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Chapter 11 Intermolecular Forces, Liquids and Solids

CHEMISTRY The Central Science 9th Edition. Chapter 11 Intermolecular Forces, Liquids and Solids. David P. White. A Molecular Comparison of Liquids and Solids. Physical properties of substances understood in terms of kinetic molecular theory:

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Chapter 11 Intermolecular Forces, Liquids and Solids

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  1. CHEMISTRYThe Central Science 9th Edition Chapter 11Intermolecular Forces, Liquids and Solids David P. White Chapter 11

  2. A Molecular Comparison of Liquids and Solids • Physical properties of substances understood in terms of kinetic molecular theory: • Gases are highly compressible, assumes shape and volume of container: • Gas molecules are far apart and do not interact much with each other. • Liquids are almost incompressible, assume the shape but not the volume of container: • Liquids molecules are held closer together than gas molecules, but not so rigidly that the molecules cannot slide past each other. Chapter 11

  3. A Molecular Comparison of Liquids and Solids • Solids are incompressible and have a definite shape and volume: • Solid molecules are packed closely together. The molecules are so rigidly packed that they cannot easily slide past each other. Chapter 11

  4. A Molecular Comparison of Liquids and Solids Chapter 11

  5. A Molecular Comparison of Liquids and Solids Chapter 11

  6. A Molecular Comparison of Liquids and Solids • Converting a gas into a liquid or solid requires the molecules to get closer to each other: • cool or compress. • Converting a solid into a liquid or gas requires the molecules to move further apart: • heat or reduce pressure. • The forces holding solids and liquids together are called intermolecular forces. Chapter 11

  7. Intermolecular Forces • The covalent bond holding a molecule together is an intramolecular forces. • The attraction between molecules is an intermolecular force. • Intermolecular forces are much weaker than intramolecular forces (e.g. 16 kJ/mol vs. 431 kJ/mol for HCl). • When a substance melts or boils the intermolecular forces are broken (not the covalent bonds). Chapter 11

  8. Intermolecular Forces Chapter 11

  9. Intermolecular Forces • Ion-Dipole Forces • Interaction between an ion and a dipole (e.g. water). • Strongest of all intermolecular forces. Chapter 11

  10. Intermolecular Forces • Dipole-Dipole Forces • Dipole-dipole forces exist between neutral polar molecules. • Polar molecules need to be close together. • Weaker than ion-dipole forces. • There is a mix of attractive and repulsive dipole-dipole forces as the molecules tumble. • If two molecules have about the same mass and size, then dipole-dipole forces increase with increasing polarity. Chapter 11

  11. Intermolecular Forces Dipole-Dipole Forces

  12. Intermolecular Forces Dipole-Dipole Forces Chapter 11

  13. Intermolecular Forces • London Dispersion Forces • Weakest of all intermolecular forces. • It is possible for two adjacent neutral molecules to affect each other. • The nucleus of one molecule (or atom) attracts the electrons of the adjacent molecule (or atom). • For an instant, the electron clouds become distorted. • In that instant a dipole is formed (called an instantaneous dipole). Chapter 11

  14. Intermolecular Forces • London Dispersion Forces • One instantaneous dipole can induce another instantaneous dipole in an adjacent molecule (or atom). • The forces between instantaneous dipoles are called London dispersion forces. Chapter 11

  15. Intermolecular Forces • London Dispersion Forces • Polarizability is the ease with which an electron cloud can be deformed. • The larger the molecule (the greater the number of electrons) the more polarizable. • London dispersion forces increase as molecular weight increases. • London dispersion forces exist between all molecules. • London dispersion forces depend on the shape of the molecule. Chapter 11

  16. Intermolecular Forces • London Dispersion Forces • The greater the surface area available for contact, the greater the dispersion forces. • London dispersion forces between spherical molecules are lower than between sausage-like molecules. Chapter 11

  17. Intermolecular Forces London Dispersion Forces

  18. Intermolecular Forces London Dispersion Forces Chapter 11

  19. Intermolecular Forces • Hydrogen Bonding • Special case of dipole-dipole forces. • By experiments: boiling points of compounds with H-F, H-O, and H-N bonds are abnormally high. • Intermolecular forces are abnormally strong. Chapter 11

  20. Intermolecular Forces • Hydrogen Bonding • H-bonding requires H bonded to an electronegative element (most important for compounds of F, O, and N). • Electrons in the H-X (X = electronegative element) lie much closer to X than H. • H has only one electron, so in the H-X bond, the + H presents an almost bare proton to the - X. • Therefore, H-bonds are strong. Chapter 11

  21. Hydrogen Bonding

  22. Hydrogen Bonding

  23. Intermolecular Forces • Hydrogen Bonding • Hydrogen bonds are responsible for: • Ice Floating • Solids are usually more closely packed than liquids; • Therefore, solids are more dense than liquids. • Ice is ordered with an open structure to optimize H-bonding. • Therefore, ice is less dense than water. • In water the H-O bond length is 1.0 Å. • The O…H hydrogen bond length is 1.8 Å. • Ice has waters arranged in an open, regular hexagon. • Each + H points towards a lone pair on O. Chapter 11

  24. Intermolecular Forces Hydrogen Bonding

  25. Intermolecular Forces

  26. Some Properties of Liquids • Viscosity • Viscosity is the resistance of a liquid to flow. • A liquid flows by sliding molecules over each other. • The stronger the intermolecular forces, the higher the viscosity. • Surface Tension • Bulk molecules (those in the liquid) are equally attracted to their neighbors. Chapter 11

