Small, dense central nucleus surrounded by orbiting electrons in electron shells
Nucleus
Consists of protons and neutrons
Has an overall positive charge
Contains almost the entire mass of the atom
Neutral atom
Number of electrons is equal to the number of protons due to the relative charges
Fundamental particles
Proton
Neutron
Electron
Proton
Relative charge +1, Relative mass 1
Neutron
Relative charge 0, Relative mass 1
Electron
Relative charge -1, Relative mass 1/1840
Maximum number of electrons in a shell
2n^2 where n is the shell number
Each electron shell must fill before the next one can hold any electrons
Mass number (A)
Sum of protons and neutrons in an atom
Atomic number (Z)
Equal to the number of protons in an atom
Isotopes
Hydrogen
Deuterium
Tritium
Isotopes
Atoms of the same element with the same atomic number but different number of neutrons, resulting in a different mass number
Neutral atoms of isotopes will react chemically in the same way as their proton number and electron configuration is the same
Different mass numbers of isotopes mean they have different physical properties
Relative atomic mass (Ar)
The mean mass of an atom of an element, relative to one twelfth of the mean mass of an atom of the carbon-12 isotope
Relative isotopic mass
The isotopic mass of an isotope relative to one twelfth of the mean mass of an atom of the carbon-12 isotope
Relative molecular mass (Mr)
The mean mass of a molecule of a compound, relative to one twelfth of the mean mass of an atom of the carbon-12 isotope
Relative molecular mass can be calculated for a molecule by adding together the separate Ar values of the component elements
Ions
Formed when an atom loses or gains electrons, meaning it is no longer neutral and will have an overall charge
Mass spectrometry
Used to identify different isotopes and find the overall relative atomic mass of an element
Time of Flight (TOF) Mass Spectrometry
1. Ionisation
2. Acceleration
3. Ion Drift
4. Detection
5. Analysis
During the ionisation process, a 2+ charged ion may be produced, which will be affected more by the magnetic field producing a curved path of smaller radius
The tallest peak on a mass spectrum corresponds to the relative molecular mass of the molecule, this peak is known as the molecular ion peak and is formed from the M+ species
Spectra produced by the mass spectrometry of chlorine display a characteristic pattern in a 3:1 ratio for Cl+ ions and a 3:6:9 ratio for Cl2+ ions
Ionisation energy
The minimum energy required to remove one mole of electrons from one mole of atoms in a gaseous state, measured in kJmol-1
Successive ionisation energies usually require more energy because as electrons are removed, the electrostatic force of attraction between the positive nucleus and the negative outer electron increases
Along a Period
First ionisation energy increases due to a decreasing atomic radius and greater electrostatic forces of attraction
Down a Group
First ionisation energy decreases due to an increasing atomic radius and electron shielding which reduces the effect of the electrostatic forces of attraction
A sudden large increase in successive ionisation energies indicates a change in energy level, because the electron is being removed from an orbital closer to the nucleus so more energy is required
The first ionisation energy of Aluminium is lower than expected due to a single pair of electrons with opposite spin, resulting in a natural repulsion which reduces the amount of energy needed to be put in to remove the outer electron
Evidence for electron configurations
Emission spectra provide evidence for the existence of quantum shells
Successive ionisation energies provide evidence for quantum shells within atoms and suggest the group to which the element belongs
The first ionisation energy of successive elements provides evidence for electron subshells
Electron orbitals
Electrons are held in clouds of negative charge called orbitals, of types s, p, d and f, each of which can hold up to two electrons with opposite spins and has a different shape
Each element in the blocks on the Periodic Table has outer electrons in the corresponding orbital type
Electron configurations
Scientific ideas on electronic configurations have developed over time as new discoveries are made
Current, accepted model of electron configurations
Based on evidence from emission spectra, successive ionisation energies, and first ionisation energy
Orbitals
Clouds of negative charge where electrons are held
Types of orbitals
s
p
d
f
Orbitals
Each one can hold up to two electrons with opposite spins and has a different shape
Blocks on the Periodic Table
Correspond with different types of orbitals, each element in the block has outer electrons in that orbital