Chemistry30 views·Updated 29 Jun 2026·7 pages

Understanding Ionization Energies and Atomic Structure

Alexia C. Tario@kikki_05

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Understanding atomic structure is crucial for mastering chemistry - it's...

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$Charge Mass Prime Tuition Nucleus $\rightarrow$ Protons +1 1 $\rightarrow$ Neutrons 0 1 $\rightarrow$ Electrons -1 0 $A_R$ = Relative atom$

Atomic Structure Basics

Every atom is made up of three fundamental particles that determine its identity and behaviour. The nucleus contains protons $charge +1, mass 1$ and neutrons (charge 0, mass 1), whilst electrons $charge -1, mass 0$ orbit around it.

Your atomic number tells you exactly how many protons and electrons an atom has - they're always equal in a neutral atom. The atomic mass is simply the total number of protons plus neutrons, which gives you the atom's weight.

Isotopes are atoms of the same element that have different numbers of neutrons but identical numbers of protons and electrons. For example, carbon can exist as ¹²C, ¹³C, and ¹⁴C - all with 6 protons but 6, 7, or 8 neutrons respectively. Since chemical properties depend on electrons, all isotopes of an element behave identically in reactions.

Quick Tip: Remember that atomic number = protons = electrons, whilst atomic mass = protons + neutrons.

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$Charge Mass Prime Tuition Nucleus $\rightarrow$ Protons +1 1 $\rightarrow$ Neutrons 0 1 $\rightarrow$ Electrons -1 0 $A_R$ = Relative atom$

Relative Atomic Mass and Mass Spectrometry

Relative atomic mass (Ar) isn't just a simple average - it's a weighted average that accounts for how common each isotope is in nature. The formula is: Ar = Σ(% abundance × isotopic mass) ÷ Σ(% abundance).

Let's see this in action with copper. Cu-63 makes up 69.2% of natural copper, whilst Cu-65 accounts for 30.8%. Using the formula: Ar = [(69.2 × 63) + (30.8 × 65)] ÷ 100 = 63.6.

Mass spectrometry is the technique scientists use to identify these isotopes and their abundances. The process involves four key steps: ionisation (creating charged particles), acceleration (speeding them up), ion drift (separating by mass), and detection (measuring the results).

Real World: Mass spectrometry is used in everything from drug testing to space exploration!

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$Charge Mass Prime Tuition Nucleus $\rightarrow$ Protons +1 1 $\rightarrow$ Neutrons 0 1 $\rightarrow$ Electrons -1 0 $A_R$ = Relative atom$

Electron Shells and Orbitals

Electrons don't just randomly orbit the nucleus - they occupy specific energy levels called shells. Think of these like the floors of a building, where each floor can only hold a certain number of residents.

The maximum number of electrons in each shell follows the 2n² rule, where n is the shell number. Shell 1 holds 2 electrons, shell 2 holds 8, shell 3 holds 18, and shell 4 holds 32 electrons maximum.

Within each shell, electrons occupy sub-shells (s, p, d, f) that have different shapes and capacities. The s sub-shell holds 2 electrons, p holds 6, d holds 10, and f holds 14. Shell 1 only has s, shell 2 has s and p, shell 3 has s, p, and d, whilst shell 4 contains all four types.

Memory Trick: The sub-shell capacities (2, 6, 10, 14) follow the pattern of adding 4 each time!

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$Charge Mass Prime Tuition Nucleus $\rightarrow$ Protons +1 1 $\rightarrow$ Neutrons 0 1 $\rightarrow$ Electrons -1 0 $A_R$ = Relative atom$

Orbital Shapes and Electron Configuration

Orbitals have distinct shapes that determine where you're likely to find electrons. The s orbital is spherical, whilst p orbitals are dumbbell-shaped and come in three orientations (px, py, pz) pointing along different axes.

When writing electron configurations, you fill orbitals starting from the lowest energy level. For example, carbon (6 electrons) has the configuration 1s² 2s² 2p², showing exactly where each electron resides.

The filling pattern follows a specific order: 1s, 2s, 2p, 3s, 3p, 4s, 3d, 4p, and so on. Notice that 4s fills before 3d because it's actually at a lower energy level despite being in the "fourth shell".

Study Tip: Draw out the orbital filling diagram - visual learners find this much easier than memorising the sequence!

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$Charge Mass Prime Tuition Nucleus $\rightarrow$ Protons +1 1 $\rightarrow$ Neutrons 0 1 $\rightarrow$ Electrons -1 0 $A_R$ = Relative atom$

Advanced Electron Configuration Rules

Pauli's Exclusion Principle states that each orbital can hold a maximum of two electrons, and they must have opposite spins (represented as ↑↓). This prevents electrons from occupying the same space with identical properties.

When electrons enter orbitals of equal energy (like the three p orbitals), they prefer to occupy separate orbitals first before pairing up. This Hund's rule minimises electron repulsion and creates more stable atoms.

Shorthand notation makes writing electron configurations much quicker. Instead of writing out every orbital, you can use the nearest noble gas in brackets. For example, calcium (20 electrons) becomes [Ar] 4s² rather than the full 1s² 2s² 2p⁶ 3s² 3p⁶ 4s².

