Chapter 10 and 11 Intermolecular forces and phases of matter Why does matter exist in different phases? What if there were no intermolecular forces? The.

Chapter 10 and 11

Intermolecular forces and phases of matter

Why does matter exist in different phases?

What if there were no intermolecular forces? The ideal gas

Physical phases of matter

• Gas• Liquid• Solid• Plasma

Physical properties of the states of matter

Gases:1. Highly compressible2. Low density3. Fill container completely4. Assume shape of container5. Rapid diffusion6. High expansion on heating

Liquid (condensed phase)

1. Slightly compressible2. High density3. Definite volume, does not

expand to fill container4. Assumes shape of container5. Slow diffusion6. Low expansion on heating

Solid (condensed phase)1. Slightly compressible2. High density3. Rigidly retains its volume4. Retains its own shape5. Extremely slow diffusion;

occurs only at surfaces6. Low expansion on heating

Why water exists in three phases?

• Kinetic energy(the state of substance at room temperature depends on the strength of attraction between its particles)

• Intermolecular forces stick molecules together (heating and cooling)

Intermolecular forces

• London Force or dispersion forces • Dipole-dipole• Hydrogen bond

London Force

•Weak intermolecular force exerted by molecules on each other, caused by constantly shifting electron imbalances.•This forces exist between all molecules.•Polar molecules experience both dipolar and London forces.•Nonpolar molecules experience only London intermolecular forces

Dipole-dipole

• Intermolecular force exerted by polar molecules on each other.

• The name comes from the fact that a polar molecule is like an electrical dipole, with a + charge at one end and a - charge at the other end. The attraction between two polar molecules is thus a "dipole-dipole" attraction.

Hydrogen bond

• Intermolecular dipole-dipole attraction between partially positive H atom covalently bonded to either an O, N, or F atom in one molecule and an O, N, or F atom in another molecule.

To form hydrogen bonds, molecules must have at least one of these covalent bonds:• H-N or H-N=• H-O-• H-F

Nonmolecular substances

• Solids that don’t consist of individual molecules.

• Ionic compounds(lattices of ions)• They are held together by strong

ionic bonds• Melting points are high

Other compounds

• Silicon dioxide(quartz sand) and diamond (allotrope of carbon)

• These are not ionic and do not contain molecules

• They are network solids or network covalent substances

Real Gas

• Molecules travel fast• Molecules are far apart• Overcome weak attractive forces

Ideal Gas

• Gas that consists of particles that do not attract or repel each other.

• In ideal gases the molecules experience no intermolecular forces.

• Particles move in straight paths.• Does not condense to a liquid or

solid.

Ideal Ideal GasesGasesIdeal gases are imaginary gases that perfectly fit all of the assumptions of the kinetic molecular theory.

  Gases consist of tiny particles that are far apart relative to their size.   Collisions between gas particles and between

particles and the walls of the container are elastic collisions

  No kinetic energy is lost in elastic collisions

Ideal Gases Ideal Gases (continued)   Gas particles are in constant, rapid motion. They

therefore possess kinetic energy, the energy of motion

  There are no forces of attraction between gas particles

  The average kinetic energy of gas particles depends on temperature, not on the identity of the particle.

Measurable properties used to describe a gas:

• Pressure (P) P=F/A• Volume (V)• Temperature (T) in Kelvins• Amount (n) specified in moles

PressurePressure

 Is caused by the collisions of molecules with the walls of a container  is equal to force/unit area  SI units = Newton/meter2 = 1 Pascal (Pa)  1 standard atmosphere = 101.3 kPa  1 standard atmosphere = 1 atm =

760 mm Hg = 760 torr

Measuring Measuring PressurePressure

The first device for measuring atmospheric pressure was developed by Evangelista Torricelli during the 17th century.The device was called a “barometer”

  Baro = weight   Meter = measure

An Early An Early BarometerBarometer

The normal pressure due to the atmosphere at sea level can support a column of mercury that is 760 mm high.

