Liquids and Solids | General Chemistry 2
Intermolecular Forces
Intramolecular vs. intermolecular forces:
- Intramolecular forces: Forces within a molecule, such as covalent, ionic, and metallic bonds.
- Intermolecular forces: Forces between molecules, responsible for the physical properties of substances.
Types of intermolecular forces:
- Ion-dipole forces (40-600 kJ.mol-1)
- Hydrogen bonding (10-40 kJ.mol-1)
- Dipole-dipole interactions (5-25 kJ.mol-1)
- Ion-induced dipole forces (3-15 kJ.mol-1)
- Dipole-induced dipole forces (2-10 kJ.mol-1)
- London dispersion forces (0.05-40 kJ.mol-1)
Hydrogen bonding:
Hydrogen bonding is a strong electrostatic interaction that occurs between a hydrogen atom bonded to highly electronegative atoms (like N, O, F) and an electronegative atom that has a lone pair of electrons. Hydrogen bonding is crucial for the properties of water and biological molecules like DNA.
Dipoles and induced dipoles:
- Dipoles: Molecules with a permanent molecular dipole due to an uneven distribution of electrons.
- Induced dipoles: Nonpolar molecules that develop a temporary dipole moment when in the presence of a charged or polar molecule.
An isolated O2 molecule is nonpolar.
However, when a polar water molecule approaches, the electron distribution in O2 is rearranged, creating an induced dipole.
London dispersion forces:
London dispersion forces are electrostatic interactions that occur between two nonpolar molecules.
Electrons within a molecule are constantly moving. At any given moment, they may be asymmetrically distributed, creating an instantaneous dipole moment. This temporary dipole can induce a dipole in a neighboring nonpolar molecule, leading to weak electrostatic interactions known as London dispersion forces.
Importance of intermolecular forces:
- Boiling and melting points: Substances with stronger intermolecular forces have higher boiling and melting points.
- Solubility: Polar solvents dissolve polar solutes, and nonpolar solvents dissolve nonpolar solutes, based on the principle "like dissolves like."
- Viscosity and surface tension: Stronger intermolecular forces result in higher viscosity and surface tension in liquids.
Properties of Liquids
Viscosity (η):
Viscosity is a measure of a liquid's resistance to flow. It is influenced by the internal friction between layers of molecules as they move past one another.
Factors affecting viscosity are:
- Intermolecular forces: Stronger intermolecular forces lead to higher viscosity because molecules are more strongly attracted to each other, making it harder for them to move past one another.
- Temperature: As temperature increases, viscosity decreases because the increased kinetic energy allows molecules to overcome intermolecular forces more easily.
- Molecular structure: Long, flexible molecules tend to have higher viscosities than shorter-chain or spherical molecules due to increased entanglement and intermolecular interactions.
Surface Tension (in J.m2):
Surface tension is the energy required to increase the surface area of a liquid. It results from the imbalance of intermolecular forces at the surface of a liquid, where molecules experience a net inward force.
Factors affecting surface tension are:
- Intermolecular forces: Liquids with stronger intermolecular forces have higher surface tension. For example, water has a high surface tension due to hydrogen bonding.
- Surfactants: Surfactants are substances that reduce surface tension by decreasing the intermolecular forces between adjacent molecules at the surface, allowing the liquid to spread more easily.
Capillary Action:
Capillary action is the ability of a liquid to flow in narrow spaces without the assistance of external forces, such as gravity. This phenomenon is a result of the adhesive forces between the liquid and the surface of the capillary, as well as the cohesive forces within the liquid.
Density and compressibility:
- Density: Liquids have a higher density than gases because their molecules are more closely packed. The density of a liquid generally decreases slightly with increasing temperature as the liquid expands.
- Compressibility: Liquids are nearly incompressible, meaning that their volume does not change significantly under pressure due to the close packing of molecules.
Vapor Pressure
Vapor pressure:
Vapor pressure is the pressure exerted by the vapor in equilibrium with its liquid phase at a given temperature in a closed system. This pressure arises as molecules escape from the liquid surface into the vapor phase.
The pressure exerted by the vapor on the liquid increases until equilibrium is reached, where the rate of evaporation equals the rate of condensation. At this point, the vapor pressure remains constant and is referred to as the equilibrium vapor pressure.
