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The idea that matter is made of indivisible particles traces back to the ancient Greek philosopher Democritus (c. 460 BCE), who coined the word atomos meaning "uncuttable". Scientific atomic theory, however, did not emerge until John Dalton's work in 1808, which proposed that:
Dalton's model was refined dramatically over the next century:
| Year | Scientist | Contribution |
|---|---|---|
| 1897 | J.J. Thomson | Discovered the electron (cathode-ray experiments); "plum pudding" model |
| 1909 | Rutherford, Geiger, Marsden | Gold-foil experiment revealed a small, dense, positive nucleus |
| 1913 | Niels Bohr | Electrons in fixed energy levels (shells) |
| 1932 | James Chadwick | Discovered the neutron |
Rutherford's famous gold-foil experiment, in which most alpha particles passed straight through a thin gold foil but a few bounced back at large angles, was described by Rutherford himself as "almost as incredible as if you fired a 15-inch shell at a piece of tissue paper and it came back and hit you". It conclusively disproved the plum-pudding model and established the nuclear atom.
Atoms are the fundamental building blocks of matter. Despite being unimaginably small (around 10⁻¹⁰ m in diameter), they are themselves composed of three sub-atomic particles: protons, neutrons and electrons.
| Particle | Symbol | Relative Mass | Relative Charge | Location |
|---|---|---|---|---|
| Proton | p | 1 | +1 | Nucleus |
| Neutron | n | 1 | 0 | Nucleus |
| Electron | e⁻ | 1/1836 (≈ 0) | −1 | Orbitals around nucleus |
The actual masses and charges are:
| Particle | Mass (kg) | Charge (C) |
|---|---|---|
| Proton | 1.673 × 10⁻²⁷ | +1.602 × 10⁻¹⁹ |
| Neutron | 1.675 × 10⁻²⁷ | 0 |
| Electron | 9.109 × 10⁻³¹ | −1.602 × 10⁻¹⁹ |
The nucleus contains the protons and neutrons (collectively called nucleons) and holds almost all of the mass of the atom. The electrons occupy the much larger volume of space around the nucleus, arranged in orbitals.
Key Fact: If an atom were the size of a football stadium, the nucleus would be roughly the size of a pea at the centre circle. Atoms are overwhelmingly empty space.
The density of the nucleus is astonishing — around 2 × 10¹⁷ kg m⁻³. One teaspoon of nuclear matter would weigh around a trillion tonnes. This is the same density found in neutron stars.
Two numbers fully describe any particular nuclide:
The standard isotope notation is:
ZAX
For example, ²³Na (sodium-23) has:
flowchart LR
A[Atom] --> B[Nucleus]
A --> C[Electron cloud]
B --> D[Protons Z]
B --> E[Neutrons A - Z]
C --> F[Electrons in orbitals]
For each species, work out the number of protons, neutrons and electrons:
| Species | Protons | Neutrons | Electrons |
|---|---|---|---|
| ¹⁶O | 8 | 8 | 8 |
| ²⁰Ne | 10 | 10 | 10 |
| ³⁹K | 19 | 20 | 19 |
| ⁵⁶Fe | 26 | 30 | 26 |
| ²³⁸U | 92 | 146 | 92 |
When an atom gains or loses electrons it becomes an ion. Crucially, the number of protons does not change — only the electron count changes. Chemical reactions involve electrons only, never protons.
How many protons, neutrons and electrons are in ²⁷Al³⁺?
Note that Al³⁺ is isoelectronic with neon (both have 10 electrons and the configuration 1s² 2s² 2p⁶). This is why Al prefers to form 3+ ions: doing so gives it a stable noble-gas configuration.
How many protons, neutrons and electrons are in ³²S²⁻?
Again S²⁻ is isoelectronic with argon — the next noble gas after sulfur.
How many protons, neutrons and electrons are in ⁵⁶Fe³⁺?
Note Fe³⁺ is not isoelectronic with a noble gas — transition metals achieve stable half-filled or full d-subshell configurations instead.
Isotopes are atoms of the same element with the same number of protons but different numbers of neutrons.
Because they have the same number of protons (and in neutral atoms therefore the same number of electrons), isotopes of an element have identical chemical properties. Chemistry is governed by electron arrangement, and isotopes are electronically identical.
However, isotopes have slightly different physical properties (density, rate of diffusion, boiling point) because they have different masses.
| Element | Isotopes | Protons | Neutrons | Natural Abundance |
|---|---|---|---|---|
| Hydrogen | ¹H (protium) | 1 | 0 | 99.985% |
| Hydrogen | ²H (deuterium, D) | 1 | 1 | 0.015% |
| Hydrogen | ³H (tritium, T) | 1 | 2 | Trace (radioactive) |
| Carbon | ¹²C | 6 | 6 | 98.93% |
| Carbon | ¹³C | 6 | 7 | 1.07% |
| Carbon | ¹⁴C | 6 | 8 | Trace (radioactive, used for dating) |
| Chlorine | ³⁵Cl | 17 | 18 | 75.78% |
| Chlorine | ³⁷Cl | 17 | 20 | 24.22% |
| Uranium | ²³⁵U | 92 | 143 | 0.72% |
| Uranium | ²³⁸U | 92 | 146 | 99.27% |
Consider ³⁵Cl and ³⁷Cl. Both have 17 protons and 17 electrons arranged as 2,8,7. When chlorine reacts with sodium, both isotopes form Cl⁻ ions just as readily because the reaction involves the outer electron only. The extra two neutrons in ³⁷Cl make no difference to bonding behaviour.
Although chemical behaviour is identical, physical properties differ slightly:
Some isotopes are unstable and decay, emitting radiation. These radioisotopes have many applications: