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Ch. 12 – States of Ch. 12 – States of Matter Matter I. Intermolecular Forces

Ch. 12 – States of Matter I. Intermolecular Forces

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Page 1: Ch. 12 – States of Matter I. Intermolecular Forces

Ch. 12 – States of MatterCh. 12 – States of MatterCh. 12 – States of MatterCh. 12 – States of Matter

I. Intermolecular ForcesI. Intermolecular Forces

Page 2: Ch. 12 – States of Matter I. Intermolecular Forces

A. Definition of IMFA. Definition of IMF

Attractive forces between molecules.

Much weaker than chemical bonds within molecules.

a.k.a. van der Waals forces

Page 3: Ch. 12 – States of Matter I. Intermolecular Forces

C. Johannesson

B. Types of IMFB. Types of IMF

Page 4: Ch. 12 – States of Matter I. Intermolecular Forces

B. Types of IMFB. Types of IMF

London Dispersion Forces

View animation online.

Page 5: Ch. 12 – States of Matter I. Intermolecular Forces

B. Types of IMFB. Types of IMF

Dipole-Dipole Forces

+ -

View animation online.

Page 6: Ch. 12 – States of Matter I. Intermolecular Forces

B. Types of IMFB. Types of IMF

Hydrogen Bonding

Page 7: Ch. 12 – States of Matter I. Intermolecular Forces

C. Determining IMFC. Determining IMF

NCl3• polar = dispersion, dipole-dipole

CH4

• nonpolar = dispersionHF

• H-F bond = dispersion, dipole-dipole, hydrogen bonding

Page 8: Ch. 12 – States of Matter I. Intermolecular Forces

II. Physical PropertiesII. Physical Properties

Ch. 12 - Liquids & SolidsCh. 12 - Liquids & SolidsCh. 12 - Liquids & SolidsCh. 12 - Liquids & Solids

Page 9: Ch. 12 – States of Matter I. Intermolecular Forces

A. Liquids vs. SolidsA. Liquids vs. Solids

LIQUIDS

Stronger than in gases

Y

high

N

slower than in gases

SOLIDS

Very strong

N

high

N

extremely slow

IMF Strength

Fluid

Density

Compressible

Diffusion

Page 10: Ch. 12 – States of Matter I. Intermolecular Forces

B. Liquid PropertiesB. Liquid Properties

Surface Tension• attractive force between particles in a

liquid that minimizes surface area

Page 11: Ch. 12 – States of Matter I. Intermolecular Forces

B. Liquid PropertiesB. Liquid Properties

Capillary Action• attractive force between the surface of

a liquid and the surface of a solid

Page 12: Ch. 12 – States of Matter I. Intermolecular Forces

B. Liquid PropertiesB. Liquid Properties

Viscosity• Measure of the resistance of a liquid to

flow

Page 13: Ch. 12 – States of Matter I. Intermolecular Forces

B. Liquid PropertiesB. Liquid Properties

Cohesion• Force of attraction between

identical moleculesAdhesion

• Force of attraction

between different

molecules water mercury

Page 14: Ch. 12 – States of Matter I. Intermolecular Forces

C. Types of SolidsC. Types of Solids

Crystalline - repeating geometric pattern• covalent network• metallic• ionic• covalent molecular

Amorphous - no geometric pattern

decreasingm.p.

Page 15: Ch. 12 – States of Matter I. Intermolecular Forces

C. Types of SolidsC. Types of Solids

Ionic(NaCl)

Metallic

Page 16: Ch. 12 – States of Matter I. Intermolecular Forces

C. Types of SolidsC. Types of Solids

CovalentMolecular

(H2O)

CovalentNetwork

(SiO2 - quartz)

Amorphous(SiO2 - glass)

Page 17: Ch. 12 – States of Matter I. Intermolecular Forces

C. Types of SolidsC. Types of Solids

Allotrope• In a covalent network, different forms in the same

state

Carbon

allotropeswater mercury

Page 18: Ch. 12 – States of Matter I. Intermolecular Forces

C. Types of SolidsC. Types of Solids

Amorphous Solid• No geometric pattern

water mercury

Page 19: Ch. 12 – States of Matter I. Intermolecular Forces

Ch. 12 - Liquids & SolidsCh. 12 - Liquids & SolidsCh. 12 - Liquids & SolidsCh. 12 - Liquids & Solids

