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    Topic 1: Atomic Structure and the Periodic Table — Edexcel A-Level Chemistry

    Test yourself on Topic 1: Atomic Structure and the Periodic Table with PEARSON EDEXCEL A-Level practice questions.

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    Topic 1: Atomic Structure and the Periodic Table explained

    This topic introduces the concept of oxidation numbers as a systematic method for classifying redox reactions, including disproportionation.

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    Students learn to define oxidation and reduction in terms of electron transfer and changes in oxidation number, and apply these principles to write and balance ionic half-equations.

    Read the Topic 1: Atomic Structure and the Periodic Table study guideFull revision notes for Edexcel A-Level Chemistry

    What to demonstrate

    1. Correct calculation of oxidation numbers in compounds and ions, including peroxides and metal hydrides.
    2. Correct identification of oxidation and reduction based on electron transfer and oxidation number changes.
    3. Correct identification of oxidising and reducing agents.
    Show all 6 objectives
    1. Correct identification of disproportionation reactions.
    2. Correct use of Roman numerals to indicate oxidation numbers.
    3. Correct construction of full ionic equations from ionic half-equations.

    Topic 1: Atomic Structure and the Periodic Table exam tips

    Topic Overview

    Topic 1: Atomic Structure and the Periodic Table is the foundation of A-Level Chemistry. It explores the internal structure of atoms, including protons, neutrons, and electrons, and how this structure dictates the arrangement of elements in the Periodic Table. You'll delve into the evolution of atomic models from Dalton to the quantum mechanical model, and understand key principles like electron configuration, ionisation energy, and periodicity. This topic is crucial because it explains why elements behave the way they do, linking atomic properties to chemical reactions and bonding.

    Mastering this topic is essential for success in later modules, such as bonding, kinetics, and organic chemistry. It provides the language and concepts needed to describe elements and their trends. For example, understanding electron shielding and nuclear charge helps explain why reactivity increases down Group 1 but decreases across Period 3. You'll also learn to interpret mass spectra and calculate relative atomic mass, skills that are directly assessed in exams. By the end, you should be able to predict properties of unfamiliar elements based on their position in the Periodic Table.

    This topic also introduces practical skills like using mass spectrometry data and plotting ionisation energy graphs. It connects to real-world applications, such as understanding why noble gases are inert (used in lighting) or why alkali metals are highly reactive (used in batteries). A solid grasp of atomic structure is not just about passing exams—it's about seeing the invisible building blocks that make up everything around us.