Factors affecting vapor pressure:
- Temperature: Vapor pressure increases with temperature. As temperature rises, more molecules gain sufficient kinetic energy to overcome intermolecular forces and escape into the vapor phase, thus increasing the vapor pressure. This phenomenon can be quantitatively described by the Clausius-Clapeyron equation:
ln Pvap = - + C
Pvap = vapor pressure (in atm or Pa)
ΔHvap = enthalpy of vaporization (in J.mol-1)
R = gas constant (8.314 J.mol-1.K-1)
T = temperature (in K)
C = constant characteristic of the specific substance
The Clausius-Clapeyron equation can also be written as:
ln = -
P1 = vapor pressure at T1 (in atm or Pa)
P2 = vapor pressure at T2 (in atm or Pa)
ΔHvap = enthalpy of vaporization (in J.mol-1)
R = gas constant (8.314 J.mol-1.K-1)
T1 and T2 = absolute temperatures (in K)
- Intermolecular forces: Substances with stronger intermolecular forces have lower vapor pressures at a given temperature because more energy is required for molecules to escape into the vapor phase.
- Vapor pressure of water: 4.58 mmHg at 273 K versus 17.5 mmHg at 293 K
- Vapor pressure of Et2O (weak dipole-dipole interactions and dispersion forces): 440 mmHg at 273K
Vapor pressure of water (strong hydrogen bonds): 4.58 mmHg at 273K
Boiling point and vapor pressure:
- The boiling point of a liquid is the temperature at which its vapor pressure equals the external atmospheric pressure. At this point, bubbles of vapor form within the liquid, leading to boiling.
- Normal boiling point: The temperature at which the vapor pressure of a liquid equals 1 atmosphere (760 mmHg).
Volatility:
A substance with a high vapor pressure at normal temperatures is considered volatile. These substances evaporate quickly and are often associated with strong odors or quick evaporation, like ethanol or acetone.
Phase Changes
Types of phase changes:
Endothermic phase transitions (processes that absorb heat from the surroundings):
- Melting (fusion): Transition from solid to liquid (ΔHfus)
- Vaporisation: Transition from liquid to gas (ΔHvap)
- Sublimation: Transition from solid to gas without passing through the liquid phase (ΔHsub = ΔHfus + ΔHvap according to Hess’s law).
Exothermic phase transitions (processes that release heat to the surroundings):
- Freezing: Transition from liquid to solid (-ΔHfus)
- Condensation: Transition from gas to liquid (-ΔHvap)
- Deposition: Transition from gas to solid without passing through the liquid phase (-ΔHsub)
Heating curves:
A heating curve illustrates how the temperature of a substance changes as heat is added at a constant rate. Different segments of the curve represent different phases and phase transitions.
- Segment A (solid phase): The substance is in the solid phase. As heat is added, the temperature increases according to:
q = n CP ΔT
q = heat added (in J)
n = number of moles (in mol)
CP = molar heat capacity of the solid at constant pressure (in J.K-1.mol-1)
- Segment B (melting): The substance undergoes a phase transition from solid to liquid. During this process, the temperature remains constant as the substance absorbs heat:
q = n ΔHfus
q = heat added (in J)
n = number of moles (in mol)
ΔHfus = enthalpy change for fusion (in J.mol-1)
- Segment C (liquid phase): The substance is in the liquid phase. As heat is added, the temperature increases according to:
q = n CP' ΔT
q = heat added (in J)
n = number of moles (in mol)
CP' = molar heat capacity of the liquid (in J.K-1.mol-1) ≠ CP from segment A
- Segment D (vaporization): The substance undergoes a phase transition from liquid to gas. The temperature remains constant as the substance absorbs heat:
q = n ΔHvap
q = heat added (in J)
n = number of moles (in mol)
ΔHvap = enthalpy change for vaporisation (in J.mol-1)
- Segment E (gas phase): The substance is in the gas phase. As heat is added, the temperature increases according to:
q = nCP''ΔT
q = heat added (in J)
n = number of moles (in mol)
CP'' = molar heat capacity of the gas (in J.K-1.mol-1)
Phase Diagrams
Phase diagrams:
A phase diagram displays the regions of all phases (solid, liquid, gas) of a pure substance across different temperatures and pressures. It maps out the conditions under which each phase is stable and where transitions between phases occur.