III. Changes of StateIII. Changes of State

Page 20: Ch. 12 – States of Matter I. Intermolecular Forces

A. Phase ChangesA. Phase Changes

Page 21: Ch. 12 – States of Matter I. Intermolecular Forces

A. Phase ChangesA. Phase Changes

EvaporationEvaporation• molecules at the surface gain enough

energy to overcome IMF

VolatilityVolatility• measure of evaporation rate• depends on temp & IMF

Page 22: Ch. 12 – States of Matter I. Intermolecular Forces

A. Phase ChangesA. Phase Changes

Kinetic Energy

# o

f P

art

icle

s

Boltzmann Distribution

temp

volatility

IMF

volatility

Page 23: Ch. 12 – States of Matter I. Intermolecular Forces

A. Phase ChangesA. Phase Changes

EquilibriumEquilibrium• trapped molecules reach a balance

between evaporation & condensation

Page 24: Ch. 12 – States of Matter I. Intermolecular Forces

A. Phase ChangesA. Phase Changes

Vapor PressureVapor Pressure• pressure of vapor above

a liquid at equilibrium

IMF v.p.temp v.p.

• depends on temp & IMF• directly related to volatility

temp

v.p

.

Page 25: Ch. 12 – States of Matter I. Intermolecular Forces

A. Phase ChangesA. Phase Changes

Boiling Point• temp at which v.p. of liquid

equals external pressure

IMF b.p.Patm b.p.

• depends on Patm & IMF

• Normal B.P. - b.p. at 1 atm

Page 26: Ch. 12 – States of Matter I. Intermolecular Forces

Which has a higher m.p.?• polar or nonpolar?• covalent or ionic?

A. Phase ChangesA. Phase Changes

Melting Point• equal to freezing point

polar

ionic

IMF m.p.

Page 27: Ch. 12 – States of Matter I. Intermolecular Forces

A. Phase ChangesA. Phase Changes

Sublimation

• solid gas

• v.p. of solid equals external pressure

EX: dry ice, mothballs, solid air fresheners

Page 28: Ch. 12 – States of Matter I. Intermolecular Forces

B. Heating CurvesB. Heating Curves

Melting - PE

Solid - KE

Liquid - KE

Boiling - PE

Gas - KE

Page 29: Ch. 12 – States of Matter I. Intermolecular Forces

B. Heating CurvesB. Heating Curves

Temperature Change• change in KE (molecular motion) • depends on heat capacity

Heat Capacity• energy required to raise the temp of 1

gram of a substance by 1°C

Page 30: Ch. 12 – States of Matter I. Intermolecular Forces

B. Heating CurvesB. Heating Curves

Phase Change• change in PE (molecular arrangement)• temp remains constant

Heat of Fusion (Hfus)

• energy required to melt 1 gram of a substance at its m.p.

Page 31: Ch. 12 – States of Matter I. Intermolecular Forces

B. Heating CurvesB. Heating Curves

Heat of Vaporization (Hvap)

• energy required to boil 1 gram of a substance at its b.p.

EX: sweating, steam burns, the drinking bird

Page 32: Ch. 12 – States of Matter I. Intermolecular Forces

C. Phase DiagramsC. Phase Diagrams

Show the phases of a substance at different temps and pressures.

Page 33: Ch. 12 – States of Matter I. Intermolecular Forces

The following slides… same information, different explanation and examples

Page 34: Ch. 12 – States of Matter I. Intermolecular Forces

Phase Changes

Page 35: Ch. 12 – States of Matter I. Intermolecular Forces

Why do liquids and solids form at all?

• KMT postulates– A gas is a collection of small particles traveling in

straight-line motion and obeying Newton's Laws. – The molecules in a gas occupy no volume. – Collisions between molecules are perfectly elastic

• no energy is gained or lost during the collision

– There are no attractive or repulsive forces between the molecules.

– Kinetic energy is proportional to temperatureX

Page 36: Ch. 12 – States of Matter I. Intermolecular Forces

What is a phase?• Region of matter that is:

– chemically uniform– physically distinct– mechanically separable.

