relative masses of sub - atomic particles
proton: 1
neutron: 1
electron: 1/1850
relative charges of sub - atomic particles
proton: +1
neutron: 0
electron: -1
where are sub - atomic particles found?
protons and neutrons: in the nucleus
electrons: in energy levels
what force holds protons and neutrons together?
strong, nuclear force
what force holds protons and electrons together?
electrostatic FOA
isotope
atoms of the same element with the same number of protons and a different number of neutrons
have the same chemical properties (same electron configuration) and different physical properties (different mass numbers)
how to calculate the number of electrons in each energy level
2n^2 (n =2 N³ energy level)
energy levels get higher in energy as you move away from the nucleus (are quantised)
What does the quantum model suggest about electron orbitals?
electrons don’t orbit in a well - defined path
It shows complex shapes of orbitals/electron cloud (volume of space where there is likely to be an electron)
Quantum model is based on probability rather than certainty
how many orbitals can the s orbital hold?
how many electrons can it hold?
shape?
1 orbital
2 electrons
spherical
how many orbitals can the d orbital hold?
how many electrons can it hold?
5 orbitals
10 electrons
how many orbitals can the p orbital hold?
how many electrons can it hold?
shape?
3 orbitals
6 electrons
dumbbell shape (drawn as figure of 8)
how many orbitals can the f orbital hold?
how many electrons can it hold?
7 orbitals
14 electrons
electron spin
electrons have a property called spin
if 2 electrons are in the same orbital, one will spin up and one will spin down
When you get to the 3d sub - energy level, what happens?
4s is filled first as it has less energy
4s is further away from the nucleus, so when electrons are lost to form ions, they’re lost from 4s first
copper electron configuration
instead of filling 4s first, fill 3d first
1s2 2s2 2p6 3s2 3p6 4s1 3d10
chromium electron configuration
fills 1 electron in each 3d orbital to minimise repulsion and give it the lowest energy level possible
1s2 2s2 2p6 3s2 3p6 4s1 3d5
ionisation energy
energy required to remove 1 mole of electrons from 1 mole of gaseous atoms or ions to form 1 mole of positive ions
is endothermic as it needs to overcome the attraction between the nucleus and electrons
measured in kJ/mol (when plotting on a graph, use log10 function)
1st ionisation energy
enthalpy change needed to remove 1 mole of electrons from 1 mole of gaseous atoms to form 1 mole of gaseous ions with a single positive charge
Mg(g) —- Mg+(g) + e- (need to write state symbols)
2nd ionisation energy
enthalpy change needed to remove 1 mole of electrons from 1 mole of gaseous +1 ions to form 1 mole of gaseous ions with a +2 charge
Mg+(g) —- Mg2+(g) + e- (need to write state symbols)
enthalpy change
change in heat energy at constant pressure
factors affecting ionisation energy
shielding (affects it the most)
nuclear charge
electrons in orbitals
how shielding affects ionisation energy
more shielding means lower ionisation energy as there’s a weaker attraction between the outer electron and nucleus which requires less energy to overcome
how nuclear charge affects ionisation energy
higher nuclear charge means greater ionisation energy as there’s a stronger attraction between the nucleus and outer electrons so it can pull the electrons more closely (decreased atomic radius)
how electrons in orbitals affect ionisation energy
when electrons begin to pair in orbitals, they experience repulsion so it is easier to remove an electron, so it has a lower ionisation energy