    Key Concepts
    • →Electron configuration: Understand how electrons fill orbitals (1s, 2s, 2p, etc.) following the Aufbau principle, Hund's rule, and Pauli exclusion principle. Be able to write configurations for atoms and ions, including exceptions like chromium and copper.
    • →Ionisation energy: Define first and successive ionisation energies, and explain trends across periods and down groups in terms of nuclear charge, atomic radius, and electron shielding. Interpret graphs of successive ionisation energies to deduce electronic structure.
    • →Periodicity: Recognise trends in atomic radius, first ionisation energy, and melting points across Period 3. Explain these trends using concepts of nuclear attraction, shielding, and metallic/bonding structures.
    • →Relative atomic mass and mass spectrometry: Calculate relative atomic mass from isotopic abundances. Interpret mass spectra to identify isotopes and determine relative atomic mass. Understand how mass spectrometry works (ionisation, acceleration, deflection, detection).
    • →Atomic models: Describe the evolution from Dalton's solid sphere to Thomson's plum pudding, Rutherford's nuclear model, Bohr's planetary model, and the modern quantum mechanical model (orbitals and probability clouds).
    Marking Points
    • Correct calculation of oxidation numbers in compounds and ions, including peroxides and metal hydrides.
    • Correct identification of oxidation and reduction based on electron transfer and oxidation number changes.
    • Correct identification of oxidising and reducing agents.
    • Correct identification of disproportionation reactions.
    • Correct use of Roman numerals to indicate oxidation numbers.
    • Correct construction of full ionic equations from ionic half-equations.
    Examiner Tips
    • 💡Always check that the sum of oxidation numbers in a neutral compound equals zero and in an ion equals the charge of the ion.
    • 💡Remember that oxidising agents are reduced (gain electrons) and reducing agents are oxidised (lose electrons).
    • 💡When balancing half-equations, ensure the total charge on both sides is equal.
    • 💡Practice identifying oxidation numbers in various contexts, especially for s- and p-block elements.
    • 💡When answering questions on ionisation energy trends, always mention three factors: nuclear charge, atomic radius, and electron shielding. Explain how each factor changes and whether it increases or decreases the ionisation energy. Use specific examples from Period 3 (e.g., Na to Ar).
    • 💡For mass spectrometry questions, be precise with the order of steps: ionisation (electron impact or electrospray), acceleration, deflection (by magnetic field), and detection. Remember that the mass-to-charge ratio (m/z) is measured, and for singly charged ions, m/z equals the mass number.
    • 💡When writing electron configurations, always use the correct order of orbital filling (1s, 2s, 2p, 3s, 3p, 4s, 3d, 4p...). For transition metals, remember that the 4s orbital is filled before 3d, but when forming ions, electrons are removed from the 4s orbital first. This is a common exam trap.
    Common Mistakes
    • Confusing the direction of electron transfer in oxidation and reduction.
    • Incorrectly assigning oxidation numbers in complex ions or species.
    • Failing to balance both atoms and charges when constructing ionic half-equations.
    • Misidentifying the species being oxidised or reduced in a disproportionation reaction.
    • Misconception: Electrons orbit the nucleus in fixed circular paths like planets. Correction: In the quantum mechanical model, electrons exist in orbitals—regions of high probability—not fixed orbits. The exact position cannot be known simultaneously with momentum (Heisenberg uncertainty principle).
    • Misconception: Ionisation energy always increases across a period. Correction: While generally true, there are drops between Group 2 and 3 (e.g., Mg to Al) due to a change from s to p subshell, and between Group 5 and 6 (e.g., P to S) due to electron pairing in the p orbital causing repulsion.
    • Misconception: The mass number is the same as relative atomic mass. Correction: Mass number is the total number of protons and neutrons in a specific isotope, while relative atomic mass is the weighted mean mass of all isotopes relative to 1/12th of carbon-12. They are often different (e.g., chlorine has mass number 35 or 37, but Ar = 35.5).
    Frequently Asked Questions
    Why does ionisation energy decrease down a group?
    Ionisation energy decreases down a group because the atomic radius increases, meaning the outermost electron is further from the nucleus. Additionally, there is more electron shielding from inner shells, which reduces the effective nuclear charge felt by the outer electron. These factors outweigh the increase in nuclear charge, making it easier to remove an electron. For example, the first ionisation energy of caesium is lower than that of lithium.
    How do I calculate relative atomic mass from mass spectrum data?
    To calculate relative atomic mass (Ar) from a mass spectrum, multiply the mass number of each isotope by its relative abundance (as a decimal or percentage), sum these products, and divide by the total abundance (usually 100 if using percentages). For example, chlorine has two isotopes: 35Cl (75%) and 37Cl (25%). Ar = (35 × 75 + 37 × 25) / 100 = (2625 + 925) / 100 = 3550 / 100 = 35.5. Always check that your answer is reasonable—chlorine's Ar is about 35.5.
    What is the difference between an orbital and a shell?
    A shell is a principal energy level (n=1,2,3...) that contains subshells (s, p, d, f). An orbital is a region within a subshell where there is a high probability of finding an electron. Each orbital can hold a maximum of two electrons with opposite spins. For example, the second shell (n=2) has two subshells: 2s (one orbital) and 2p (three orbitals), so a total of four orbitals and eight electrons. Orbitals have specific shapes (s is spherical, p is dumbbell-shaped) and orientations.
    Why is chromium's electron configuration [Ar] 4s1 3d5 instead of [Ar] 4s2 3d4?
    Chromium is an exception because a half-filled d subshell (3d5) is more stable than a partially filled one (3d4) due to exchange energy and reduced electron-electron repulsion. The energy difference between the 4s and 3d orbitals is small, so promoting one electron from the 4s to the 3d orbital results in a lower overall energy configuration. Similarly, copper has [Ar] 4s1 3d10 for a fully filled d subshell. You should memorise these exceptions for exams.
    How do I explain the trend in melting points across Period 3?
    Melting points across Period 3 depend on the type of bonding and structure. Sodium, magnesium, and aluminium are metals with metallic bonding; melting points increase from Na to Al because the number of delocalised electrons per atom increases (Na:1, Mg:2, Al:3), strengthening the metallic bond. Silicon is a giant covalent structure (diamond-like) with very strong covalent bonds, giving it a very high melting point. Phosphorus (P4), sulfur (S8), chlorine (Cl2), and argon (Ar) are simple molecular substances with weak van der Waals forces between molecules, so they have low melting points. Sulfur has a higher melting point than phosphorus because S8 molecules are larger and have stronger van der Waals forces.
    What is the difference between first and second ionisation energy?
    First ionisation energy is the energy required to remove one mole of electrons from one mole of gaseous atoms to form one mole of gaseous +1 ions. Second ionisation energy is the energy required to remove one mole of electrons from one mole of gaseous +1 ions to form one mole of gaseous +2 ions. The second ionisation energy is always higher than the first because the electron is being removed from a positively charged ion, so there is greater electrostatic attraction holding the electron. For example, the first IE of magnesium is 738 kJ/mol, while the second IE is 1451 kJ/mol.