Components of a phase diagram:
- Axes: pressure (y-axis) and temperature (x-axis).
- Regions: solid region, liquid region, and gas region.
- Phase boundaries: The lines that separate different regions on the diagram, representing the conditions (temperature and pressure) at which two phases coexist in equilibrium (solid-liquid, liquid-gas, and solid-gas).
Key points on a phase diagram:
- Triple point: The point on the phase diagram where all three phases coexist in equilibrium. Each substance has a unique triple point defined by a specific temperature and pressure.
- Critical point: The point on the phase diagram where the liquid and gas phases become indistinguishable from one another. Beyond this point, the substance exists as a supercritical fluid with properties of both liquids and gases.
Types of Crystals
Crystals:
Crystals are solids with an ordered, repeating arrangement of atoms, ions, or molecules. They can be classified based on the type of forces between their constituent particles, which determine their physical properties. The main types of crystals include ionic, molecular, network, metallic, and amorphous crystals.
Ionic crystals:
Ionic crystals are composed of cations and anions held together by coulombic (charge-charge) attractions, also known as ionic bonds.
Properties:
- Hard and brittle due to the strong electrostatic forces between ions.
- High melting points because a large amount of energy is required to break the ionic bonds.
- Poor electrical conductors in solid form but conduct electricity when molten or dissolved in water because the ions are free to move.
Sodium chloride (NaCl), Magnesium oxide (MgO).
Covalent (network) crystals:
Covalent crystals are composed of atoms connected by an extended network of covalent bonds, forming a continuous, three-dimensional structure.
Properties:
- Very hard and have high melting points because covalent bonds are strong and require significant energy to break.
- Typically non-conductive due to the lack of free electrons.
Diamond (carbon, C), Silicon dioxide (quartz, SiO2).
Metallic crystals:
Metallic crystals are composed of positive metal cations arranged in a lattice structure with a "sea" of delocalized electrons that move freely throughout the structure.
Properties:
- Good electrical and thermal conductivity due to the mobility of the free electrons.
- Malleable and ductile because metal ions can slide past each other without breaking the metallic bond.
- Lustrous appearance due to the reflection of light by free electrons.
- Variable melting points, typically high but lower than ionic or covalent crystals.
Silver (Ag), Copper (Cu), Iron (Fe), gold (Au).
Molecular crystals:
Molecular crystals are composed of molecules held together by weak van der Waals forces, dipole-dipole interactions, or hydrogen bonds.
Properties:
- Lower melting and boiling points due to the weak intermolecular forces.
- Generally soft and have low hardness.
- Non-conductive because they lack free-moving electrons or ions.
Iodine (I2), Ice (H2O), Carbon dioxide (dry ice, CO2).
X-Ray Crystallography
Principle of X-ray crystallography:
X-ray crystallography relies on the diffraction of X-rays by the orderly arrangement of atoms in a crystal. As X-rays pass through the crystal, they are scattered by the electrons around the atoms. The scattered X-rays interfere with each other, producing a diffraction pattern unique to the structure of the crystal.
Bragg's law:
The relationship between the wavelength of the X-rays, the angle at which they are diffracted, and the spacing between planes in the crystal lattice is described by Bragg's Law:
nλ = 2dsinΘ
n = small integer, usually 1
λ = wavelength of the X-rays (in m)
d = distance between the planes in the crystal lattice (in m)
Θ = angle of incidence (in degrees or radians)
Steps in X-ray crystallography:
- Crystal preparation: The crystal must be pure, well-ordered, and free of defects, as imperfections can distort the diffraction pattern.
- X-ray exposure: The crystal is exposed to a beam of X-rays. As the X-rays pass through the crystal, they are diffracted by the atomic planes within the crystal.
- Data collection: The diffraction pattern is recorded on a detector. The pattern consists of spots that correspond to the angles and intensities of the diffracted X-rays. The position and intensity of these spots provide information about the crystal structure.
- Data analysis: The diffraction data is analyzed using mathematical techniques, including Fourier transforms, to construct an electron density map. This map shows the distribution of electrons within the crystal, allowing scientists to determine the positions of the atoms.
