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Democritus
460 BC
Greek philosopher
Particle Theory of Matter
discovered ATOMS - retain identity in a chemical reaction
John Dalton
1804
Solid Sphere Model
atoms of one element are all the same, combine in whole-number ratios to form compounds, and can’t be broken down

J.J. Thomson
1897
Plum Pudding Model
Discovered electrons in Cathode Ray Tube experiment

Robert Millikan
1909
Oil Drop Experiment
determined negative charge and mass of electrons
Ernest Rutherford
1911
Nuclear Model
Gold Foil experiment →alpha particles deflected by a positive NUCLEUS

Niels Bohr
1913
Planetary Model
Electrons orbit the nucleus at fixed energy levels

Erwin Schrodinger & Werner Heisenberg
1926
Quantum Model
Heisenberg Uncertainty Principle: an electron’s position and velocity of an electron cannot be determined at the same time

James Chadwick
1932
Discovered NEUTRON
Protons
positive subatomic particles found in the nucleus with a mass of about 1 amu. The number of protons = atomic number (z)

Neutrons
neutral subatomic particles found in the nucleus with a mass of about 1 amu. They act as the glue that holds together the nucleus
Electrons
negatively charged subatomic particles found in the electron cloud that have almost no mass
Isotopes
Atoms of the same element with differing numbers of neutrons, resulting in varying atomic masses.
Ions
Atoms that have gained or lost electrons, resulting in a net charge.
Cations
positive ions (lost electrons)
Anions
negative ions (gained electrons)
Average Atomic Mass (AAM)
AAM = (mass1)(% abundance1) + (mass2)(% abundance2)
Nuclear Notation

Radioactivity
the spontaneous emission of radiation in the form of particles or high-energy photons resulting from nuclear reactions
Pierre & Marie Curie = first to use the term radioactive
Ernest Rutherford = set the laws for radioactive decay
Nuclear reactions vs Chemical reactions
Nuclear: protons and neutrons in nucleus are rearranged → releases tremendous amount of energy
Chemical: involve electrons
Nuclear stability
the stability of a nucleus is dependent on the neutron (N) to proton (Z) ratio (N : Z)
For light nuclei (elements 1-20), N : Z should be 1 : 1
For heavy nuclei (elements above 20), N : Z should be 1.5 : 1
Nuclear Decay
stabilization of an atom → particles & electromagnetic waves released during nuclear decay
OG atom → alpha/beta/gamma particle + daughter atom
Alpha Decay
a helium nucleus is the particle released
poor penetration; can be stopped by paper

Beta Decay
an electron/negatron released (a neutron emits a negatron and then becomes a proton)
moderate penetration; can be stopped by aluminum

Gamma Decay
a gamma photon released (no particles of matter leaves the nucleus; only energy)
strong, dangerous penetrating ability → can only be stopped by lead or concrete
can be released with other forms of decay

Radioisotope
an unstable, radioactive atom that decays over time to become more stable
Half-life
the amount of time that it takes for half of a radioisotope sample to decay