Topic 1: Atomic Structure and the Periodic
Table
Atomic Structure
Atoms consist of a nucleus surrounded by shells of electrons
The nucleus consists of protons and neutrons
The protons in the nucleus causes a positive charge
The electrons orbit the nucleus and have a negative charge
Atomic and Mass Numbers
The Atomic Number is the number of protons in an atom
The Mass Number is the number of protons and neutrons in an atom
The Mass Number displayed on the Periodic Table is the average mass number based on
the relative abundancy of the different isotopes of the element
Isotopes and Ions
An Isotope is an element whose atomic number is the same but the mass
number(number of neutrons) is different.
Isotopes only have different numbers of neutrons. The number of protons and electrons
is the same
Ions are charged atoms which have a different number of electrons
Positive Ions have lost electrons
Negative Ions have gained electrons
Protons determine the element. Changing the number of protons means a new element
is formed
Relative Masses
The Relative Atomic Mass of an element is the average mass of all the isotopes of an
atom relative to the mass of 1/12 of the mass of Carbon-12
The Relative Isotopic Mass is the mass of an isotope of an element relative to the mass
of 1/12 of the mass of Carbon-12
The Relative Molecular Mass is the average mass of all the atoms in a moleculerelative
to the mass of 1/12 of the mass of Carbon-12
Carbon-12 is used because it is a stable and abundant isotope
Mass Spectrometry
Mass spectrometers can be used to determine all the isotopes present in a sample of an
element and their percentage or relative abundancy.
The relative atomic mass quoted on the periodic table is a weighted average of all the
isotopes of an element
The data collected from a mass spectrum can help to calculate a relative atomic mass:
RAM = Σ (isotopic mass x % abundancy)
100
RAM =Σ (isotopic mass x relative abundancy)
total relative abundancy
Chlorine has 2 isotopes: Cl-35 (75%) and Cl-37 (25%) so the RAM is calculated to be 35.5
On a mass spectrum however, there will be three peaks at 70, 72 and 74 due the
presence of the different isotopes in each molecule (35-35; 35-37; 37-37)
Mass spectrometers are used for:
Drug testing in sports to identify chemicals in the blood
Quality control in the pharmaceutical industry
Radioactive Carbon-13 Dating to determine ages of fossils or human remains
Testing rocks on different planets
Ionisation Energies
The first ionisation energy is the energy required when one mole of gaseous
atoms forms one mole of gaseous ions with a 1+ charge
X(g) –> X+(g) + e-
The second ionisation energy is the energy required when one mole of gaseous
ions with a 1+ charge forms one mole of gaseous ions with a 2+ charge
X+(g) –> X2+(g) + e-
Ionisation energies are affected by:
The attraction of the nucleus (the more protons, the greater the attraction)
The distance of the valence electrons from the nucleus (the further from the nucleus,
the weaker the attraction)
The shielding provided by the electrons (the more electrons infront of the valence
electrons, the weaker the attraction)
Helium has the highest first ionisation energy because its nuclear attraction is
strongest as the atomic radius is shorter than other atoms and there is no shielding
Successive ionisation energies are always larger because there is a greater
positive:negative charge ratio as there are fewer electrons and the ionic radius is smaller
Ionisation Energies and Electronic Structures
The more electrons removed from an atom, the higher the ionisation energy as there
are more protons to electrons so the nuclear attraction is greater for each subsequent electron
removed
A larger jump in Succesive Ionisation energy can be seen when an electron is removed
from a shell closer to the nucleus as there is less shielding and the distance is smaller
Nobel Gases have higher first ionisation energies as they have the most protons with
the least amounts of shielding
A large drop in first ionisation energies occurs between the Nobel Gases and Group
1 metals as shielding increases weakening the nuclear attraction and causing electrons to
be more easily lost
Small drops in first ionisation energies can be seen between Group 2 and 3elements (e.g.
Be and B) as the electrons are removed from a different subshell
Small drops in first ionisation energies can be seen between Group 5 and 6elements (e.g.
N and O) as the electrons start to pair up in a subshell
Graph of First Ionisation Energies
Electronic Structure of the Atom
Electrons are arranged into principle energy levels (shells) which are split into sub
energy levels (subshells) and can contain a certain number of electrons.
Subshells are split into
s (holds up to 2 electrons)
p (holds up to 6 electrons)
d (holds up to 10 electrons)
f (holds up to 14 electrons)
Subshells are made up of orbitals which hold up to two electrons of opposite spin
Orbitals represent the mathematical propabilities of finding an electron at any point
within certain spatial distributions around the nucleus
s subshells are spherical
p subshells have a dumbbell shape
The periodic table is split into block based on the subshell that the valence electron is
found
Electronic Configurations
An atom fills up the subshells in order of increasing energy
The 3d subshell is higher in energy than the 3d subshell so gets filled after the 4s
1s > 2s > 2p > 3s > 3p > 4s > 3d > 4p > 5s > 4d > 5p
An electronic configuration includes the main energy level, the name of type of sub-
level and the number of electrons in the sub-level e.g. Oxygen = 1s2 2s2 2p4
Spin diagrams can be drawn to show the number of electrons and the spin of the
electrons in the orbitals of an element.
When filling up sublevels with several orbitals, the orbital are filled individuallybefore electrons
start to pair up
Periodicity
Periodicity is the trend of chemical and physical properties across a period or down a
group of elements
Atomic Radius decreases across a period as there are more protons so the nuclear
charge is greater and pulls the electrons in more
Atomic Radius increases down a group as more shells and increased shielding weaken the
nuclear attraction on the valence electrons
First Ionisation Energy tends to increase across a period due to an increase in protons
providing a stronger nuclear attractive force on the electrons
First Ionisation Energy tends to decrease down a group because the increased number of shells
results in shielding weakening the nuclear attractive force
Melting Points are based on bonding and intermolecular forces within the elements.
For Na, Mg and Al – These elements have metallic bonding so the increase in outer electrons
and a smaller ion results in a larger melting point
For Si – Silicon is a macromolecular substance so requires a lot of energy to break the multiple
covalent bonds in the structure
For Cl2, S8, P4 and Ar – These elements exist as simple molecular substances that have
weak Van der Waals Forces between them so less energy is required to break these
Intermolecular Forces. The more electrons they have in a molecule, the higher the m.p.