Comprehensive Study Guide · Chemistry

The CentralScience

From the quantum structure of atoms to the reactions that built the universe — a complete journey through the science of matter and its transformations.

12
Chapters
118
Elements
50+
Key Formulas
12
Quizzes
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Atomic Structure
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Chemical Bonding
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Thermodynamics
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Organic Chemistry
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Electrochemistry
Chapter 01 · Atomic Structure
01
Chapter 01 · Foundations

Atomic Structure

The atom is chemistry's fundamental unit. Understanding its architecture — protons, neutrons, quantum orbitals — unlocks all of chemistry.

Chemistry is called the central science because it bridges physics and biology — explaining how matter is built at the atomic level, and how atoms combine to produce everything from granite to DNA. The atom itself was once thought indivisible, but we now know it contains a dense nucleus of protons and neutrons surrounded by a quantum cloud of electrons that defines all chemical behaviour.

The modern quantum mechanical model replaced the simple "Bohr" planetary model. Electrons do not orbit in fixed paths — they inhabit probability clouds called orbitals, regions of space where there is high probability of finding an electron. The energy levels and number of electrons in each orbital determine every chemical property of an element.

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Subatomic Particles
ParticleSymbolChargeMass (amu)Location & Role
Protonp?+11.0073Nucleus — defines the element (atomic number Z)
Neutron01.0087Nucleus — defines the isotope (mass number A = Z + N)
Electrone?-10.000549Orbitals — defines bonding, reactivity, and chemistry
Electron Configuration

Electrons fill orbitals by three rules: Aufbau principle (lowest energy first), Pauli exclusion (max 2 electrons per orbital with opposite spins), and Hund's rule (half-fill degenerate orbitals before pairing).

Carbon (Z=6): 1s² 2s² 2p²
Iron (Z=26): 1s² 2s² 2p6 3s² 3p6 3d6 4s² ? abbreviated [Ar] 3d6 4s²
s orbitals (max 2e) · p orbitals (max 6e) · d orbitals (max 10e) · f orbitals (max 14e)
Valence electrons (outermost shell) determine all chemical behaviour
Key Elements — Tiles
1
H
Hydrogen
1.008
6
C
Carbon
12.011
7
N
Nitrogen
14.007
8
O
Oxygen
15.999
11
Na
Sodium
22.990
17
Cl
Chlorine
35.453
26
Fe
Iron
55.845
79
Au
Gold
196.97
Electronegativity — Pauling Scale
Higher = More Electron-Attracting Atom
Fluorine (F)
3.98
Oxygen (O)
3.44
Nitrogen (N)
3.04
Carbon (C)
2.55
Sodium (Na)
0.93
Cesium (Cs)
0.79
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The Four Quantum NumbersEach electron is uniquely described by four quantum numbers: n (principal — energy level, 1,2,3…), l (angular momentum — shape: 0=s, 1=p, 2=d, 3=f), m? (magnetic — orientation of orbital), and m? (spin: +½ or -½). No two electrons in an atom can share all four quantum numbers — the Pauli exclusion principle.
Periodic Trends
TrendAcross Period (?)Down Group (?)Reason
Atomic radiusDecreasesIncreasesMore protons pull electrons closer; more shells added going down
Ionisation energyIncreasesDecreasesMore nuclear charge holds electrons tighter; outer shells farther from nucleus
ElectronegativityIncreasesDecreasesSame reasons as ionisation energy; fluorine = most electronegative
Electron affinityGenerally increasesDecreasesTendency to gain electrons follows similar pattern to EN
Metallic characterDecreasesIncreasesNon-metals gain electrons; metals lose; bottom-left = most metallic
Knowledge Check · Ch 01
What property of an atom determines which element it is — and cannot change without creating a different element?
Select an answer above.
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02
Chapter 02 · Foundations

Chemical Bonding

Atoms bond to achieve stable electron configurations. The type of bond — ionic, covalent, metallic — determines everything about a substance's physical and chemical properties.