- Structure determination: The electron density map is used to build a three-dimensional model of the crystal's atomic structure. This model reveals the arrangement of atoms, the types of chemical bonds, and the geometry of the molecule or solid.
Crystal Structure
Unit cell:
The unit cell is the smallest repeating unit in a crystal lattice that, when repeated in all directions, creates the entire crystal structure. It defines the crystal’s symmetry and dimensions.
Types of unit cells:
- Primitive (Simple): Atoms are located only at the corners of the unit cell.
- Body-centered: Atoms are located at the corners and one atom at the center of the unit cell.
- Face-centered: Atoms are located at the corners and at the centers of each face of the unit cell.
Crystal lattice:
A crystal lattice is a three-dimensional arrangement of points that represent the positions of atoms, ions, or molecules in a crystal. The unit cells stack together in space to form this lattice.
The lattice parameters include the lengths of the unit cell edges (a, b, c) and the angles between them (α, β, γ), which define the geometry of the lattice.
Packing efficiency:
Packing efficiency refers to the fraction of the volume of a unit cell that is occupied by the constituent particles (atoms, ions, or molecules). It indicates how tightly the particles are packed in the crystal.
Cubic packing: Simple cubic (52%), body-centered cubic (68%), face-centered cubic (74%).
Coordination number:
The coordination number of a particle in a crystal structure is the number of nearest neighbors that surround it. This number affects the stability and properties of the crystal.
- In a face-centered cubic (FCC) structure, the coordination number is 12.
- In a body-centered cubic (BCC) structure, the coordination number is 8.
Common Crystal Structures
Simple cubic (SC):
- Atoms at each corner of the cube
- Coordination Number: 6
- Stacking pattern: a-a-a-a-
- Lattice parameter: length of an edge = 2 x radii of the atom
Body-centered cubic (BCC):
- Atoms at each corner and one atom at the center of the cube
- Coordination Number: 8
- Stacking pattern: a-b-a-b-
- Lattice parameter: length of the main diagonal = 4 x crystallographic radii
Face-centered cubic (FCC):
- Atoms at each corner and at the centers of all the faces of the cube.
- Coordination Number: 12
- Stacking pattern: a-b-c-a-b-c-
- Lattice parameter: length of the diagonal of a face = 4 x crystallographic radii
Check your knowledge about this Chapter
Dipole-dipole interactions and London dispersion forces are two types of van der Waals forces, which are the weakest intermolecular forces.
- Dipole-dipole interactions occur between molecules that possess permanent dipoles, which means there is an uneven distribution of electron density within the molecule, resulting in regions of partial positive and negative charges. These permanent dipoles attract each other when the positive end of one molecule is near the negative end of another, giving rise to an electrostatic force of attraction.
- In contrast, London dispersion forces are present in all molecules, including nonpolar ones. They arise due to momentary fluctuations in electron distribution, which lead to the creation of instantaneous dipoles. Even in nonpolar molecules where the electron density is usually evenly distributed, electrons can momentarily concentrate in one area, inducing a temporary dipole that can then induce dipoles in adjacent molecules.
While London dispersion forces are generally weaker than dipole-dipole interactions, they become more significant in molecules with larger molar masses or more surface area, because of the increased likelihood of fluctuations in the electron density.
Hydrogen bonding is a specific type of intermolecular force that occurs when a hydrogen atom is covalently bonded to a highly electronegative atom, such as nitrogen, oxygen, or fluorine, and is also attracted to another electronegative atom in a nearby molecule. This results in a strong dipole-dipole attraction due to the significant difference in electronegativity between hydrogen and the electronegative atom.
In contrast, other types of intermolecular forces, such as London dispersion forces and dipole-dipole interactions, generally involve weaker attractions. London dispersion forces are the result of temporary dipoles induced in atoms or molecules, while dipole-dipole interactions occur between the permanent dipoles of polar molecules. Hydrogen bonds are typically stronger than these other types of intermolecular forces and have significant effects on the physical properties of compounds, such as higher boiling points and greater viscosity.
Liquids have a fixed volume but no fixed shape because of the intermolecular forces present between their molecules. These forces are strong enough to keep the molecules relatively close together, conferring a definite volume. However, the forces are not strong enough to hold the molecules in fixed positions, allowing them to move fluidly past one another, which means that a liquid will conform to the shape of its container.
