3.2 thermal properties of matter

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Thermal Physics Topic 3.2 Thermal Properties of Matter

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Page 1: 3.2 Thermal Properties of Matter

Thermal Physics

Topic 3.2 Thermal Properties of Matter

Page 2: 3.2 Thermal Properties of Matter

Heat Capacity/Thermal Capacity When substances undergo the same

temperature change they can store or release different amounts of energy

They have different Heat Capacities Heat capacity = Q / T in JK-1

Q = the change in thermal energy in joules

T = the change in temperature in Kelvin Defined as the amount of energy to

change the temperature of a body by unit temperature

Applies to a specific BODY

Page 3: 3.2 Thermal Properties of Matter

Heat Capacity - 2

A body with a high heat capacity will take in thermal energy at a slower rate than a substance with a low heat capacity because it needs more time to absorb a greater quantity of thermal energy

They also cool more slowly because they give out thermal energy at a slower rate

Page 4: 3.2 Thermal Properties of Matter

Specific Heat Capacity

Defined as the amount of thermal energy required to produce unit temperature rise in unit mass of the MATERIAL

Unit mass is normally 1kg, and unit temperature rise is normally 1K

Specific Heat Capacity = Q / (mT)

in J kg -1 K-1

• where m is the mass of the material

Page 5: 3.2 Thermal Properties of Matter

For an object made of 1specific material then

Heat Capacity = m x Specific Heat Capacity

Page 6: 3.2 Thermal Properties of Matter

Specific Heat Capacity - 2 Unit masses of different

substances contain

• different numbers of molecules• of different types• of different masses

If the same amount of internal energy is added to each unit mass

• it is distributed amongst the molecules

Page 7: 3.2 Thermal Properties of Matter

Specific Heat capacity - 3 The average energy change

of each molecule will be different for each substance

Therefore the temperature changes will be different

So the specific heat capacities will be different

Page 8: 3.2 Thermal Properties of Matter

Methods of finding the S.H.C Two methods

• Direct• Indirect

Page 9: 3.2 Thermal Properties of Matter

Direct Method - Liquids Using a calorimeter of known

Heat Capacity

(or Specific Heat Capacity of the material and the mass of the calorimeter)

Because Heat Capacity = Mass x Specific Heat Capacity

Page 10: 3.2 Thermal Properties of Matter

SHC of Liquids

ThermometerCalorimeterHeating coilLiquidInsulation

Stirrer To joulemeteror voltmeterand ammeter

Page 11: 3.2 Thermal Properties of Matter

Calculations - Liquids

Electrical Energy input is equal to the thermal energy gained by the liquid and the calorimeter – this is the assumption that we are making

Electrical energy = V x I x t Energy gained by liquid = ml cl

Tl

Energy gained by calorimeter = mc cc Tc

Page 12: 3.2 Thermal Properties of Matter

Calculations - Liquids -2 Using conservation of energy Electrical energy in = thermal

energy gained by liquid + thermal energy gained by calorimeter

V x I x t = ml cl Tl + mc cc Tc

The only unknown is the specific heat capacity of the liquid

Page 13: 3.2 Thermal Properties of Matter

Direct Method - Solids

Using a specially prepared block of the material

The block is cylindrical and has 2 holes drilled in it• one for the thermometer and one

for the heater• Heater hole in the centre, so the

heat spreads evenly through the block

• Thermometer hole, ½ way between the heater and the outside of the block, so that it gets the averge temperature of the block

Page 14: 3.2 Thermal Properties of Matter

SHC of Solids

InsulationThermometer

Heating coilSolidInsulation

To joulemeteror voltmeterand ammeter

Page 15: 3.2 Thermal Properties of Matter

Calculations - Solids

Again using the conservation of energy

Electrical Energy input is equal to the thermal energy gained by the solid

Electrical energy = V x I x t

Energy gained by solid = ms cs Ts

Page 16: 3.2 Thermal Properties of Matter

Calculations - Solids -2 V x I x t = ms cs Ts

The only unknown is the specific heat capacity of the solid

Page 17: 3.2 Thermal Properties of Matter

Indirect Method

Sometimes called the method of mixtures

In the case of solid, a known mass of solid is heated to a known temperature (usually by immersing in boiling water for a period of time)

Then it is transferred to a known mass of liquid in a calorimeter of known mass

Page 18: 3.2 Thermal Properties of Matter

Indirect Method cont….. The change in temperature is

recorded and from this the specific heat capacity of the solid can be found

Energy lost by block = Energy gained by liquid and calorimeter

mb cb Tb = mw cw Tw + mc cc Tc• the SHC of water and the

calorimeter are needed

Page 19: 3.2 Thermal Properties of Matter

Apparatus

Heat

ThermometerBeakerBoiling WaterBlock

ThermometerCalorimeterWaterBlockInsulation

Page 20: 3.2 Thermal Properties of Matter

Indirect Method – cont…. In the case of a liquid

A hot solid of known specific heat capacity is transferred to a liquid of unknown specific heat capacity

A similar calculation then occurs

Page 21: 3.2 Thermal Properties of Matter

Phases (States) of Matter Matter is defined as anything

that has mass and occupies space

There are 4 states of matter Solids, Liquids, Gases and

Plasmas Most of the matter on the

Earth in the form of the first 3 Most of the matter in the

Universe is in the plasma state

Page 22: 3.2 Thermal Properties of Matter

Macroscopic Macroscopic properties are

all the observable behaviours of that material such as shape, volume, compressibility

The many macroscopic or physical properties of a substance can provide evidence for the nature of that substance

