violet. Beyond violet is ultraviolet (more energy); below red is infrared (less energy).

Worked example (only if your class did the calculation). Hydrogen’s red line has λ = 656 nm = 6.56 × 10⁻⁷ m. f = c ÷ λ = (3.00 × 10⁸) ÷ (6.56 × 10⁻⁷) = 4.57 × 10¹⁴ Hz. E = hf = (6.626 × 10⁻³⁴)(4.57 × 10¹⁴) = 3.03 × 10⁻¹⁹ J.

Why lines and not a rainbow? Energy levels are quantized: an electron can only be in certain levels, so only certain drops are possible, so only certain colors come out.

Flame tests use this. Heating a metal salt excites its electrons, and the color seen as they fall back identifies the metal: lithium red, sodium yellow, potassium lilac, calcium orange-red, copper blue-green.


Topic 8 — Atomic Emission Spectra (Matching Lines)

The matching rule. An element is in the unknown sample only if every one of its lines appears in the unknown’s spectrum. One matching line is not enough. Lines left over belong to another element.

Which elements are in the unknown?

Worked example (the figure).

Method for the exam: take one reference element at a time, put a ruler (or the edge of your paper) on each of its lines, and tick it only if the unknown has a line in exactly the same place. All ticked → present.


Unit 2 — Periodic Trends (20%)

Every trend comes from three ideas. Learn these and you can explain any of them.

  1. Nuclear charge: more protons pull electrons in more strongly.
  2. Shielding: inner (core) electrons block some of the pull. Across a period shielding stays about the same; down a group it increases.
  3. Distance: more energy levels put the outer electrons farther from the nucleus, where the pull is weaker.

Effective nuclear charge (the pull an outer electron actually feels) ≈ protons − inner electrons. Sodium: 11 − 10 = +1. Chlorine: 17 − 10 = +7. Same period, same shielding, much stronger pull on chlorine’s outer electrons.

The trends on one picture
Property Definition Across a period → Down a group ↓
Atomic radius size of the atom (half the distance between two bonded nuclei) decreases: more protons, same shielding, electrons pulled closer increases: a new energy level each row, more shielding
First ionization energy energy needed to remove the outermost electron from a gaseous atom increases: electrons held more tightly decreases: outer electron is farther away and more shielded
Electronegativity how strongly an atom attracts shared electrons in a bond increases decreases
Ionic radius size of an ion cations shrink, then anions shrink (see below) increases

Small atom = tight hold. A small atom holds its electrons tightly, so it has a high ionization energy and a high electronegativity. A large atom holds them loosely, so both are low. Atomic radius runs opposite to the other two.

Data to see the trends (NCERT values)

Period 3 Na Mg Al Si P S Cl
Atomic radius (pm) 186 160 143 117 110 104 99
First ionization energy (kJ/mol) 496 737 577 786 1011 1000 1256
Electronegativity 0.9 1.2 1.5 1.8 2.1 2.5 3.0
Group 1 Li Na K Rb Cs
Atomic radius (pm) 152 186 231 244 262
First ionization energy (kJ/mol) 520 496 419 403 374
Electronegativity 1.0 0.9 0.8 0.8 0.7

The ionization energy does not rise perfectly smoothly (Mg to Al and P to S dip slightly). The general trend is what the exam asks for, unless your class studied the dips.

Ionic radius

Ions compared with their atoms

Ionization energy tells you the valence electrons

Removing a second or third electron always takes more energy. The huge jump comes when you start removing core electrons.

Element 1st 2nd 3rd 4th Reading
Na 496 4562 jump after 1 electron: 1 valence electron
Mg 738 1451 7733 jump after 2: 2 valence electrons
Al 578 1817 2745 11 577 jump after 3: 3 valence electrons

(kJ/mol)

How to write a trend explanation (the three-part answer)

Claim (which is larger) → cause (protons, shielding, or energy levels) → effect (pull on the outer electrons).

Link to Unit 3. The difference in electronegativity between two atoms decides the bond: large difference → ionic; medium → polar covalent; small → nonpolar covalent. Metals (low ionization energy) lose electrons and form cations; non-metals (high electronegativity) gain electrons and form anions.


Unit 3 — Chemical Bonding (20%)

The full version is Session C4. This is the exam-day summary in the teacher’s order.

1. Identifying types of bonds

Atoms Bond Electrons are ΔEN Examples
metal + metal metallic delocalized: a “sea” of electrons around + ions not used Cu, brass
metal + non-metal ionic transferred more than 1.7 NaCl, MgO
two different non-metals polar covalent shared unequally 0.5 to 1.7 H–Cl, O–H
identical or similar non-metals nonpolar covalent shared equally less than 0.5 Cl₂, C–H

Electronegativities: H 2.1 · C 2.5 · N 3.0 · O 3.5 · F 4.0 · Na 0.9 · Mg 1.2 · Al 1.5 · Si 1.8 · P 2.1 · S 2.5 · Cl 3.0 · K 0.8 · Br 2.8. Kinds of atoms come first; ΔEN refines it.

