Important Groups
3. Group 0/18: Noble Gases
Learning outcomes
- I can identify the noble gases on the periodic table.
- I can describe the physical properties of noble gases.
- I can explain why noble gases are generally unreactive.
- I can relate noble gas stability to electron arrangements.
- I can describe practical applications of noble gases.
What Are the Noble Gases?
The noble gases are the elements found in Group 18 of the modern periodic table.
In some school systems and older textbooks, this group is called Group 0.
The noble gases are:
- helium (He)
- neon (Ne)
- argon (Ar)
- krypton (Kr)
- xenon (Xe)
- radon (Rn)
- oganesson (Og)
The first six are the noble gases most commonly discussed in introductory chemistry.
Noble gases are unusual because they are extremely unreactive compared with most other elements.
Finding the Noble Gases
Group 18 is the vertical column on the far-right side of the periodic table.
Moving down the group:
He → Ne → Ar → Kr → Xe → Rn → Og
Their position at the end of each period is closely connected to their electron arrangements and chemical stability.
Electron Arrangements of Noble Gases
The most important feature of noble gases is their complete outer electron shell.
Helium:
2
Neon:
2,8
Argon:
2,8,8
Neon and the other main-group noble gases have eight valence electrons in their outer shell.
Helium is the exception.
Its first shell can hold only two electrons, so helium is stable with:
2 electrons
A Full Outer Electron Shell
Atoms often react because gaining, losing, or sharing electrons can produce a more stable electron arrangement.
Noble gases already have very stable outer electron arrangements.
They therefore have little tendency to:
- gain electrons
- lose electrons
- share electrons
This explains their very low chemical reactivity.
Why Are Noble Gases Unreactive?
Consider neon.
Its electron arrangement is:
2,8
Its outer shell is already full.
Neon does not need to gain an electron because the outer shell is complete.
It also does not readily lose electrons because removing electrons from this stable arrangement requires considerable energy.
Therefore, neon usually remains as individual:
Ne atoms
rather than forming ions or molecules.
Stability and Electron Arrangements
The stability of noble gases helps explain why many other elements react.
For example:
Sodium:
2,8,1
can lose one electron to form:
Na⁺ → 2,8
Chlorine:
2,8,7
can gain one electron to form:
Cl⁻ → 2,8,8
Both ions then have electron arrangements corresponding to nearby noble gases.
This is one reason noble-gas configurations are so important in understanding chemical bonding.
The Octet Rule
A useful introductory model is the octet rule.
Many main-group atoms tend to gain, lose, or share electrons in ways that give them eight electrons in their outer shell.
The rule helps explain many simple examples of:
- ionic bonding
- covalent bonding
- ion formation
However, it is a useful model rather than an absolute rule. There are many important exceptions in chemistry.
Helium and the Duet Rule
Helium does not have eight valence electrons.
It has only:
2 electrons
Why is it stable?
The first electron shell can hold a maximum of only two electrons.
Therefore, helium's first shell is completely filled.
This is sometimes described using the duet rule.
Helium is therefore chemically stable even though it does not have an octet.
Noble Gases Are Monatomic
Many elements exist naturally as molecules.
For example:
Hydrogen = H₂
Oxygen = O₂
Chlorine = Cl₂
Noble gases are different.
They normally exist as individual atoms.
This is described as:
monatomic
For example:
He
Ne
Ar
rather than He₂, Ne₂, or Ar₂.
Why Are Noble Gases Monatomic?
A covalent bond forms when atoms share electrons.
Noble gas atoms already have stable outer electron arrangements.
They therefore have little tendency to form ordinary covalent bonds with another identical atom.
As a result, ordinary samples of noble gases consist mainly of separate atoms.
Physical Properties of Noble Gases
Noble gases share several physical properties.
They are generally:
- gases at room temperature
- colourless
- odourless
- monatomic
- non-flammable
- low-density compared with liquids and solids
- relatively low in melting and boiling points
They are also poor electrical conductors under ordinary conditions.
Noble Gases Are Colourless
The gases themselves are colourless under ordinary conditions.
This is important because noble gases are often associated with colourful lights.
The colours seen in gas-discharge tubes occur when electrical energy excites electrons in the atoms.
When the electrons return to lower energy levels, they emit light at characteristic wavelengths.
The gas itself is not naturally glowing or coloured.
Melting and Boiling Points
Noble gases have very low melting and boiling points.
However, both generally increase down Group 18.
So:
He → Ne → Ar → Kr → Xe → Rn
shows an overall increase in melting and boiling temperatures.
This means helium remains a gas at much lower temperatures than xenon.
Why Boiling Points Increase Down the Group
Moving down Group 18:
- atoms become larger
- the number of electrons increases
- electron clouds become more polarizable
- London dispersion forces between atoms become stronger
Therefore, more energy is needed to separate the atoms.
As a result:
boiling point generally increases down the group.
Density Down Group 18
Density also generally increases down Group 18.
Helium has a very low density.
Heavier noble gases such as krypton and xenon are considerably denser.
The increase occurs largely because the atoms become progressively more massive down the group.
Are Noble Gases Completely Inert?
Noble gases were once often described as inert gases, meaning that they did not react chemically.
Today, we know this description is not completely accurate.
The heavier noble gases, especially xenon, can form compounds under suitable conditions.
Examples include compounds containing xenon and fluorine.
Therefore, it is more accurate to say:
noble gases are generally very unreactive
rather than:
noble gases never react.
Why Heavier Noble Gases Can React
Moving down Group 18:
- atomic radius increases
- shielding increases
- outer electrons become farther from the nucleus
- first ionization energy generally decreases
This means the outer electrons of heavier noble gases are held somewhat less strongly than those of lighter noble gases.
As a result, elements such as xenon can participate in some reactions under suitable conditions.
Noble Gases and Ionization Energy
Noble gases have relatively high first ionization energies because of their stable electron arrangements.