Atomic Theory, Structure, and Mass Relationships Notes

Philosophical Atomic Theory in Antiquity

  • Leucippus (5th century BC): Traditionally credited as the founder of atomism. He proposed that atoms exist in constant motion within a deterministic world, where everything results from the collisions of atoms.

  • Democritus (460-371 BC): Developed the philosophical basis for atomism.

    • All matter is composed of atoms, which are bits of matter too small to be seen.

    • Atoms are indivisible and completely solid.

    • Atoms are homogeneous and lack any internal structure.

    • The "void" is the empty space existing between atoms.

    • Atoms differ in their sizes, shapes, and weights.

  • This theory was largely ignored and forgotten for more than 2,000 years.

The Scientific Revolution and Atomic Structure

  • Robert Boyle (1627-1691):

    • Performed detailed experiments with gases.

    • Provided physical evidence for the atomic makeup of matter.

    • Defined an "element" as a substance that cannot be chemically broken down further.

    • Proposed that atoms of different elements join together in various ways to yield chemical compounds.

  • Joseph Priestley (1733-1804):

    • Prepared and isolated oxygen gas (O2O_2).

    • Reaction: 2HgO2Hg+O22HgO \rightarrow 2Hg + O_2.

  • Antoine Lavoisier (1743-1794):

    • Demonstrated the role of oxygen in combustion.

    • Observed that in a closed container, the mass of the products exactly equals the mass of the starting reactants.

    • Conclusion: Mass is neither created nor destroyed.

    • Established the Law of Mass Conservation.

Fundamental Laws of Chemistry

  • Law of Conservation of Mass:

    • Example: Mixing Potassium Iodide (KIKI) and Mercury(II) Nitrate (Hg(NO3)2Hg(NO_3)_2).

    • Equation: Hg(NO3)2(aq)+2KI(aq)HgI2(s)+2KNO3(aq)Hg(NO_3)_2(aq) + 2KI(aq) \rightarrow HgI_2(s) + 2KNO_3(aq).

    • Quantitative Proof: 3.25g+3.32g=6.57g3.25\,g + 3.32\,g = 6.57\,g (reactants) yields 4.55g+2.02g=6.57g4.55\,g + 2.02\,g = 6.57\,g (products).

  • Law of Definite Proportions (Law of Constant Composition):

    • Proposed by Joseph Proust (1754-1826).

    • A given chemical compound contains its constituent elements in a fixed mass ratio regardless of the source or method of preparation.

    • A substance is defined by the specific proportions of its elements, not just the types.

    • Example: By mass, water (H2OH_2O) is always 8/98/9 oxygen and 1/91/9 hydrogen.

  • Law of Multiple Proportions:

    • In compounds containing two particular elements (A and B), the amount of element A per measure of element B is a simple integer number.

    • Example: Nitrous oxide contains 7g7\,g of nitrogen per 8g8\,g of oxygen; nitrogen dioxide contains 7g7\,g of nitrogen per 16g16\,g of oxygen.

Dalton’s Atomic Theory (1803)

  • John Dalton (1766–1844):

    • Solid Sphere Model: Imagined atoms as tiny, solid spheres resembling billiard balls.

    • Atoms of the same element are identical in mass and properties.

    • Atoms cannot be created, divided, or destroyed.

    • Compounds form when atoms of different elements combine in fixed ratios.

    • Chemical reactions involve rearranging how atoms are combined; the atoms themselves do not change.

  • A Quantitative Theory:

    • The cardinal point of Dalton's theory was its quantitative nature.

    • He used measured mass ratios of elements in compounds and assumed molecular structures to convert mass ratios into relative atomic weights.

    • He asserted that atoms of different elements have different weights, which are proportions by weight in which elements combine (or simple multiples/sub-multiples).

  • Impact of Dalton's Model:

    • Linked atoms to quantitative laws and scientific models based on experimental evidence.

    • Atomic weights became essential for explanations.

    • Laid the groundwork for modern chemistry; atoms became central explanatory entities rather than just metaphors.

The 19th-Century Debate on Atomism

  • Resistance to Atoms:

    • Much of 19th-century chemistry functioned perfectly well without asserting the reality of atoms; stoichiometry could be done by mass and laws established empirically.

    • Atoms were unobservable, leading many chemists (like Ernst Mach and Wilhelm Ostwald) to treat them as "useful fictions."

