Chapter 7 Periodicity Flashcards
Timeline of the atom 1803 - 1911
1803 - Dalton - Proposed that matter is made of tiny atoms.
1897 - Thompson - Realised that atoms are divisible and contain very tiny, negatively charged particles called electrons.
1911 - Rutherford - Realised atoms are made of a nucleus. The central nucleus is positvely charged and negative electrons revolve around this central nucleus
Timeline of the atom 1915 - 1932
1915 - Bohr - Proposed electrons orbit the nucleus in a set size and energy.
1924 - Pauli - Proposed the concept of an electron spin
1932 - Chadwick - Discovered atoms contain neutral particles called neutrons.
Ionisation energy
the amount of energy required to remove one electrons from each atom in one mole of gaseous atoms to form one mole of gaseous 1+ ions
How many ionisation energies can you have
As many ionisation energies as the amount of electrons
Periodicity
A regular periodic variation of properties of element with atomic number and position in the periodic table.
Factors affecting the ionisation energy
Atomic Radius - the force of attraction falls off sharply with increasing distance.
Nuclear charge - The number of protons. The greater the attraction between the nucleus and the outer electrons.
Electron shielding - Electrons are negatively charged so inner shell electrons will repel. Shielding effect.
How can you tell Successive ionisation energies and shells
You can tell when there is a switch between shells. This is when there is a big jump on the graph.
Trend in first ionisation energy down a group
First ionisation energy decrease down a group. Although the nuclear energy increase, its effect is outweighed by the increased radius and, to a less extent, the increased shielding.
Trend in the first ionisation energy across a period
There is a general increase in first ionisation energy across the first three periods. At some points across the period there are drops in ionisation energy. These can be as a result of sub shells since they are filled up.
Metallic Bonding
Bonding for metals
Delocalised electrons spread out around the structure.
The cations are fixed in position maintaining the structure.
Electrons are able to move.
The ions create a giant metallic lattice.
Properties of metals
Strong metallic bonds - attracction between positive ions and delocalised electrons.
High electrical conductivity
High melting and boiling points.
Electrical conductivity of metals
Conduct as solid and liquid.
When voltage is applied the delocalised electrons can move through the structure.
Melting and Boiling points of metals
High melting and boiling points. This point depends on the strength of the metallic bonds holding together the atoms in the giant metallic lattice.
Giant covalent structures
With non metals, many billion atoms are held together by a network of strong covalent bonds to form a giant covalent lattice.
Melting and Boiling points of giant covalent
high melting and boiling points. This is because there are covalent bonds which are strong. High temperatures are necessary to provide the large quantity of energy needed to break the strong covalent bonds