Atoms form chemical bonds to achieve more stable electron configurations — typically a full outer shell of 8 electrons (the octet rule). The type of bond depends on the electronegativity difference between atoms: large differences produce ionic bonds (electron transfer), small differences produce covalent bonds (electron sharing), and metals form a special electron-sea metallic bond.

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Types of Chemical Bonds
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Ionic Bond
Electron transfer: metal ? non-metal. ?EN > 1.7. Electrostatic attraction between ions. Hard, brittle, high mp, conducts when dissolved. Example: NaCl, MgO.
:: ::
Covalent Bond
Electron sharing between non-metals. ?EN < 1.7. Can be single, double, or triple. Forms molecules or network solids. Example: H2O, CO2, diamond.
~e?~
Metallic Bond
Delocalised electron "sea" around metal cation lattice. Explains malleability, ductility, electrical and thermal conductivity, and metallic lustre.
···H···
Hydrogen Bond
N–H, O–H, or F–H bonded to lone pair of N, O, or F. Responsible for water's unique properties, DNA base pairing, and protein structure.
VSEPR — Molecular Geometry
Electron PairsShapeBond AngleExamplePolar?
2 bond, 0 loneLinear180°CO2, BeCl2No (if symmetric)
3 bond, 0 loneTrigonal planar120°BF3, SO3No (if symmetric)
4 bond, 0 loneTetrahedral109.5°CH4, CCl4No (if symmetric)
3 bond, 1 loneTrigonal pyramidal107°NH3, PCl3Yes
2 bond, 2 loneBent / Angular104.5°H2O, SO2Yes
5 bond, 0 loneTrigonal bipyramidal90°/120°PCl5No
6 bond, 0 loneOctahedral90°SF6, [Co(NH3)6]³?No
Bond strength: Triple > Double > Single (energy required to break)
C–C: 347 kJ/mol · C=C: 614 kJ/mol · C=C: 839 kJ/mol
?H_rxn ˜ S(bonds broken) - S(bonds formed) [endothermic - exothermic]
Polar covalent: partial charges d+ and d- create a dipole moment µ = q × d
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Lewis Structures & Formal ChargeA Lewis structure shows all valence electrons as dots or bond lines. Formal charge = (valence electrons) - (lone pair electrons) - ½(bonding electrons). The best Lewis structure minimises formal charge and places negative formal charges on the most electronegative atoms.
Knowledge Check · Ch 02
Water (H2O) has a bent molecular geometry. What makes it a polar molecule despite both O–H bonds being identical?
Select an answer above.
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03
Chapter 03 · Foundations

Stoichiometry & Moles

The mole bridges the atomic world and the measurable world. Stoichiometry uses balanced equations to calculate precisely how much of each substance reacts or is produced.

The mole is the chemist's counting unit. One mole of any substance contains exactly 6.022 × 10²³ particles (Avogadro's number, N?). Since atoms are unimaginably tiny — a hydrogen atom weighs 1.67 × 10?²4 grams — the mole allows chemists to work with amounts that can be weighed on a balance. The molar mass of any element (in g/mol) equals its atomic mass in amu.

Stoichiometry — from the Greek for "element measure" — is the quantitative relationship between reactants and products in a chemical reaction. A balanced equation is a recipe: coefficients give molar ratios, enabling calculation of theoretical yield, limiting reagent, and percent yield.