    • Chief stumbling blocks included Dalton's arbitrary assumptions about compound formulae and the high number of different atoms required by the theory.

    • Thermodynamics and energetics were highly successful without requiring atomic theory.

  • Collapse of Anti-Atomism (1900–1915):

    1. Brownian Motion: Albert Einstein (1905) and Jean Perrin (1908–1913) provided quantitative predictions tied to atomic size and number. Perrin experimentally measured Avogadro’s number.

    2. Electron Discovery: J.J. Thomson (1897) proved atoms had internal structure.

    3. X-ray Crystallography: Bragg (1912–1913) directly revealed atomic spacing in solids.

Discovery of the Electron and Cathode Rays

  • Cathode Ray Tube Experiments:

    • A high voltage across electrodes in a hollow vessel causes negative particles to move from the cathode to the anode.

    • Julius Plücker (1801-1868): Observed rays are moved by magnets, implying they are electrically charged.

    • Eugen Goldstein (1850-1930): Observed rays cast shadows; coined the name "cathode ray."

    • William Crooks (1832–1919): Observed rays could rotate a wheel, proving they are particulate and negatively charged.

  • Properties of Cathode Rays/Electrons:

    • Deflect parallel to an electrostatic field (toward the positive plate) and perpendicular to a magnetic field.

    • Deflection degree depends on magnetic/electric field strength, magnitude of negative charge, and mass of the electron.

  • J.J. Thomson (1856-1940):

    • By balancing opposing magnetic and electric forces, he determined the charge-to-mass ratio (e/me/m) of an electron.

    • Determined that electrons are a part of all matter.

Millikan’s Oil Drop Experiment

  • Robert A. Millikan (1868-1953):

    • Experiment: Oil droplets were sprayed into a chamber and allowed to reach terminal velocity to calculate mass. X-rays gave droplets a negative charge. Droplets were then suspended between charged plates.

    • Results: The charge on any droplet was always a whole-number multiple of 1.60×1019C1.60 \times 10^{-19}\,C.

    • Calculations: Using the charge-to-mass ratio (1.76×108C/g1.76 \times 10^8\,C/g), the mass of an electron was calculated.

    • Accepted Mass of Electron: 9.10939×1028g9.10939 \times 10^{-28}\,g.

Evolution of Atomic Models

  • Thomson’s Plum Pudding Model (1904):

    • The atom is a continuously distributed positive particle with point-like negative electrons inside.

    • The model was dynamic: electrons arranged in concentric rings rotating inside a uniform sphere of positive charge for stability.

    • Implied shell structure and attempted to relate structures to chemical periodicity.

  • Radioactivity:

    • Henri Becquerel (1896): Discovered radiation from uranium salts.

    • Marie Curie (1867-1934): Coined the term "radioactivity"; discovered polonium and radium.

    • Alpha (α\alpha) Particle: A helium nucleus consisting of 22 protons and 22 neutrons.

  • Rutherford’s Gold Foil Experiment (1906/1911):

    • Ernest Rutherford and Hans Geiger fired α\alpha particles at thin gold foils.

    • Observations: Most particles passed through unimpeded; some deflected; 1 in 10,000 deflected by nearly 180180^{\circ}.

    • Conclusion: The atom contains a positively charged nucleus concentrated in a very small space. This nucleus is much heavier than the α\alpha particle.

  • Rutherford’s Nuclear Model:

    • Determined that the number of positive charges equals the element's atomic number.

    • Problem: Classical electrodynamics suggested orbiting electrons should radiate energy and collapse into the nucleus (later resolved by Niels Bohr).

Discovery of Protons and Neutrons

  • The Proton (p+p^+):

    • Discovered by Rutherford in 1917 via artificial disintegration of the atomic nucleus.

    • Irradiated nitrogen gas with α\alpha particles; observed hydrogen nuclei being ejected from nitrogen atoms.

    • Named the particle the "proton" in 1920.

  • The Neutron (n0n^0):

    • Discovered by James Chadwick (1932).

    • Followed research by Irene Joliot-Curie and Frederick Joliot, who found a penetrating radiation when light elements were bombarded with α\alpha particles.

    • Chadwick proved this radiation consisted of neutral particles with approximately the same mass as a proton.

Nuclear Arithmetic and Isotopes

  • Subatomic Particle Comparison:

    • Proton: Charge +1+1 (1.602×1019C1.602 \times 10^{-19}\,C); Mass 1.007amu\approx 1.007\,amu.