2. Drawing bonds

Ionic bonds drawn with brackets

3. Properties: weaker vs stronger

Property Ionic Metallic Covalent (molecules) Covalent network
Melting point high usually high low very high
Hardness hard but brittle malleable, ductile soft very hard
Conducts electricity only molten or dissolved yes, even as a solid no no (except graphite)
Examples NaCl, MgO Cu, Fe H₂O, CO₂, wax diamond, SiO₂

Reasons to give: ionic solids have ions fixed in a lattice (no conduction until they can move); metals have delocalized electrons; molecular substances melt low because only the weak forces between molecules are overcome, not the covalent bonds.

4. Naming

  1. Metal (or NH₄⁺) first → ionic, no prefixes. Metal with more than one charge (Fe, Cu, most transition metals): add a Roman numeral. A polyatomic ion keeps its own name. Otherwise the non-metal ends in -ide.
  2. Two non-metals → covalent, use prefixes (mono, di, tri, tetra, penta, hexa), ending in -ide. No “mono” on the first element.
Formula Name Rule used
MgCl₂ magnesium chloride ionic, -ide
Fe₂O₃ iron(III) oxide Roman numeral: 3 O²⁻ = 6−, so each Fe is 3+
Ca(NO₃)₂ calcium nitrate polyatomic ion
N₂O₄ dinitrogen tetroxide prefixes

Polyatomic ions: ammonium NH₄⁺ · hydroxide OH⁻ · nitrate NO₃⁻ · nitrite NO₂⁻ · carbonate CO₃²⁻ · sulfate SO₄²⁻ · sulfite SO₃²⁻ · phosphate PO₄³⁻.

5. Designing materials

List the properties the job needs, then choose the bond type that gives them: metallic to conduct or to be shaped (wires, pans); ionic ceramic for very high temperatures and electrical insulation (but brittle); covalent network for extreme hardness (drill tips); molecular covalent (plastics) for light, flexible insulators (wire coating, handles).

6. Molecular geometry (VSEPR)

Electron domains on the central atom = bonded atoms (a double or triple bond counts once) + lone pairs.

Domains Lone pairs Electron geometry Molecular geometry Angle Example
2 0 linear linear 180° CO₂
3 0 trigonal planar trigonal planar 120° BF₃
3 1 trigonal planar bent < 120° SO₂
4 0 tetrahedral tetrahedral 109.5° CH₄
4 1 tetrahedral trigonal pyramidal ≈ 107° NH₃
4 2 tetrahedral bent ≈ 104.5° H₂O

7. Molecular polarity

A molecule is polar if it has polar bonds and the bond dipoles do not cancel. They cancel only when the shape is symmetric and all the outer atoms are the same.

Dipoles that cancel and dipoles that add

Practice Set (answers follow)

Unit 1

  1. Which experiment led to the discovery of the nucleus, and what three observations were made?
  2. State one limitation of (a) Thomson’s model, (b) Rutherford’s model, (c) Bohr’s model.
  3. Give the number of protons, neutrons and electrons in ⁴⁰₂₀Ca²⁺ and in ¹⁵₇N³⁻.
  4. Are ³⁵₁₇Cl and ³⁷₁₇Cl isotopes or ions? What about ³⁵₁₇Cl and ³⁵₁₇Cl⁻?
  5. Silver has two isotopes: Ag-107 (106.905 amu, 51.839%) and Ag-109 (108.905 amu, 48.161%). Calculate its average atomic mass.
  6. Gallium’s two isotopes are Ga-69 (68.926 amu) and Ga-71 (70.925 amu). The average atomic mass is 69.723 amu. Find the percent abundance of each.
  7. Complete the fusion equation: ²₁H + ¹₁H → ?
  8. Write the full and the noble gas configurations of (a) sulfur, (b) potassium, (c) zinc.
  9. Draw the orbital diagram of the 2p sublevel of fluorine. How many unpaired electrons does it have?
  10. Classify as ground state, excited state or not possible, and name the element: (a) 1s² 2s² 2p⁶ 3s² 3p¹ (b) 1s² 2s² 2p⁶ 3s¹ 3p² (c) 1s² 2s³.
  11. An electron falls from n = 5 to n = 2 in one atom and from n = 3 to n = 2 in another. Which emits the photon with the shorter wavelength? Why?
  12. An unknown spectrum has lines at 405, 436, 447, 471, 492, 502, 546, 578, 588 and 668 nm. Using the reference lines in this note (mercury: 405, 436, 546, 578; helium: 447, 471, 492, 502, 588, 668; hydrogen: 410, 434, 486, 656), which elements are present?

Unit 2

  1. Arrange in order of increasing atomic radius: Cl, Na, K, S.
  2. Which has the higher first ionization energy, Mg or Ba? Explain in terms of energy levels and shielding.
  3. Arrange in order of decreasing size: Mg²⁺, O²⁻, Na⁺, F⁻. Explain.
  4. An element has successive ionization energies of 590, 1145, 4912 and 6491 kJ/mol. How many valence electrons does it have, and which group is it in?

Unit 3

  1. Classify the bond in each: KF, HBr, O₂, bronze.
  2. Name Cu₂O, PCl₅ and Na₂SO₄.
  3. For NH₃ give the electron geometry, molecular geometry, bond angle and molecular polarity.
  4. Solid sodium chloride does not conduct electricity but molten sodium chloride does. Explain.

