States of Matter, Phase Changes, and Atomic Structure

States of Matter Properties

StateShape & VolumeParticle ArrangementParticle MotionAttractive Forces
Solid (s)Fixed shape and volumeRegular, closely packed latticeVibrate about fixed positionsVery strong
Liquid (l)Fixed volume, fits containerIrregular, closely touchingSlide past each otherModerate
Gas (g)Fills container entirelyRandom, far apartRapid, random motionNegligible or weak

Phase Changes and Transitions

  • Melting: Solid to Liquid (thermal energy overcomes strong forces holding particles in fixed positions).
  • Freezing: Liquid to Solid (removal of thermal energy allows particles to form bonds in fixed positions).
  • Boiling: Liquid to Gas (occurs throughout the liquid at a specific boiling point; attractive forces completely break).
  • Evaporating: Liquid to Gas (occurs only at the liquid’s surface below boiling point as high-energy particles escape).
  • Condensing: Gas to Liquid (gas cools, particles lose kinetic energy and move closer together).

Heating Curves and Energy

A standard heating curve contains sloped regions and flat plateaus:

  • Sloped Sections (Single State: P = Solid, R = Liquid):
    • Heat energy increases the kinetic energy of the particles.
    • Temperature increases as particle vibration or motion speeds up.
  • Flat Plateaus (Phase Changes: Q = Melting, S = Boiling):
    • Temperature remains constant.
    • Thermal energy is used to overcome intermolecular attractive forces rather than increasing particle kinetic energy.

Gas Behavior: Temperature and Pressure

  • Effect of Temperature: Increasing temperature increases the average kinetic energy and speed of gas particles, causing the gas to expand (volume increases at constant pressure).
  • Effect of Pressure: Increasing pressure forces gas particles closer together, decreasing gas volume.

Diffusion and Molecular Mass

Diffusion is the random mixing and net movement of particles from an area of higher concentration to an area of lower concentration.

  • Liquids vs. Gases: Diffusion occurs much faster in gases than in liquids because gas particles have higher energy and move freely through large empty spaces.
  • Temperature Effect: Higher temperatures increase kinetic energy, leading to faster movement and a higher rate of diffusion.
  • Relative Molecular Mass (Mr):
    • Lighter gas molecules (lower Mr) diffuse faster.
    • Heavier gas molecules (higher Mr) diffuse slower.

Advanced States of Matter

  • Liquid Crystals: Exhibit properties between conventional liquids and solid crystals; particles flow like a liquid while maintaining an oriented pattern.
  • Superfluids: Formed at near absolute zero temperatures (e.g., liquid helium); display zero viscosity and infinite fluidity.
  • Plasma (The Fourth State of Matter): Ionized gases existing at very high temperatures (e.g., in lightning, stars) that conduct electricity.

Atomic Composition of Common Elements

  • He (Helium): 2e, 2p, 2n
  • Li (Lithium): 3e, 3p, 4n
  • Be (Beryllium): 4e, 4p, 5n
  • B (Boron): 5e, 5p, 6n
  • C (Carbon): 6e, 6p, 6n
  • N (Nitrogen): 7e, 7p, 7n
  • O (Oxygen): 8e, 8p, 8n
  • F (Fluorine): 9e, 9p, 10n
  • Ne (Neon): 10e, 10p, 10n
  • Na (Sodium): 11e, 11p, 12n
  • Mg (Magnesium): 12e, 12p, 12n
  • Al (Aluminum): 13e, 13p, 14n
  • Si (Silicon): 14e, 14p, 14n
  • P (Phosphorus): 15e, 15p, 16n
  • S (Sulfur): 16e, 16p, 16n
  • Cl (Chlorine): 17e, 17p, 18n
  • Ar (Argon): 18e, 18p, 22n
  • K (Potassium): 19e, 19p, 20n
  • Ca (Calcium): 20e, 20p, 20n

Isotopes: Definition and Properties

  • Isotopes are atoms of the same element that have the same number of protons (same atomic number) but a different number of neutrons (different mass or nucleon number).
  • Same Chemical Properties: They have identical electronic configurations and valence electrons, meaning they react chemically in the exact same way.
  • Different Physical Properties: They vary slightly in mass, density, and melting or boiling points due to differences in mass number.

Subatomic Particle Summary

ParticleRelative MassRelative ChargeLocation
Proton (p)1+1Nucleus
Neutron (n)10Nucleus
Electron (e–)1/2000-1Shells / Orbitals
  • Atomic Number: Number of protons.
  • Mass Number: Protons + Neutrons.
  • Neutron Count: Number of Neutrons = Mass Number (A) – Atomic Number (Z).

Relative Atomic Mass Formula:

Ar = [(Mass of Isotope 1 × Abundance %) + (Mass of Isotope 2 × Abundance %)] / 100