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The Mole — Key Relationships
1 mol = 6.022 × 10²³ particles (Avogadro's number, N?)
n = m / M [n = mol · m = mass (g) · M = molar mass (g/mol)]
n = N / N? [N = number of particles]
n = V / 22.4 L [for gases at STP: 0°C, 1 atm exactly]
n = c × V [c = concentration (mol/L) · V = volume (L)]
Concentration: c = n/V ? mol/L = M (molar)
Key Balanced Equations
Combustion of Methane (Natural Gas)
CH4 + 2 O2 ? CO2 + 2 H2O
1 mol CH4 : 2 mol O2 : 1 mol CO2 : 2 mol H2O — ratios used in all stoichiometric calculations
Haber Process — Synthesis of Ammonia
N2 + 3 H2 ? 2 NH3
Feeds ~50% of world's population — uses 1–2% of global energy. Fritz Haber (Nobel 1918).
Photosynthesis
6 CO2 + 6 H2O + light ? C6H12O6 + 6 O2
Endothermic — requires ~2870 kJ per mole of glucose. Foundation of almost all life on Earth.
% Yield = (actual yield / theoretical yield) × 100
Limiting reagent: the reactant completely consumed first — sets the theoretical yield
Excess reagent: remaining after limiting reagent is exhausted
Empirical formula: simplest whole-number ratio (CH2O for glucose)
Molecular formula: actual atoms per molecule (C6H12O6 for glucose) = n × empirical, where n = M / M_empirical
Knowledge Check · Ch 03
In the reaction N2 + 3H2 ? 2NH3, if you start with 1 mol N2 and 2 mol H2, what is the limiting reagent?
Select an answer above.
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04
Chapter 04 · Matter & Energy

States of Matter & Gases

Solid, liquid, gas, plasma — the states of matter and the elegantly simple gas laws that govern the behaviour of gases under changing temperature, pressure, and volume.

Matter exists in different states depending on the balance between the kinetic energy of its particles and the intermolecular forces holding them together. In a solid, particles vibrate in fixed positions. In a liquid, particles flow past each other while remaining close. In a gas, they move rapidly and independently, filling all available space. Phase transitions occur when energy input or removal tips the balance between kinetic energy and attractive forces.

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The Gas Laws
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Boyle's Law
Constant T: P1V1 = P2V2. Pressure and volume inversely proportional. Compress gas to half volume ? pressure doubles.
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Charles's Law
Constant P: V1/T1 = V2/T2. Volume ? Temperature (ALWAYS use Kelvin!). K = °C + 273.15
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Avogadro's Law
Constant T,P: V1/n1 = V2/n2. Volume ? moles. 1 mol ideal gas = 22.4 L at STP.
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Ideal Gas Law
PV = nRT. Combines all gas laws. R = 8.314 J/(mol·K) or 0.0821 L·atm/(mol·K).
PV = nRT — The Ideal Gas Law
P = pressure (atm or Pa) · V = volume (L or m³) · n = moles · R = 8.314 J/mol·K · T = Kelvin
Van der Waals (real gases): (P + a·n²/V²)(V - nb) = nRT
a = intermolecular attraction correction · b = molecular volume correction
Dalton's Law: P_total = P1 + P2 + P3 + … (partial pressures in a gas mixture)
Phase Transitions
TransitionDirection?HExample
Melting (fusion)Solid ? LiquidEndothermic +?H_fusIce: +6.01 kJ/mol at 0°C
FreezingLiquid ? SolidExothermic -?H_fusWater: -6.01 kJ/mol at 0°C
VaporisationLiquid ? GasEndothermic +?H_vapWater: +40.7 kJ/mol at 100°C
CondensationGas ? LiquidExothermic -?H_vapSteam: -40.7 kJ/mol at 100°C
SublimationSolid ? GasEndothermicDry ice (CO2): +25.2 kJ/mol
DepositionGas ? SolidExothermicFrost formation from water vapour
Knowledge Check · Ch 04
A gas occupies 4.0 L at 300 K at constant pressure. Using Charles's Law, what volume does it occupy at 600 K?
Select an answer above.
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05
Chapter 05 · Energy

Thermodynamics

The laws of energy — enthalpy, entropy, Gibbs free energy, and why some reactions release heat and proceed spontaneously while others require constant energy input.

Thermodynamics governs the flow of energy in chemical systems. The First Law states energy is always conserved: ?U = q + w (internal energy = heat + work). The Second Law states the entropy of the universe always increases for any spontaneous process — disorder is the natural direction of change.

The decisive quantity for spontaneity is Gibbs free energy: ?G = ?H - T?S. When ?G < 0, a reaction is spontaneous. Enthalpy (?H) captures heat released or absorbed; entropy (?S) captures the change in disorder. Temperature determines which factor dominates when they conflict.