Exam Tip: Learn the electron configurations of the first 20 elements - they appear in most chemistry exams!

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$Charge Mass Prime Tuition Nucleus $\rightarrow$ Protons +1 1 $\rightarrow$ Neutrons 0 1 $\rightarrow$ Electrons -1 0 $A_R$ = Relative atom$

Ionisation Energy Fundamentals

Ionisation energy is the energy needed to remove one mole of electrons from one mole of gaseous atoms, creating positive ions. It's measured in kJ/mol and tells you how tightly an atom holds onto its electrons.

The process can happen multiple times: first ionisation energy removes the first electron $X → X⁺ + e⁻$ , second ionisation energy removes the second $X⁺ → X²⁺ + e⁻$ , and so on. Each successive ionisation requires more energy because you're removing electrons from increasingly positive ions.

Down a group, ionisation energy decreases dramatically. As you move from lithium to sodium to potassium, the atoms get larger and the outer electrons become further from the nucleus. This weaker nuclear attraction makes electrons easier to remove.

Key Insight: Ionisation energy patterns help explain why metals lose electrons easily whilst non-metals prefer to gain them!

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$Charge Mass Prime Tuition Nucleus $\rightarrow$ Protons +1 1 $\rightarrow$ Neutrons 0 1 $\rightarrow$ Electrons -1 0 $A_R$ = Relative atom$

Ionisation Energy Trends

Across a period, ionisation energy generally increases from left to right. As you move from lithium to neon, the nuclear charge increases whilst the atomic radius decreases slightly, creating a stronger pull on the electrons.

However, there are important exceptions to this trend. Boron has a lower ionisation energy than beryllium because its electron is in a higher energy p orbital. Similarly, oxygen's ionisation energy is slightly lower than nitrogen's due to electron repulsion in paired orbitals.

These periodic trends in ionisation energy help predict chemical behaviour. Elements with low ionisation energies (like sodium) readily form positive ions, whilst those with high ionisation energies (like fluorine) prefer to gain electrons instead.

Exam Focus: Learn the exceptions to the general trend - examiners love testing these anomalies!

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Chemistry30 views·Updated 29 Jun 2026·7 pages

Understanding Ionization Energies and Atomic Structure

Alexia C. Tario@kikki_05

Add to Google sources

Understanding atomic structure is crucial for mastering chemistry - it's the foundation that explains how elements behave and react. You'll explore everything from the basic parts of an atom to electron configurations and ionisation energy trends.

of 7

$Charge Mass Prime Tuition Nucleus $\rightarrow$ Protons +1 1 $\rightarrow$ Neutrons 0 1 $\rightarrow$ Electrons -1 0 $A_R$ = Relative atom$

Atomic Structure Basics

Quick Tip: Remember that atomic number = protons = electrons, whilst atomic mass = protons + neutrons.

of 7

$Charge Mass Prime Tuition Nucleus $\rightarrow$ Protons +1 1 $\rightarrow$ Neutrons 0 1 $\rightarrow$ Electrons -1 0 $A_R$ = Relative atom$

Relative Atomic Mass and Mass Spectrometry

Let's see this in action with copper. Cu-63 makes up 69.2% of natural copper, whilst Cu-65 accounts for 30.8%. Using the formula: Ar = [(69.2 × 63) + (30.8 × 65)] ÷ 100 = 63.6.

Real World: Mass spectrometry is used in everything from drug testing to space exploration!

of 7

$Charge Mass Prime Tuition Nucleus $\rightarrow$ Protons +1 1 $\rightarrow$ Neutrons 0 1 $\rightarrow$ Electrons -1 0 $A_R$ = Relative atom$

Electron Shells and Orbitals

Memory Trick: The sub-shell capacities (2, 6, 10, 14) follow the pattern of adding 4 each time!

of 7

$Charge Mass Prime Tuition Nucleus $\rightarrow$ Protons +1 1 $\rightarrow$ Neutrons 0 1 $\rightarrow$ Electrons -1 0 $A_R$ = Relative atom$

Orbital Shapes and Electron Configuration

Study Tip: Draw out the orbital filling diagram - visual learners find this much easier than memorising the sequence!

of 7

$Charge Mass Prime Tuition Nucleus $\rightarrow$ Protons +1 1 $\rightarrow$ Neutrons 0 1 $\rightarrow$ Electrons -1 0 $A_R$ = Relative atom$

Advanced Electron Configuration Rules

Exam Tip: Learn the electron configurations of the first 20 elements - they appear in most chemistry exams!

of 7

$Charge Mass Prime Tuition Nucleus $\rightarrow$ Protons +1 1 $\rightarrow$ Neutrons 0 1 $\rightarrow$ Electrons -1 0 $A_R$ = Relative atom$

Ionisation Energy Fundamentals

Key Insight: Ionisation energy patterns help explain why metals lose electrons easily whilst non-metals prefer to gain them!

of 7

$Charge Mass Prime Tuition Nucleus $\rightarrow$ Protons +1 1 $\rightarrow$ Neutrons 0 1 $\rightarrow$ Electrons -1 0 $A_R$ = Relative atom$

Ionisation Energy Trends

Exam Focus: Learn the exceptions to the general trend - examiners love testing these anomalies!