  27. Some Properties of Liquids Viscosity Chapter 11

  28. Surface Tension

  29. Some Properties of Liquids • Surface Tension • Surface molecules are only attracted inwards towards the bulk molecules. • Therefore, surface molecules are packed more closely than bulk molecules. • Surface tension is the amount of energy required to increase the surface area of a liquid. • Cohesive forcesbind molecules to each other. • Adhesive forcesbind molecules to a surface. Chapter 11

  30. Some Properties of Liquids • Surface Tension • Meniscusis the shape of the liquid surface. • If adhesive forces are greater than cohesive forces, the liquid surface is attracted to its container more than the bulk molecules. Therefore, the meniscus is U-shaped (e.g. water in glass). • If cohesive forces are greater than adhesive forces, the meniscus is curved downwards. • Capillary Action: When a narrow glass tube is placed in water, the meniscus pulls the water up the tube. Chapter 11

  31. Phase Changes • Surface molecules are only attracted inwards towards the bulk molecules. • Sublimation: solid  gas. • Vaporization: liquid  gas. • Melting or fusion: solid  liquid. • Deposition: gas  solid. • Condensation: gas  liquid. • Freezing: liquid  solid. Chapter 11

  32. Phase Changes

  33. Phase Changes • Energy Changes Accompanying Phase Changes • Sublimation: Hsub > 0 (endothermic). • Vaporization: Hvap > 0 (endothermic). • Melting or Fusion: Hfus > 0 (endothermic). • Deposition: Hdep < 0 (exothermic). • Condensation: Hcon < 0 (exothermic). • Freezing: Hfre < 0 (exothermic). Chapter 11

  34. Phase Changes • Energy Changes Accompanying Phase Changes • Generally heat of fusion (enthalpy of fusion) is less than heat of vaporization: • it takes more energy to completely separate molecules, than partially separate them. Chapter 11

  35. Phase Changes

  36. Phase Changes • Energy Changes Accompanying Phase Changes • All phase changes are possible under the right conditions. • The sequence • heat solid  melt  heat liquid  boil  heat gas • is endothermic. • The sequence • cool gas  condense  cool liquid  freeze  cool solid • is exothermic. Chapter 11

  37. Phase Changes • Heating Curves • Plot of temperature change versus heat added is a heating curve. • During a phase change, adding heat causes no temperature change. • These points are used to calculate Hfus and Hvap. • Supercooling: When a liquid is cooled below its melting point and it still remains a liquid. • Achieved by keeping the temperature low and increasing kinetic energy to break intermolecular forces. Chapter 11

  38. Chapter 11

  39. Phase Changes • Critical Temperature and Pressure • Gases liquefied by increasing pressure at some temperature. • Critical temperature: the minimum temperature for liquefaction of a gas using pressure. • Critical pressure: pressure required for liquefaction. Chapter 11

  40. Phase Changes Critical Temperature and Pressure Chapter 11

  41. Vapor Pressure • Explaining Vapor Pressure on the Molecular Level • Some of the molecules on the surface of a liquid have enough energy to escape the attraction of the bulk liquid. • These molecules move into the gas phase. • As the number of molecules in the gas phase increases, some of the gas phase molecules strike the surface and return to the liquid. • After some time the pressure of the gas will be constant at the vapor pressure. Chapter 11

  42. Vapor Pressure • Explaining Vapor Pressure on the Molecular Level Chapter 11

  43. Vapor Pressure • Explaining Vapor Pressure on the Molecular Level • Dynamic Equilibrium: the point when as many molecules escape the surface as strike the surface. • Vapor pressure is the pressure exerted when the liquid and vapor are in dynamic equilibrium. • Volatility, Vapor Pressure, and Temperature • If equilibrium is never established then the liquid evaporates. • Volatile substances evaporate rapidly. Chapter 11

  44. Vapor Pressure • Volatility, Vapor Pressure, and Temperature • The higher the temperature, the higher the average kinetic energy, the faster the liquid evaporates. Chapter 11

  45. Vapor Pressure • Volatility, Vapor Pressure, and Temperature

  46. Vapor Pressure • Vapor Pressure and Boiling Point • Liquids boil when the external pressure equals the vapor pressure. • Temperature of boiling point increases as pressure increases. Chapter 11

  47. Vapor Pressure • Vapor Pressure and Boiling Point • Two ways to get a liquid to boil: increase temperature or decrease pressure. • Pressure cookers operate at high pressure. At high pressure the boiling point of water is higher than at 1 atm. Therefore, there is a higher temperature at which the food is cooked, reducing the cooking time required. • Normal boiling point is the boiling point at 760 mmHg (1 atm). Chapter 11

  48. Phase Diagrams • Phase diagram: plot of pressure vs. Temperature summarizing all equilibria between phases. • Given a temperature and pressure, phase diagrams tell us which phase will exist. • Any temperature and pressure combination not on a curve represents a single phase. Chapter 11

  49. Phase Diagrams • Features of a phase diagram: • Triple point: temperature and pressure at which all three phases are in equilibrium. • Vapor-pressure curve: generally as pressure increases, temperature increases. • Critical point: critical temperature and pressure for the gas. • Melting point curve: as pressure increases, the solid phase is favored if the solid is more dense than the liquid. • Normal melting point: melting point at 1 atm. Chapter 11

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