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The Laws of Thermodynamics
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Zeroth Law
If A is in thermal equilibrium with B, and B with C, then A is in equilibrium with C. Establishes temperature as a measurable property.
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First Law
?U = q + w. Energy is conserved — it can be converted between heat, work, and chemical energy, but never created or destroyed.
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Second Law
?S_universe > 0 for any spontaneous process. Entropy always increases. Why heat flows hot?cold, why gases expand, why processes are irreversible.
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Third Law
Entropy of a perfect crystal at absolute zero (0 K) is zero. Provides an absolute scale for all entropy measurements.
?G = ?H - T?S (spontaneous when ?G < 0)
?G < 0 ? Spontaneous (exergonic) · ?G > 0 ? Non-spontaneous (endergonic) · ?G = 0 ? At equilibrium
?G° = -RT ln K (relates to equilibrium constant)
?G° = -nFE° (relates to electrochemical cell potential)
Hess's Law: ?H_rxn = S ?H_f°(products) - S ?H_f°(reactants)
Standard conditions: 25°C (298 K), 1 atm, 1 mol/L concentrations
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Exothermic ? SpontaneousMany students assume exothermic reactions (?H < 0) are always spontaneous. This is wrong. Spontaneity is determined by ?G = ?H - T?S. An exothermic reaction with large negative ?S can become non-spontaneous at high temperature. An endothermic reaction with large positive ?S becomes spontaneous at high temperature. Always calculate ?G.
Knowledge Check · Ch 05
A reaction has ?H = +80 kJ/mol and ?S = +200 J/(mol·K). Under what conditions is it spontaneous?
Select an answer above.
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06
Chapter 06 · Dynamics

Chemical Kinetics

Kinetics answers: how fast? Rate laws, activation energy, and catalysts determine the speed of chemical reactions — independent of thermodynamic favourability.

A thermodynamically favourable reaction can still be effectively impossible if the activation energy barrier is enormous. Diamond is thermodynamically unstable relative to graphite (?G < 0 for diamond ? graphite), yet diamonds persist for billions of years because the kinetic barrier is insurmountable at room temperature. Kinetics and thermodynamics are independent — both must be considered.

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Rate Laws
Rate = k[A]?[B]n (determined experimentally, NOT from stoichiometry)
k = rate constant (T-dependent) · m = order w.r.t. A · n = order w.r.t. B · overall order = m + n
0th order: rate = k (constant, independent of concentration)
1st order: rate = k[A] ? half-life t½ = 0.693/k (constant, independent of [A]0)
2nd order: rate = k[A]² ? half-life t½ = 1/(k[A]0) (depends on initial concentration)
k = A · e^(-E?/RT) ln k = ln A - E?/RT
E? = activation energy (J/mol) · A = pre-exponential factor (collision frequency × steric factor)
R = 8.314 J/(mol·K) · T = temperature in Kelvin
Rule of thumb: rate roughly doubles per 10°C rise
Catalyst: lowers E? ? larger k ? faster reaction. Does NOT change ?G or equilibrium position.
Factors Affecting Reaction Rate
FactorEffect on RateMechanism
Temperature ?Increases exponentiallyMore molecules have energy = E?; Maxwell-Boltzmann distribution shifts right
Concentration ?Increases (order-dependent)More frequent collisions between reactant molecules per unit volume
Surface area ?Increases (heterogeneous)More reactant surface exposed; powders react faster than lumps
Homogeneous catalystIncreases; E? decreasesAlternative lower-energy pathway — same phase as reactants
Heterogeneous catalystIncreases; E? decreasesAdsorption weakens/orients bonds; Fe in Haber, Pt in catalytic converters
Pressure ? (gases)IncreasesEquivalent to increasing concentration; more collisions per volume
Knowledge Check · Ch 06
A catalyst speeds up a reaction. Which of the following correctly describes its mechanism?
Select an answer above.
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07
Chapter 07 · Reactions

Chemical Equilibrium

Reversible reactions reach a dynamic balance. Le Chatelier's principle and the equilibrium constant K describe how chemical systems respond to disturbance.