• Often synonymous with (same meaning as) “state of matter”

Page 37: Ch. 12 – States of Matter I. Intermolecular Forces

Changing phases

Distinguish liquid vs. solid?

Page 38: Ch. 12 – States of Matter I. Intermolecular Forces

Properties of …• Gas phase

– Like/unlike soccer players on field

• Liquid phase– Like/unlike crowd at a rally– Like/unlike gases

• Solid phase– Like/unlike movie theatre

• Compare intermolecular interactions – gases vs. liquids vs. solids

Page 39: Ch. 12 – States of Matter I. Intermolecular Forces

Phases of matter

Add

mor

e en

ergy

Page 40: Ch. 12 – States of Matter I. Intermolecular Forces

Phase change vocabulary

Page 41: Ch. 12 – States of Matter I. Intermolecular Forces

Phase changes and IMF’s• As InterMolecular Forces increase, melting

and boiling temperatures _________? (increase or decrease)?

Metallic bonding

Network covalent bonding

Larger sphere, higher

melting point

Page 42: Ch. 12 – States of Matter I. Intermolecular Forces

Strength of interactions

• Which simulation has stronger intermolecular interactions? A or B– How do you know?

A BSame temperature

Page 43: Ch. 12 – States of Matter I. Intermolecular Forces

Ranking of intermolecular interactions • Water• Wood• Iron• Air• Gold• Mercury• Carbon dioxide• Oxygen• Gasoline• Lead

vs.

Why?

Page 44: Ch. 12 – States of Matter I. Intermolecular Forces

Why is water special?

• Periodic trends– Boiling and melting points of hydrides

Page 45: Ch. 12 – States of Matter I. Intermolecular Forces

KMT, energy and phase

changes

Page 46: Ch. 12 – States of Matter I. Intermolecular Forces

Total energy

Page 47: Ch. 12 – States of Matter I. Intermolecular Forces

Water phases present?

Page 48: Ch. 12 – States of Matter I. Intermolecular Forces

Heating curves

Why are b and d flat?

Page 49: Ch. 12 – States of Matter I. Intermolecular Forces

Boiling vs. melting

Which takes more energy?(same mass)

Page 50: Ch. 12 – States of Matter I. Intermolecular Forces

Consider liquid gasEvaporation removes energy

Page 51: Ch. 12 – States of Matter I. Intermolecular Forces

Evaporative Cooling

Page 52: Ch. 12 – States of Matter I. Intermolecular Forces

Evaporation and volatility

• Evaporation– molecules at the surface gain enough energy

to overcome attractive intermolecular forces (IMF)

• Volatility– measure of evaporation rate– depends on temperature and IMF

Page 53: Ch. 12 – States of Matter I. Intermolecular Forces

Volatility

Kinetic Energy

# o

f P

art

icle

s

Boltzmann Distribution

temp

volatility

IMF

volatility

Page 54: Ch. 12 – States of Matter I. Intermolecular Forces

Boiling – Fixed temperature

Page 55: Ch. 12 – States of Matter I. Intermolecular Forces

Why do liquids boil?• Boiling Point

–T at which liquid vapor pressure = atmospheric pressure• depends on Patm & IMF

–Normal boiling point - b.p. at 1 atm

IMF b.p.Patm b.p.

Page 56: Ch. 12 – States of Matter I. Intermolecular Forces

Temperature/pressure phase diagram for water

Page 57: Ch. 12 – States of Matter I. Intermolecular Forces

Transition to Supercritical CO2

Page 58: Ch. 12 – States of Matter I. Intermolecular Forces

Interpret phase diagram for water

Page 59: Ch. 12 – States of Matter I. Intermolecular Forces

Draw a phase diagram for NH3

(used as a refrigerant in RV’s and solar cooling systems)

Page 60: Ch. 12 – States of Matter I. Intermolecular Forces

Ammonia phase diagram

Page 61: Ch. 12 – States of Matter I. Intermolecular Forces

Phase Changes Need to know…

• Know why liquids and solids exist at all– Failure of KMT postulate

• Know phase names and changes – molecular views of phases and changes– distinguish S vs. L on molecular level

• Explain heating curve origins and parts– Why no change in T during phase change?

• Explain differences and similarities between evaporation, volatility and boiling

• Explain evaporative cooling on a molecular level

• Interpret temperature-pressure phase diagrams