    • Neutron: Charge 00; Mass 1.008amu\approx 1.008\,amu.

    • Electron: Charge 1-1 (1.602×1019C-1.602 \times 10^{-19}\,C); Mass 0.0005amu\approx 0.0005\,amu.

    • Nucleons: Collective term for protons and neutrons.

  • Atomic Number (ZZ): Number of protons; defines the element and its periodic table position. In neutral atoms, Z=number of electronsZ = \text{number of electrons}.

  • Mass Number (AA): Total number of nucleons (Z+NZ + N). Symbol AA comes from German Atomgewichtzahl.

  • Isotopes: atoms with identical ZZ but different AA (different number of neutrons).

    • Notation: ZAE{^A_Z}E (Example: Uranium-235 is 92235U{^{235}_{92}}U).

    • Stability:

      • For light elements (Z20Z \le 20): NZN \approx Z and A2ZA \approx 2Z.

      • For heavier elements (Z > 20): Stability requires N > Z to counteract proton-proton repulsion. The N/ZN/Z ratio reaches 1.5\approx 1.5 for heavy elements (e.g., Lead-208 has N/Z1.54N/Z \approx 1.54).

Atomic Mass and Atomic Weight

  • Atomic Mass: The mass of a single atom measured in atomic mass units (amuamu) or Daltons (DaDa).

    • Standard: One atom of 12C{^{12}C} is exactly 12amu12\,amu.

    • Mass Defect: The actual atomic mass is less than the sum of its individual nucleons due to energy released during nuclear formation (E=mc2E=mc^2).

    • Mass of atom in amuamu \approx atom's mass number (AA).

  • Atomic Weight (Relative Atomic Mass): A weighted average of the atomic masses of an element's naturally occurring isotopes.

    • Formula: Atomic weight=(isotopic mass×fractional abundance)\text{Atomic weight} = \sum(\text{isotopic mass} \times \text{fractional abundance}).

    • It is a dimensionless number.

    • Example for Carbon: (12amu)(0.9889)+(13.0034amu)(0.0111)=12.01amu(12\,amu)(0.9889) + (13.0034\,amu)(0.0111) = 12.01\,amu.

The Mole and Molar Mass

  • The Mole (mol): The SI unit for amount of substance.

    • Historical Definition: Amount of substance containing as many entities as there are atoms in 12g12\,g of 12C{^{12}C}.

    • 2019 Revised Definition: Exactly 6.02214076×10236.02214076 \times 10^{23} specified entities (Avogadro's number, NAN_A).

  • Molar Mass (MM): The mass of one mole of a substance, expressed in g/molg/mol.

    • Numerically equivalent to an element's atomic weight.

  • Calculations:

    • Moles (n)=Mass (m)Molar Mass (M)\text{Moles (n)} = \frac{\text{Mass (m)}}{\text{Molar Mass (M)}}

    • Moles (n)=Volume (v)Molar Volume (V)\text{Moles (n)} = \frac{\text{Volume (v)}}{\text{Molar Volume (V)}}

    • Number of Particles=n×6.022×1023\text{Number of Particles} = n \times 6.022 \times 10^{23}

Worked Examples

  • Interpreting Uranium-235 (92235U{^{235}_{92}}U):

    • Protons: 9292

    • Electrons: 9292

    • Neutrons: 23592=143235 - 92 = 143

  • Calculating Atomic Weight of Chlorine:

    • Isotope 1: 35Cl{^{35}Cl} (34.969amu34.969\,amu, 75.76%75.76\%

    • Isotope 2: 37Cl{^{37}Cl} (36.966amu36.966\,amu, 24.24%24.24\%

    • Calculation: (34.969×0.7576)+(36.966×0.2424)=35.45amu(34.969 \times 0.7576) + (36.966 \times 0.2424) = 35.45\,amu.

  • Mass to Moles/Atoms for Silicon (10.53g10.53\,g, Atomic Mass 28.0855amu28.0855\,amu):

    • Moles: 10.53gSi×1mol28.0855g=0.3749molSi10.53\,g\,Si \times \frac{1\,mol}{28.0855\,g} = 0.3749\,mol\,Si

    • Atoms: 0.3749mol×(6.022×1023)=2.258×1023atomsSi0.3749\,mol \times (6.022 \times 10^{23}) = 2.258 \times 10^{23}\,atoms\,Si