Most chemical reactions are reversible — products can react to regenerate reactants. At equilibrium, the forward and reverse reactions occur at equal rates, so concentrations remain constant. Equilibrium is dynamic, not static: reactions continue in both directions. The equilibrium constant K tells us where equilibrium lies — whether reactants or products are favoured.

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aA + bB ? cC + dD Kc = [C]?[D]? / [A]?[B]?
K >> 1 ? products favoured (reaction goes nearly to completion)
K << 1 ? reactants favoured (reaction barely proceeds)
K = 1 ? significant amounts of both reactants and products at equilibrium
Kp (partial pressures) · Ka (acid) · Kb (base) · Ksp (solubility product) · Kw = 1×10?¹4 (water)
?G° = -RT ln K ?? large K means large negative ?G° (thermodynamically driven)
Le Chatelier's Principle

When a system at equilibrium is disturbed, it shifts to oppose the change and reach a new equilibrium.

Stress AppliedDirection of ShiftEffect on K
Increase [reactant]Forward ? (toward products)K unchanged
Increase [product]Reverse ? (toward reactants)K unchanged
Increase pressure (gas)Toward fewer moles of gasK unchanged
Increase temperatureEndothermic directionK changes (? for endothermic rxn)
Decrease temperatureExothermic directionK changes (? for exothermic rxn)
Add catalystNo shift — equilibrium reached fasterK unchanged
Remove productForward ? (drives reaction)K unchanged
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Haber Process — OptimisationN2 + 3H2 ? 2NH3 (?H = -92 kJ/mol). Le Chatelier predicts: high pressure and low temperature favour NH3. But low temperature slows the rate (kinetics). Industrial compromise: 400–500°C, 150–300 atm, iron catalyst — a classic thermodynamics vs. kinetics trade-off that produces ammonia for fertilisers feeding half of humanity.
Knowledge Check · Ch 07
For 2SO2(g) + O2(g) ? 2SO3(g), increasing total pressure will:
Select an answer above.
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08
Chapter 08 · Reactions

Acids, Bases & pH

Proton donors and acceptors — acid-base chemistry governs biological systems, industrial processes, and everything from blood pH to ocean acidification.

The Brønsted-Lowry definition is most useful: an acid is a proton (H?) donor; a base is a proton acceptor. Every acid-base reaction involves conjugate pairs — the acid loses a proton to become its conjugate base; the base gains a proton to become its conjugate acid. Acid strength is quantified by Ka: the larger the Ka (smaller the pKa), the stronger the acid.

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pH = -log[H3O?] pOH = -log[OH?] pH + pOH = 14 at 25°C
Kw = [H?][OH?] = 1.0 × 10?¹4 at 25°C (autoionisation of water)
Strong acid (HCl, HNO3, H2SO4): fully dissociate ? [H?] = initial acid concentration
Weak acid: use ICE table and Ka expression; pH = ½(pKa - log c) (approximation)
Henderson-Hasselbalch: pH = pKa + log([A?]/[HA]) ? buffer equation
Common Acids & Bases
SubstanceTypeKa / KbpKaKey Application
HClStrong acid~107-7Stomach acid, metal cleaning, pickling
H2SO4Strong diprotic acid>>1 (1st), 0.012 (2nd)-, 1.92Car batteries, fertiliser (H3PO4) production
CH3COOHWeak acid1.8×10?54.74Vinegar; acetate buffer in biochemistry
H2CO3Weak diprotic acid4.3×10?7 (1st)6.37Blood buffering (CO2/HCO3? system)
NaOHStrong baseSaponification, drain cleaner
NH3Weak baseKb = 1.8×10?5pKb = 4.74Household cleaner, fertiliser precursor
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Blood Buffer SystemBlood pH must stay within 7.35–7.45 — a deviation of just ±0.4 units is fatal. The bicarbonate buffer: CO2 + H2O ? H2CO3 ? H? + HCO3?. Lungs regulate CO2 (acidosis ? breathe faster); kidneys regulate HCO3? (long-term). This elegant equilibrium system is one of the most critical acid-base applications in biology.
Knowledge Check · Ch 08
What is the pH of a 0.01 M solution of HCl (a strong acid that fully dissociates in water)?
Select an answer above.
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Chapter 09 · Advanced

Electrochemistry

Oxidation and reduction — electron transfer drives galvanic cells, electrolysis, corrosion, and every battery from AA cells to lithium-ion packs.