Units of PressureUnits of PressureUnit Symbo

l Definition/Relationship

Pascal Pa SI pressure unit

1 Pa = 1 newton/meter2

Millimeter of mercury

mm Hg Pressure that supports a 1 mm column of mercury in a barometer

Atmosphere atm Average atmospheric pressure at sea level and 0 C

Torr torr 1 torr = 1 mm Hg

Standard Temperature and Standard Temperature and PressurePressure

“STP”“STP”

  P = 1 atmosphere, 760 torr, 101.3 kPa   T = C, 273 Kelvins   The molar volume of an ideal gas is 22.4 liters at STP

Behavior of gases

• Rule 1: P is proportional to 1/V• Rule 2: P is proportional to T• Rule 3: P is proportional to nCombining all three:P is proportional to nT/VP=constant x nT/vR=constant= 0.0821 L atm/K mole

Boyle’s Law

• P inversely proportional to V• PV= k• Temperature and number of moles

constant

Boyle’s LawBoyle’s Law

Pressure is inversely proportional to volume when temperature is held constant.

2211 VPVP

A Graph of Boyle’s A Graph of Boyle’s LawLaw

Charles’s Law

• V directly proportional to T• T= absolute temperature in kelvins

• V/T =k2

• Pressure and number of moles constant

Charles’s LawCharles’s Law

 The volume of a gas is directly proportional to temperature, and extrapolates to zero at zero Kelvin.

(P = constant)

VT

VT

P1

1

2

2 ( constant)

Temperature MUST be in KELVINS!

A Graph of Charles’ A Graph of Charles’ LawLaw

Gay Lussac’s LawGay Lussac’s Law

The pressure and temperature of a gas are directly related, provided that the volume remains constant.

2

2

1

1

T

P

T

P

Temperature MUST be in KELVINS!

A Graph of Gay-Lussac’s A Graph of Gay-Lussac’s LawLaw

The Combined Gas LawThe Combined Gas Law

The combined gas law expresses the relationship between pressure, volume and temperature of a fixed amount of gas.

2

22

1

11

T

VP

T

VP

Boyle’s law, Gay-Lussac’s law, and Charles’ law are all derived from this by holding a variable constant.

Standard Molar Standard Molar VolumeVolume

Equal volumes of all gases at the same temperature and pressure contain the same number of molecules.

- Amedeo Avogadro

Avogadro’s Law

• V directly proportional to n

• V/n = k3

• Pressure and temperature are constant

Dalton’s Law of Partial Dalton’s Law of Partial PressuresPressures

For a mixture of gases in a container,

PTotal = P1 + P2 + P3 + . . .

This is particularly useful in calculating the pressure of gases collected over water.

Ideal Gas LawIdeal Gas Law

PV = nRT  P = pressure in atm  V = volume in liters  n = moles  R = proportionality constant

= 0.0821 L atm/ mol·

 T = temperature in Kelvins

Holds closely at P < 1 atm

Gas DensityGas Density

molar mass

molar volume

massDensity

volume

… so at STP…

molar mass

22.4 LDensity

Density and the Ideal Gas Density and the Ideal Gas LawLaw

Combining the formula for density with the Ideal Gas law, substituting and rearranging algebraically:

MPD

RT

M = Molar Mass

P = Pressure

R = Gas Constant

T = Temperature in Kelvins

Diffusion: describes the mixing of gases. The rate of diffusion is the rate of gas mixing.

DiffusionDiffusion

EffusionEffusionEffusion: describes the passage of gas into an evacuated chamber.

Rate of effusion for gas 1Rate of effusion for gas 2

2

1

MM

Distance traveled by gas 1Distance traveled by gas 2

2

1

MM

Effusion:Effusion:

Diffusion:Diffusion:

Graham’s LawGraham’s LawRates of Effusion and DiffusionRates of Effusion and Diffusion