Chemistry Review Part 5: Phases of Matter and Kinetic Molecular Theory Intermolecular Forces Kinetic Molecular Theory Molar Heats of Fusion and Vaporization.

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Presentation transcript:

Chemistry Review Part 5: Phases of Matter and Kinetic Molecular Theory Intermolecular Forces Kinetic Molecular Theory Molar Heats of Fusion and Vaporization Specific Heat Capacity Calculations Colligative Properties You will need a calculator and periodic table to complete this section.

Chemistry Review— Phases of Matter Intermolecular Forces COVALENT BOND POLARITY non-polar covalent bonds: bonding electrons shared equally between two atoms Example: H 2 polar covalent bonds (polar bonds): bonding electrons shared unequally. –Example: HCl BOND POLARITY BASED ON ATOMS’ ELECTRONEGATIVITY the more electronegative atom acquires a slight negative charge (δ-). the less electronegative atom acquires a slight positive charge(δ+ ). The unequal sharing creates “polarized” bonds with opposite charges. Two ways to show polarity in structural formulas. δ - and δ+ or a slashed arrow pointing toward electronegative element δ+δ+ δ-δ-

Chemistry Review— Phases of Matter Intermolecular Forces POLAR MOLECULES Polar Molecules: One end of the molecule is slightly negative, and one end is slightly positive. Nonpolar polar Symmetric molecules are usually nonpolar. The polarities all cancel out. The CO 2 molecule is nonpolar. When the arrows do not cancel the molecule is polar as in water. Unsymmetrical molecules are polar if there are polar bonds in the structure.

Chemistry Review— Phases of Matter Intermolecular Forces Intermolecular Attractions and Molecular Properties As intermolecular forces increase, the molecules are held more strongly together. Solids resist melting because melting requires breaking intermolecular attractions and reforming new ones as the molecules slide past each other. Liquids resist boiling because the liquid molecules will have to overcome the intermolecular attraction of the other liquid molecules to enter the gas phase.

Chemistry Review— Phases of Matter Kinetic Molecular Theory Kinetic Molecular Theory: 1.The tiny particles in all forms of matter are in constant motion. 2.As kinetic energy increases, temperature increases. 3.Kinetic Energy is directly proportional to the Kelvin temperature scale. 4.At zero Kelvin, K, all molecular motion theoretically stops. 0°C = 273K

Chemistry Review— Phases of Matter Kinetic Molecular Theory LIQUIDS When gas molecules lose kinetic energy (cool and slow down) then intermolecular forces can cause the molecules to stick together and liquify. Evaporation: molecules with enough kinetic energy to overcome the intermolecular attractions in a liquid can escape the liquid and enter the gas phase. Vapor Pressure: the force due to the gas above a liquid. This increases as temperature increases. The curves are different for each liquid due to intermolecular forces

Chemistry Review— Phases of Matter Kinetic Molecular Theory LIQUIDS Boiling Point: the temperature where a liquid’s vapor pressure equals the external pressure or atmospheric pressure. Boiling Point increases as external/atmospheric pressure increases. Boiling Point decreases as external/atmospheric pressure decreases.

Chemistry Review— Phases of Matter Kinetic Molecular Theory LIQUIDS

Chemistry Review— Phases of Matter Kinetic Molecular Theory SOLIDS 1.Particles in liquids are free to slide past each other 2.Particles in solids do not slide past each other, but vibrate in place. 3.Melting point: temperature where a solid becomes a liquid.

Chemistry Review— Phases of Matter Kinetic Molecular Theory PHASE CHANGES OR CHANGES OF STATE a to b: solid increases in temperature. b to c: solid melts to liquid at a constant temperature c to d: liquid increases in temperature d to e: liquid vaporizes to gas at a constant temperature e to f: gas increases in temperature

Chemistry Review— Phases of Matter Molar Heats of Fusion and Vaporization Molar heat of fusion: the energy required to melt one mole of a substance. (ΔH fusion ) Molar heat of vaporization: the energy required to vaporize one mole of a substance. (ΔH vaporization ) ΔH fusion ΔH vaporization

Chemistry Review--Molar Relationships References for New York Regent’s exam powerpoint.