Electrochemistry connects chemistry with electricity through oxidation-reduction (redox) reactions — reactions involving electron transfer. The mnemonic OIL RIG — Oxidation Is Loss, Reduction Is Gain (of electrons) — is essential. In a galvanic (voltaic) cell, a spontaneous redox reaction generates electricity. In an electrolytic cell, electricity drives a non-spontaneous reaction.

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E°_cell = E°_cathode - E°_anode ?G° = -nFE°
n = moles electrons transferred · F = Faraday's constant = 96,485 C/mol
E°_cell > 0 ? ?G° < 0 ? spontaneous galvanic cell
Nernst equation: E = E° - (0.0592/n) log Q [at 25°C]
Galvanic cell: anode (oxidation, -) ? salt bridge ? cathode (reduction, +)
Electrolysis: same setup but driven by external power supply — non-spontaneous reaction forced to occur
Standard Reduction Potentials (E°)
Half-reactionE° (V)Tendency
F2 + 2e? ? 2F?+2.87Strongest oxidising agent
MnO4? + 8H? + 5e? ? Mn²? + 4H2O+1.51Potassium permanganate oxidiser
Cl2 + 2e? ? 2Cl?+1.36Disinfectant, water treatment
O2 + 4H? + 4e? ? 2H2O+1.23Fuel cell cathode reaction
Cu²? + 2e? ? Cu+0.34Copper plating; above H2 in series
2H? + 2e? ? H20.00Reference electrode (SHE)
Zn²? + 2e? ? Zn-0.76Anode in Zn-Cu (Daniell) cell
Li? + e? ? Li-3.04Strongest reducing agent; lithium batteries
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The Daniell CellThe classic Zn-Cu galvanic cell: Zn anode (Zn ? Zn²? + 2e?, oxidation) connected via a salt bridge to a Cu cathode (Cu²? + 2e? ? Cu, reduction). E°_cell = +0.34 - (-0.76) = +1.10 V. This positive cell potential confirms the reaction is spontaneous — electrons flow spontaneously from zinc to copper through the external circuit.
Knowledge Check · Ch 09
In a galvanic cell, electrons flow spontaneously from the anode to the cathode through the external circuit. What occurs at the anode?
Select an answer above.
```
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10
Chapter 10 · Advanced

Organic Chemistry

Carbon's unique ability to form four bonds and create chains, rings, and polymers makes organic chemistry the chemistry of life — and of petroleum, plastics, drugs, and materials.

Organic chemistry is the chemistry of carbon compounds. Carbon is unique: it forms 4 covalent bonds, bonds strongly to itself (C–C, C=C, C=C), and creates chains, branches, and rings of virtually unlimited complexity. Over 10 million organic compounds are known — more than all other chemical compounds combined. They include fuels, plastics, drugs, DNA, proteins, and all biochemical molecules.

The key to organic chemistry is functional groups — specific arrangements of atoms that give characteristic chemical properties regardless of the rest of the molecule. Knowing a functional group's properties tells you almost everything about how a molecule will react.

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Major Functional Groups
GroupStructureClassExampleKey Property
Hydroxyl –OHR–OHAlcoholEthanol (C2H5OH)H-bonding; polar; soluble in water
Carbonyl C=OR–CHOAldehydeFormaldehyde (HCHO)Reactive; oxidised to carboxylic acid
Carbonyl C=OR–CO–R'KetoneAcetone (CH3COCH3)Solvent; nucleophilic addition reactions
Carboxyl –COOHR–COOHCarboxylic acidAcetic acid (CH3COOH)Weak acid; forms esters and amides
Amine –NH2R–NH2AmineMethylamine (CH3NH2)Weak base; nucleophile; fishy odour
Ester –COO–R–COO–R'EsterEthyl acetate (CH3COOC2H5)Fragrant; solvent; in fats and oils
Amide –CONH–R–CONH–R'AmidePeptide bond in proteinsStable; planar; basis of protein structure
Halide –XR–X (F,Cl,Br,I)HaloalkaneChloroform (CHCl3)SN1/SN2 reactions; polar C–X bond
Key Organic Reactions
Esterification (Fischer Esterification)
R–COOH + R'–OH ? R–COO–R' + H2O (H? catalyst)
Reversible — remove water to drive forward. Esters have fruity aromas. Reverse = saponification (base + ester ? soap + alcohol).
SN2 Nucleophilic Substitution
