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This is the Ultimate A-Level Edexcel Chemistry Cheat Sheet Pack designed to help you tackle the most challenging chemistry concepts with confidence. These condensed notes cover all the essential Year 12 topics you'll encounter in your studies.

The pack is structured to give you quick access to key information when you're revising or need a refresher before exams. Each section focuses on the core concepts that examiners love to test, presented in a clear and digestible format.

Tip: Use this pack alongside your textbook and past papers for maximum effectiveness - these notes are your quick reference guide when time is short!

Platform Overview

This page shows the SnapRevise platform interface, which offers comprehensive chemistry support through multiple learning tools. You can see various features including bite-size videos, smart quizzes, and mini revision guides.

The platform tracks your progress (showing 45% completion here) and provides personalised learning paths based on your performance. The heart structure topic is highlighted, showing how biological concepts connect to chemistry.

The interface demonstrates how modern learning platforms can supplement traditional revision methods. Notice the 24/7 tutor support and predicted exam packs - these tools can help identify your weak spots and focus your revision efforts more effectively.

Remember: Digital platforms are great for practice, but don't forget to work through problems by hand as you would in an actual exam!

Atomic Structure, Mass & Electronic Configuration

Atoms are the building blocks of everything around you, made up of protons, neutrons, and electrons. The nucleus contains protons $+1 charge$ and neutrons (no charge), whilst electrons $-1 charge$ orbit in shells around it.

The atomic model has evolved dramatically over time. Dalton thought atoms were indivisible balls, Thomson proposed the "plum pudding" model with electrons in a positive "sea", and Rutherford discovered the dense nucleus. Bohr then suggested electrons orbit in fixed paths, leading to our current quantum model.

Mass spectrometry is your go-to technique for finding atomic masses and isotope abundances. The process involves ionisation, acceleration, ion drift, and detection. You'll use the formula: Ar = Σ(relative isotopic mass × abundance)/100 to calculate relative atomic mass from mass spectra.

Electronic configuration follows strict rules - electrons fill the lowest energy orbitals first (Aufbau principle), and orbitals of the same energy fill singly before pairing. Remember that 4s fills before 3d, which catches many students out!

Exam Tip: Mass spectrometry questions often ask you to calculate relative atomic mass - practice using the abundance data from mass spectra!

Ionisation Energy & Basic Equations

Ionisation energy measures how much energy you need to remove an electron from an atom. First ionisation energy removes one electron, whilst successive ionisation energies remove additional electrons - and they get progressively harder!

Three key factors affect ionisation energy: atomic radius $bigger atoms = easier to remove electrons$, nuclear charge $more protons = harder to remove$, and shielding $more inner electrons = easier to remove outer ones$. These patterns explain why ionisation energy increases across periods and decreases down groups.

The mole is chemistry's counting unit - it's 6.022 × 10²³ particles of anything. You'll constantly use n = m/M to convert between moles and mass, and c = n/V for concentrations. Master these equations early!

Gas calculations use the molar gas volume (24 dm³ at standard conditions) or the ideal gas equation PV = nRT. Remember to convert units carefully - pressure in Pa, volume in m³, and temperature in Kelvin.

Empirical and molecular formulas come from composition data. Find moles of each element, divide by the smallest, and you've got your empirical formula. The molecular formula is just whole-number multiples of this.

Practice Tip: Set up a conversion table for units - it'll save you marks when you're rushing in exams!

Chemical Bonding

Ionic bonding occurs when metals lose electrons and non-metals gain them, creating charged ions that attract electrostatically. The strength depends on charge $higher charges = stronger bonds$ and size $smaller ions = stronger bonds due to closer packing$.

Covalent bonding happens when non-metals share electrons to get full outer shells. You can have single, double, or triple bonds depending on how many pairs are shared. Coordinate bonds are special - one atom donates both electrons in the pair.

Molecular shapes are determined by electron pair repulsion. Bonding pairs and lone pairs repel each other, but lone pairs repel more strongly, reducing bond angles by about 2.5° each. Learn the common shapes: linear (180°), trigonal planar (120°), tetrahedral (109.5°).

Metallic bonding creates a "sea" of delocalised electrons around positive metal ions. This explains why metals conduct electricity, are malleable, and have high melting points. Stronger metallic bonding occurs with smaller, more highly charged metal ions.

Different crystal structures have characteristic properties - ionic compounds conduct when molten, metals conduct in all states, and molecular substances like ice have low melting points.

Memory Aid: "Lone pairs are bullies" - they push bonding pairs around more than other bonding pairs do!

Enthalpies, Calorimetry & Hess's Law

Enthalpy changes measure heat energy transfers at constant pressure. Exothermic reactions release energy (ΔH negative), warming the surroundings, whilst endothermic reactions absorb energy (ΔH positive), cooling things down.

Calorimetry experiments let you measure enthalpy changes directly using q = mcΔT. Coffee cup calorimeters work well for neutralisation reactions, whilst spirit burner setups measure combustion enthalpies. Always account for heat losses and incomplete reactions in your error analysis.

Hess's Law states that enthalpy change is independent of route - incredibly useful when you can't measure something directly! You can use combustion data $ΔH = Σ combustion of reactants - Σ combustion of products$ or formation data $ΔH = Σ formation of products - Σ formation of reactants$.

Bond enthalpies give approximate enthalpy changes using ΔH = Σ bonds broken - Σ bonds made. Remember that bond breaking is endothermic (energy in) and bond making is exothermic (energy out).

The activation energy is the minimum energy needed for reaction - it's the same whether a reaction is exothermic or endothermic, just measured from different starting points.

Calculation Tip: Always check your signs - formation enthalpies are usually negative, and combustion enthalpies are always negative!

Collision Theory & Chemical Equilibrium

Collision theory explains reaction rates simply - particles must collide with enough energy (above activation energy) and in the correct orientation. Not every collision leads to reaction, which is why most reactions aren't instantaneous!

The Maxwell-Boltzmann distribution shows how molecular energies are spread in a gas. Higher temperatures shift the curve right, meaning more molecules have sufficient energy to react. Catalysts provide alternative pathways with lower activation energy.

Factors affecting reaction rate include temperature $more energy = more successful collisions$, concentration/pressure $more particles = more collisions$, surface area $more contact = more collisions$, and catalysts (lower activation energy).

Chemical equilibrium occurs in closed systems when forward and backward reaction rates are equal, keeping concentrations constant. It's dynamic - reactions continue, but there's no net change.

Le Chatelier's principle predicts equilibrium shifts: the system opposes changes. Increase temperature and equilibrium shifts to absorb heat (endothermic direction). Change concentration and equilibrium shifts to oppose the change. Increase pressure and equilibrium favours fewer gas molecules.

Common Mistake: Catalysts speed up reaching equilibrium but don't change the equilibrium position itself!

Industrial Processes & Advanced Concepts

The Haber Process demonstrates real-world compromise conditions. Theoretically, high pressure and low temperature maximise ammonia yield, but practically, 400-500°C and 200 atm balance yield with cost and safety. Iron catalyst speeds up the reaction without affecting equilibrium position.

Equilibrium constants (Kc) show where equilibrium lies. Kc > 1 means products are favoured, Kc < 1 means reactants dominate. Temperature changes Kc values, but pressure, concentration, and catalysts don't affect it.

Redox reactions involve electron transfer - oxidation loses electrons (increase in oxidation number), reduction gains electrons (decrease in oxidation number). Balance redox equations by combining half-equations after balancing electrons.

Oxidation numbers help track electron transfer. Use the rules: uncombined elements = 0, simple ions = their charge, oxygen usually -2, hydrogen usually +1. The sum of oxidation numbers equals the overall charge.

Lattice enthalpy measures ionic bond strength but can't be measured directly. It depends on ion charge $higher charges = stronger lattice$ and ion size $smaller ions = stronger lattice due to closer packing$.

Industrial Reality: Perfect conditions often aren't economically viable - compromise is key in chemical manufacturing!

Born-Haber Cycles & Thermodynamics

Born-Haber cycles use Hess's Law to calculate lattice enthalpies indirectly. You'll work with atomisation, ionisation, electron affinity, and formation enthalpies. Group 2 compounds need extra steps - second ionisation energies and doubled electron affinities.

Dissolving ionic compounds involves two competing processes: breaking the lattice (endothermic) and hydrating the ions (exothermic). The overall enthalpy of solution depends on which process dominates.

Entropy measures disorder - gases have higher entropy than liquids, which have higher entropy than solids. Reactions producing more gas molecules typically increase entropy. Calculate entropy changes using ΔS = Σ products - Σ reactants.

Gibbs Free Energy determines reaction feasibility using ΔG = ΔH - TΔS. Reactions are feasible when ΔG ≤ 0. Temperature can make unfeasible reactions become feasible by changing the TΔS term.

The relationship between enthalpy, entropy, and temperature determines whether reactions occur spontaneously. Some reactions are feasible at all temperatures, others only above or below specific temperatures.

Key Insight: Thermodynamics tells you if a reaction can happen, but kinetics determines if it actually will - high activation energy can prevent feasible reactions!

Rate Equations & Reaction Mechanisms

Rate equations show how concentration affects reaction rate, but they can't be predicted from chemical equations - you must determine them experimentally. The general form is Rate = k$A$^m$B$^n, where m and n are the orders of reaction.

Reaction orders tell you the concentration effect: zero order means concentration doesn't affect rate, first order means doubling concentration doubles rate, second order means doubling concentration quadruples rate. The sum of all orders gives the overall reaction order.

Rate constants (k) have units that depend on the overall reaction order. Temperature increases rate constants exponentially, following the Arrhenius equation: k = Ae^$-Ea/RT$. Plot ln k against 1/T to find activation energy from the gradient.

Clock reactions measure initial rates by timing how long specific changes take. You assume concentration doesn't change significantly during the measured time period, making Rate ∝ 1/time.

Rate-concentration graphs show reaction orders clearly: zero order gives horizontal lines, first order gives straight lines through origin, second order gives curves. Concentration-time graphs have characteristic shapes for each order.

The rate-determining step is the slowest step in multi-step reactions - it controls the overall rate. The orders in the rate equation tell you how many molecules participate in this crucial step.

Practical Tip: Clock reactions are great for coursework - choose easily observable endpoints like colour changes or precipitate formation!