Answers

  1. Rutherford’s gold foil (alpha scattering) experiment. Most alpha particles passed straight through; a few were deflected through small angles; very few (about 1 in 20 000) bounced back.
    1. No nucleus, so it cannot explain the gold foil results. (b) An orbiting electron should lose energy and spiral into the nucleus; it also does not explain line spectra. (c) It works only for hydrogen (one electron).
  2. Ca²⁺: 20 protons, 40 − 20 = 20 neutrons, 20 − 2 = 18 electrons. N³⁻: 7 protons, 15 − 7 = 8 neutrons, 7 + 3 = 10 electrons.
  3. ³⁵Cl and ³⁷Cl are isotopes (same protons, different neutrons). ³⁵Cl and ³⁵Cl⁻ are an atom and its ion (same protons and neutrons, different electrons).
  4. 106.905 × 0.51839 + 108.905 × 0.48161 = 55.418 + 52.450 = 107.87 amu.
  5. Let x = fraction of Ga-69. 68.926x + 70.925(1 − x) = 69.723 → 70.925 − 1.999x = 69.723 → x = 1.202 ÷ 1.999 = 0.6013. Ga-69 is 60.1%, Ga-71 is 39.9%.
  6. Top: 2 + 1 = 3. Bottom: 1 + 1 = 2. Element 2 is helium: ³₂He.
    1. S: 1s² 2s² 2p⁶ 3s² 3p⁴ = [Ne] 3s² 3p⁴. (b) K: 1s² 2s² 2p⁶ 3s² 3p⁶ 4s¹ = [Ar] 4s¹. (c) Zn: 1s² 2s² 2p⁶ 3s² 3p⁶ 4s² 3d¹⁰ = [Ar] 4s² 3d¹⁰.
  7. Fluorine is 1s² 2s² 2p⁵. The 2p boxes are [↑↓] [↑↓] [↑]. One unpaired electron.
    1. 13 electrons, aluminum, ground state. (b) 13 electrons, aluminum, excited (3s is not full but 3p is used). (c) Not possible: an s sublevel holds only 2.
  8. 5 → 2. It is the bigger drop, so the photon has more energy, a higher frequency and a shorter wavelength (434 nm, against 656 nm for 3 → 2).
  9. Mercury (405, 436, 546, 578 all present) and helium (447, 471, 492, 502, 588, 668 all present). Hydrogen is absent: none of 410, 434, 486, 656 appear. All ten lines are accounted for.
  10. Cl < S < Na < K. Across period 3 the radius decreases (Na > S > Cl); K is in period 4, below Na, so it is the largest.
  11. Mg. Barium’s outer electrons are in the 6th energy level, far from the nucleus and shielded by many inner electrons, so they are held weakly and are easier to remove.
  12. O²⁻ > F⁻ > Na⁺ > Mg²⁺. All have 10 electrons. The more protons (8, 9, 11, 12), the stronger the pull on the same electrons and the smaller the ion.
  13. The big jump is between the 2nd and 3rd, so it has 2 valence electrons: group 2 (it is calcium).
  14. KF ionic (metal + non-metal, ΔEN 3.2) · HBr polar covalent (ΔEN 0.7) · O₂ nonpolar covalent (ΔEN 0) · bronze metallic.
  15. Copper(I) oxide (O is 2−, so each of the two Cu is 1+) · phosphorus pentachloride · sodium sulfate.
  16. 4 domains (3 bonds + 1 lone pair): electron geometry tetrahedral, molecular geometry trigonal pyramidal, angle about 107°, polar (the lone pair makes it unsymmetric, so the N–H dipoles do not cancel).
  17. In the solid the ions are fixed in the lattice and cannot move. When it melts the ions are free to move and carry the charge.

The mistakes that cost the most marks

  1. Saying Rutherford discovered the electron, or that Thomson discovered the nucleus. Thomson: electron. Rutherford: nucleus. Chadwick: neutron.
  2. Subtracting the wrong way for ions: a positive charge means fewer electrons.
  3. Changing the number of protons when making an ion or an isotope. Protons never change.
  4. Using percents (75.78) instead of fractions (0.7578) in average atomic mass.
  5. Writing 3d before 4s is full, or forgetting that 3d comes before 4p.
  6. Pairing electrons in a p sublevel before each orbital has one (Hund’s rule).
  7. Using the noble gas from the same row for the noble gas configuration. It is always the one from the row above.
  8. Saying light is emitted when the electron jumps up. It is emitted when the electron falls down.
  9. Mixing up wavelength and energy: short wavelength means high energy.
  10. Calling an element present in a spectrum because one line matches. All of its lines must match.
  11. Saying atomic radius increases across a period because there are more electrons. It decreases: more protons, same shielding.
  12. Explaining a trend with “it is further right on the table”. Always give the cause: protons, shielding or energy levels.
  13. In Unit 3: prefixes on ionic names, a missing Roman numeral, a double bond counted as two domains, and “polar bonds, so polar molecule”.

Notes for next session