Nu:? + R–X ? Nu–R + X? (backside attack; inversion of configuration)
Bimolecular; concerted; favoured with primary substrates and strong nucleophiles; rate = k[Nu][R–X]
Aldol Condensation
2 CH3CHO ? CH3CH(OH)CH2CHO (base or acid catalyst)
Forms C–C bond; fundamental in biosynthesis and industrial chemistry; self-condensation of aldehydes/ketones.
Isomerism
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Structural Isomers
Same molecular formula, different connectivity. Example: butane (n-C4H10) and isobutane (2-methylpropane). Different physical and chemical properties.
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Stereoisomers
Same formula and connectivity, different spatial arrangement. Geometric (cis/trans around C=C) or optical (non-superimposable mirror images — enantiomers).
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Enantiomers
Chiral molecules (4 different groups on carbon) exist as non-superimposable mirror images. Designated R/S. Often dramatically different biological activity.
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Conformational
Different spatial arrangements from rotation about C–C single bonds (eclipsed vs staggered). Not isolable at room temperature — interconvert rapidly.
Knowledge Check · Ch 10
Which functional group is responsible for the acidic properties of carboxylic acids like acetic acid (vinegar)?
Select an answer above.
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Chapter 11 · Advanced

Nuclear Chemistry

Reactions in the nucleus — radioactive decay, fission, fusion, and the extraordinary energies locked inside matter itself, described by E = mc².

Nuclear chemistry involves changes in the nucleus rather than the electron shell. These reactions involve energies millions of times greater than chemical reactions — and can transform one element into another (transmutation). Radioactivity was discovered by Henri Becquerel in 1896 and studied by Marie Curie, who coined the term and discovered polonium and radium — becoming the first person to win two Nobel prizes in different sciences.

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Types of Radioactive Decay
TypeSymbolCompositionMass ChangePenetrating Power
Alpha decaya (42He)2 protons + 2 neutrons; helium-4 nucleus-4 mass, -2 protonLow — stopped by paper
Beta-minus decayß? (e?)Neutron ? proton + electron + antineutrinoNo mass change, +1 protonMedium — stopped by aluminium
Beta-plus (positron)ß? (e?)Proton ? neutron + positron + neutrinoNo mass change, -1 protonMedium; annihilates with e? ? ?
Gamma decay? (photon)High-energy electromagnetic radiationNo mass or charge changeHigh — needs lead or concrete shielding
Electron captureECProton + e? ? neutron + neutrinoNo mass, -1 protonX-rays emitted
E = mc² ?E = ?m × c² (mass-energy equivalence)
1 amu mass defect = 931.5 MeV of energy
Half-life: N(t) = N0 × (½)^(t/t½) or N = N0 × e^(-?t) where ? = 0.693/t½
Fission: ²³5U + n ? ?²Kr + ¹4¹Ba + 3n + ~200 MeV (chain reaction in reactors/bombs)
Fusion: ²H + ³H ? 4He + n + 17.6 MeV (powers the sun; tokamak reactors)
A Brief History of Nuclear Science
1896
Radioactivity Discovered
Henri Becquerel discovers uranium emits penetrating radiation spontaneously — not requiring sunlight as previously believed.
1898
Marie Curie — Polonium & Radium
Coins the term "radioactivity." Discovers two new elements. First Nobel 1903 (Physics); second Nobel 1911 (Chemistry). Pioneer in a male-dominated field.
1905
E = mc²
Einstein's special relativity shows mass and energy are equivalent — explaining the enormous energies released in nuclear reactions.
1938
Nuclear Fission Discovered
Otto Hahn, Lise Meitner, and Fritz Strassmann discover that uranium splits into lighter elements when struck by a neutron, releasing enormous energy.
1942
First Self-Sustaining Chain Reaction
Enrico Fermi leads the first controlled nuclear chain reaction at Chicago Pile-1, demonstrating the feasibility of nuclear power.
1951 ?
Nuclear Power
First electricity from nuclear fission (EBR-1, Idaho). Today nuclear provides ~10% of global electricity with zero carbon emissions during operation.
Knowledge Check · Ch 11
Carbon-14 has a half-life of 5,730 years. If a sample begins with 1,000 atoms, approximately how many C-14 atoms remain after 17,190 years?
Select an answer above.
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Chapter 12 · Applications

Chemistry & Our World

From climate change to drug design, from green chemistry to materials science — how the principles of chemistry shape the most pressing challenges of the 21st century.

Chemistry is not confined to the laboratory. Every product of modern civilisation — medicines, materials, fuels, food, fertilisers, electronics — exists because of chemistry. And every major challenge facing humanity — climate change, antibiotic resistance, renewable energy, clean water — requires chemistry for its solution. The 12 Principles of Green Chemistry, formulated by Paul Anastas and John Warner in 1998, guide chemists to design processes that reduce hazardous substances, minimise waste, and use renewable resources.

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Chemistry in Key Domains
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Green Chemistry
Design chemical products and processes that reduce or eliminate the use of hazardous substances. Atom economy = (desired product mass / total reactant mass) × 100. Higher = better.
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Medicinal Chemistry
Drug design — molecule must have right shape, polarity, and binding affinity. Chirality is critical: one enantiomer of thalidomide treats morning sickness; the other causes birth defects.
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Energy Chemistry
Lithium-ion batteries (intercalation of Li?), hydrogen fuel cells (H2 oxidation, O2 reduction), solar cells (photovoltaic semiconductor chemistry), and nuclear fission/fusion.
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Materials Chemistry
Graphene (single-layer carbon; 200× stronger than steel), carbon nanotubes, semiconductors, superconductors, biomaterials, and conducting polymers for flexible electronics.
Climate Change & Atmospheric Chemistry
GasFormulaGWP (100yr)SourceAtmospheric Lifetime
Carbon dioxideCO21 (reference)Combustion, deforestationCenturies–millennia
MethaneCH486Agriculture, natural gas, landfills~12 years
Nitrous oxideN2O298Fertilisers, combustion~120 years
Ozone (stratosphere)O3ProtectiveO2 + UV ? O + O2; O + O2 ? O3Hours–days in troposphere
CFC-12CCl2F210,900Old refrigerants (banned)~100 years; destroys ozone
SF6SF623,500Electrical equipment~3,200 years
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The Haber Process LegacyThe Haber-Bosch process synthesises ammonia from N2 and H2. It produces nitrogen fertilisers that feed approximately 4 billion people who could not otherwise be sustained by organic farming alone. It is arguably the most important chemical process in human history — but also uses ~1–2% of global energy and releases significant CO2. Developing a green alternative using renewable electricity and electrochemical nitrogen fixation is one of chemistry's great current challenges.
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Study Complete — The Central ScienceYou have explored all 12 chapters of this chemistry study guide — from quantum atomic structure to the pressing chemistry of climate change. Chemistry is the bridge between the molecular world and the world we experience. Every material object, every living thing, every energy source, and every medicine exists because of chemical principles. Return to any chapter via the sidebar to review.
Final Check · Ch 12
Green Chemistry's "atom economy" measures what?
Select an answer above.
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