AQA Boards Chemistry
The below links are for MARVEL and Diatomic Constants (DC)-type projects on Molecular Spectroscopy for Astrophysical Applications.
3.1.1.1 Fundamental Particles
- Appreciate that knowledge and understanding of atomic structure has evolved over time.
- Protons, neutrons and electrons: relative charge and relative mass.
- An atom consists of a nucleus containing protons and neutrons surrounded by electrons.
3.1.1.3 Electron Configuration
- Electron configurations of atoms and ions up to Z = 36 in terms of shells and sub-shells (orbitals) s, p and d.
3.2.5.4 Formation of coloured ions (A-level only)
- Colour arises when some of the wavelengths of visible light are absorbed and the remaining wavelengths of light are transmitted or reflected.
- The energy difference between the ground state and the excited state of the d electrons is given by:
ΔE = hν = hc/λ
- The absorption of visible light is used in spectroscopy
For some projects involving transition metals
For some projects involving transition metals
3.2.5.1 General properties of transition metals (A-level only)
- Transition metal characteristics of elements Ti–Cu arise from an incomplete d sub-level in atoms or ions. The characteristic properties include: formation of coloured ions and variable oxidation state.
3.2.5.4 Formation of coloured ions (A-level only)
- d electrons move from the ground state to an excited state when light is absorbed
- Changes in oxidation state, co-ordination number and ligand alter ΔE and this leads to a change in colour.
3.2.5.5 Variable oxidation states (A-level only)
- Transition elements show variable oxidation states.