Intermolecular forces have a direct impact on vapor pressure. Stronger intermolecular forces, such as hydrogen bonding or dipole-dipole interactions, tend to hold molecules in the liquid phase more tightly, resulting in a lower rate of evaporation and, consequently, a lower vapor pressure. Conversely, substances with weaker intermolecular forces, like those with primarily London dispersion forces, have molecules that can escape more easily into the gas phase, which leads to a higher vapor pressure.
During a phase change, such as melting or boiling, the kinetic energy of the molecules changes significantly. For melting, energy is absorbed, increasing molecular motion until the molecules have enough energy to overcome the attractive intermolecular forces that hold them in a fixed position in the solid, allowing them to move past each other as a liquid. During boiling, energy input continues to increase the kinetic energy of the molecules until they can overcome the intermolecular forces that keep them as a liquid, transitioning into the gaseous phase where the molecules are much further apart and move freely.
Phase diagrams are graphical representations of the physical states of a substance under different conditions of temperature and pressure. They delineate regions that correspond to the solid, liquid, and gas phases, as well as areas where phases coexist at equilibrium, such as along the lines dividing the regions. The triple point shows where all three phases are in equilibrium, while the critical point indicates the temperature and pressure above which the distinct liquid and gas phases no longer exist.
By analyzing a phase diagram, one can predict the phase of a substance at a specific temperature and pressure, understand the conditions under which phase transitions occur, and gather information related to the substance's melting, boiling, sublimation, and deposition conditions.
The critical point on a phase diagram represents the end of the line that demarcates the liquid and gas phases, known as the vapor-pressure curve. At this exact temperature and pressure, the properties of the liquid and gas phases become indistinguishable, and the substance becomes a supercritical fluid. In this supercritical state, the fluid can diffuse through solids like a gas and dissolve materials like a liquid, enabling unique chemical applications and extractions.
The main types of crystals are categorized based on the types of particles that make up the crystal and the nature of the bonds holding them together. These include:
- Ionic crystals: Comprise ions and are held together by ionic bonds. Characterized by high melting points and hardness, and are often soluble in water.
- Covalent or network crystals: Atoms are connected by covalent bonds in a continuous network. They are very hard, have high melting points, and are generally insoluble.
- Metallic crystals: Consist of metal atoms packed closely together, bonded by a "sea" of delocalized electrons, allowing for conductivity and malleability.
- Molecular crystals: Composed of molecules held together by weaker forces such as London dispersion, dipole-dipole interactions, or hydrogen bonds. These crystals tend to have lower melting points and are usually soft.
X-ray crystallography is a technique that enables us to determine the atomic and molecular structure of a crystal. When a crystal is bombarded with X-rays, the electrons within the crystal scatter the incoming rays in various directions. This scattering produces a diffraction pattern, which can be analyzed to reveal the positions of the atoms within the crystal, thereby providing a three-dimensional picture of the internal arrangement of the atoms, ions, or molecules. This information is crucial in fields like chemistry, biology, materials science, and physics, as it helps in understanding the properties and functions related to the crystal structure.
Unit cells are the basic building blocks of a crystal structure, representing the smallest portion of the crystal lattice that, when repeated in three dimensions, creates the entire crystal. They capture the geometric shape of the crystal lattice and contain the lattice points that represent the repetitive arrangement of atoms, ions, or molecules in the crystal. By examining a unit cell, one can determine the symmetry, dimensions, and orientation of the crystal, as well as infer the crystal system to which it belongs.
Metals commonly crystallize in three main types of crystal structures: face-centered cubic (FCC), body-centered cubic (BCC), and hexagonal close-packed (HCP). Each of these structures influences material properties in distinct ways.
- The FCC structure, found in metals like aluminum, copper, and gold, has atoms packed closely together, allowing for greater ductility and the ability to undergo plastic deformation.
- In contrast, the BCC structure, characteristic of metals such as iron at room temperature, typically has a lower packing efficiency, resulting in materials that are generally stronger but less ductile.
- Lastly, metals with an HCP structure, like zinc and magnesium, often have limited slip systems which can lead to anisotropic behavior, meaning their mechanical properties are direction-dependent. These crystal structures are critical in determining mechanical properties such as hardness, tensile strength, and malleability.