How Atomic Models Evolved
Dalton
Atom is a solid, indivisible particle
Thomson
Electrons embedded in a positive sphere (plum pudding)
Rutherford
Tiny dense nucleus; electrons revolve around it
Bohr
Electrons in fixed energy levels → atom is stable
Modern model — electrons as “electron clouds”
Atoms
The building blocks of matter.
Thomson’s model
Electrons embedded in a positively charged sphere.
Rutherford’s model
Mostly empty space with a dense, positive nucleus at the centre and electrons orbiting.
Bohr’s model
Electrons move in fixed energy levels (shells) around the nucleus.
Shells
Named K, L, M, N… from the nucleus outward.
Subatomic particles
Electrons (−1), protons (+1) and neutrons (0); neutron found by Chadwick.
Octet
A full outermost shell of 8 electrons (2 for helium) → stable, unreactive.
Valency
The combining capacity — electrons gained, lost or shared for a stable configuration.
Atomic number (Z)
Number of protons in the nucleus.
Mass number (A)
Total nucleons = protons + neutrons.
Isotopes
Same atomic number, different mass numbers.
Average atomic mass
Based on the relative abundance of the isotopes in nature.
Isobars
Different elements with the same mass number but different atomic numbers.
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