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Ionisation Energy Trends Simplified Revision Notes

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Ionisation Energy Trends

Introduction to Ionisation Energy

Ionisation Energy: The energy required to remove an electron from a neutral gaseous atom. It is a fundamental concept in chemistry, essential for understanding the reactivity and stability of elements. Lower ionisation energies indicate higher reactivity, especially among metals.

infoNote

Definition: Ionisation energy: the energy necessary to remove an electron from a neutral gaseous atom, resulting in the formation of a cation. This measurement is vital for predicting chemical behaviours and interactions.

Fundamental Concepts of Ionisation Energy

First Ionisation Energy

  • First ionisation energy: The energy required to remove the first electron from a neutral atom.
  • This metric reflects an element's reactivity and stability.
  • Each successive electron removal necessitates more energy due to the increased positive charge on the cation.
infoNote

Definition: First ionisation energy: the energy required to remove the first electron from a neutral atom.

Successive Ionisation Energies

  • Ionisation energy increases with each electron removed, as a result of the heightened nuclear charge.
  • Example: Sodium (Na):
    • First electron removal: Na to Na+
    • Additional electrons require increasing energy.
  • Attaining a noble gas configuration enhances stability, complicating further ionisation.
chatImportant

Successive ionisation energies showcase the growing stability associated with noble gas configurations.

Formula for Ionisation Energy

Ionisation energy can be determined using the following equation:

IE=Eatom(Eion+Eelectron)IE = E_{\text{atom}} - (E_{\text{ion}} + E_{\text{electron}})

  • IE = Ionisation Energy
  • It represents the difference between the initial energy and the energy post-ionisation.

Numeric Example

  • Initial energy of atom (EatomE_{\text{atom}}) = 500 kJ/mol
  • Energy of resulting ion plus electron (Eion+EelectronE_{\text{ion}} + E_{\text{electron}}) = 200 kJ/mol

Calculation:

IE=500200=300 kJ/molIE = 500 - 200 = 300 \text{ kJ/mol}

This shows the energy necessary to remove an electron.

Trends in Ionisation Energy

Across a Period

  • Increases from left to right due to an increased nuclear charge, leading to a stronger attraction of electrons.
  • Atomic Radius: Decreases across a period, resulting in stronger electron-nucleus interactions.
  • Notable Exceptions:
    • Be vs. B: The filled s-subshell in Be requires more energy than in B.
    • N vs. O: Electron pairing in O decreases the energy compared to N.

Figure 1: Periodic Trend Diagram

Down a Group

  • Decreases down a group because:
    • Increasing atomic size places electrons further from the nucleus.
    • Enhanced electron shielding: Additional inner electrons reduce the nuclear attraction to outer electrons.

Figure 2: Group Trend Diagram

Exceptional Cases

Beryllium vs. Boron

  • Despite being to the right of beryllium, boron demonstrates lower ionisation energy.
  • The extra electron enters a higher-energy p-subshell.

Electron configurations of Beryllium and Boron

Nitrogen vs. Oxygen

  • Oxygen exhibits lower ionisation energy than nitrogen due to electron pairing, which increases repulsion.

Electron configurations of Nitrogen/Oxygen

Factors Influencing Ionisation Energy

Key Influencing Factors

  1. Atomic Size:

    • A larger size corresponds with lower ionisation energy.
    • Electrons that are more distant from the nucleus are more easily removed.
  2. Nuclear Charge:

    • A higher nuclear charge increases the energy required to remove an electron.
  3. Electron Shielding:

    • Inner electrons diminish the nuclear pull on outer electrons.
    • Greater shielding results in lower required energy.

Diagram illustrating atomic size and electron shielding

Ionisation Energy in Practical Applications

  • Industrial Relevance: Metals with low ionisation energy, such as sodium and potassium, are highly reactive.
  • Comparison Table:
MetalFirst Ionisation Energy (kJ/mol)Reactivity Level
Lithium520.2Low
Sodium495.8Medium
Potassium418.8High

Calculation Methods

  1. Spectroscopy:

    • Emission lines reflect energy levels.
  2. Photoelectron Spectroscopy (PES):

    • It measures the kinetic energy of electrons after ejection, providing precise ionisation energy assessment.
  3. Einstein's Equation:

    • Calculate ionisation energy using KEmax=hfIEKE_{\text{max}} = hf - IE

Spectroscopy diagram

Key Study Points

  • Trends: Ionisation energy increases across a period and decreases down a group.
  • Essential Concepts:
    • Atomic Radius affects electron removal ease.
    • Nuclear Charge & Shielding are influential factors.
  • Exceptions: Observe energy variations due to electron shell configurations.

Practice Problems

Problem 1: Period Trend

  • Arrange elements by increasing first ionisation energy within Period 2.
    • Solution: Li < Be < B < C < N < O < F < Ne (Elements are arranged from lowest to highest ionisation energy, following the general trend across Period 2)

Period Trend Diagram

Problem 2: Group Trend

  • Compare ionisation energies in Group 1: Li > Na > K.
    • Solution: This ordering is correct. Ionisation energy decreases down Group 1, with Li having the highest and K the lowest due to increasing atomic radius and electron shielding.

Group Trend Diagram

Calculation Exercise

  • Given frequency f=6×1014f = 6 \times 10^{14} Hz, compute ionisation energy using Planck's constant.
    • Solution: Using KEmax=hfIEKE_{\text{max}} = hf - IE, where h=6.626×1034h = 6.626 \times 10^{-34} J·s
    • IE=hfKEmaxIE = hf - KE_{\text{max}}
    • If KEmax=0KE_{\text{max}} = 0 (threshold frequency case), then IE=hf=6.626×1034×6×1014=3.98×1019IE = hf = 6.626 \times 10^{-34} \times 6 \times 10^{14} = 3.98 \times 10^{-19} J per atom
    • Converting to kJ/mol: 3.98×1019 J/atom×6.022×1023 atoms/mol×103 kJ/J239.7 kJ/mol3.98 \times 10^{-19} \text{ J/atom} \times 6.022 \times 10^{23} \text{ atoms/mol} \times 10^{-3} \text{ kJ/J} \approx 239.7 \text{ kJ/mol}
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