Page 23: 3.2 Thermal Properties of Matter

Macroscopic Characteristics

Characteristics Solid Liquid Gas

Shape Definite Variable Variable

Volume Definite Definite Variable

Compressibilty Almost Incompressible

Very Slightly Compressible

Highly Compressible

Diffusion Small Slow Fast

Comparative Density High High Low

Page 24: 3.2 Thermal Properties of Matter

These will help to explain what is happening at the atomic level, and this part of the model will be interpreted later

Page 25: 3.2 Thermal Properties of Matter

Microscopic Characteristics

Characteristics Solid Liquid Gas

KE Vibrational

Vibrational Rotational

Some Translational

Mostly Translational

Higher Rotational

Higher Vibrational

PE High Higher Highest

Page 26: 3.2 Thermal Properties of Matter

Fluids

Liquids Gases are both fluids Because they FLOW

Page 27: 3.2 Thermal Properties of Matter

Arrangement of Particles - 1 Solids

•Closely packed •Strongly bonded to neighbours•held rigidly in a fixed position•the force of attraction between particles gives them PE

Page 28: 3.2 Thermal Properties of Matter

Arrangement of Particles - 2

Liquids

•Still closely packed •Bonding is still quite strong•Not held rigidly in a fixed position and bonds can break and reform•PE of the particles is higher than a solid because the distance between the particles is higher

Page 29: 3.2 Thermal Properties of Matter

Arrangement of Particles - 3

Gases

•Widely spaced •Only interact significantly on closest approach or collision•Have a much higher PE than liquids because the particles are furthest apart

Page 30: 3.2 Thermal Properties of Matter

Changes of State

A substance can undergo changes of state or phase changes at different temperatures

Pure substances have definite melting and boiling points which are characteristic of the substance

Page 31: 3.2 Thermal Properties of Matter

Changes of State - 2

The moving particle theory can be used to explain the microscopic behaviour of these phase changes• When the solid is heated the

particles of the solid vibrate at an increasing rate as the temperature is increased

• The vibrational KE of the particles increases

Page 32: 3.2 Thermal Properties of Matter

Changes of State -3

• At the melting point a temperature is reached at which the particles vibrate with sufficient thermal energy to break from their fixed positions and begin to slip over each other

• As the solid continues to melt more and more particles gain sufficient energy to overcome the forces between the particles and over time all the solid particles are changed to a liquid

• The PE of the system increases as the particles move apart

Page 33: 3.2 Thermal Properties of Matter

Changes in State - 4

• As the heating continues the temperature of the liquid rises due to an increase in the vibrational, rotational and translational energy of the particles

• At the boiling point a temperature is reached at which the particles gain sufficient energy to overcome the inter-particle forces and escape into the gaseous state. PE increases.

• Continued heating at the boiling point provides the energy for all the particles to change

Page 34: 3.2 Thermal Properties of Matter

Heating Curve

Solid

Liquid

GasSolid - liquidphase change

Liquid - gasphase change

Temp / oC

Time /min

Page 35: 3.2 Thermal Properties of Matter

Changes of State

GASSOLID LIQUID

Freezing/solidification

vaporisation

condensation

melting

sublimation

Thermal energy given out

Thermal energy added

Page 36: 3.2 Thermal Properties of Matter

Evaporation

The process of evaporation is a change from the liquid state to the gaseous state which occurs at a temperature below the boiling point

The Moving Particle (Kinetic) theory can be applied to understand the evaporation process

Page 37: 3.2 Thermal Properties of Matter

Explanation

A substance at a particular temperature has a range of particle energies

So in a liquid at any instant, a small fraction of the particles will have KE considerably greater than the average value

Page 38: 3.2 Thermal Properties of Matter

So

If these particles are near the surface of the liquid, they will have enough KE to overcome the attractive forces of the neighbouring particles and escape from the liquid as a gas

This energy is needed as gases have more PE than liquids.

Page 39: 3.2 Thermal Properties of Matter

Cooling

Now that the more energetic particles have escaped

The average KE of the remaining particles in the liquid will be lowered

Since temperature is related to the average KE of the particles

A lower KE infers a lower temperature

Page 40: 3.2 Thermal Properties of Matter

Cool

This is why the temperature of the liquid falls as an evaporative cooling takes place

A substance that cools rapidly is said to be a volatile liquid

When overheating occurs in a human on hot days, the body starts to perspire

Evaporation of the perspiration cools the body

Page 41: 3.2 Thermal Properties of Matter

Factors Affecting The Rate Evaporation can be increased

by• Increasing temperature(more particles have a higher KE)• Increasing surface area(more particles closer to the

surface)• Increasing air flow above the

surface(gives the particles somewhere to

go to)

Page 42: 3.2 Thermal Properties of Matter

Latent Heat

The thermal energy which a particle absorbs in melting, vaporising or sublimation or gives out in freezing, condensing or sublimating is called Latent Heat because it does not produce a change in temperature

Page 43: 3.2 Thermal Properties of Matter

Latent Heat cont….

When thermal energy is absorbed/released by a body, the temperature may rise/fall, or it may remain constant

• If the temperature remains constant then a phase change will occur as the thermal energy must either increase the PE of the particles as they move further apart

• or decrease the PE of the particles as they move closer together

Page 44: 3.2 Thermal Properties of Matter

Definition

The quantity of heat energy required to change one kilogram of a substance from one phase to another, without a change in temperature is called the Specific Latent Heat of Transformation

Latent Heat = Q / m in J kg -1

Page 45: 3.2 Thermal Properties of Matter

Types of Latent Heat

Fusion Vaporisation Sublimation

The latent heat of fusion of a substance is less than the latent heat of vaporisation or the latent heat of sublimation

Page 46: 3.2 Thermal Properties of Matter

Questions

When dealing with questions think about

• where the heat is being given out

• where the heat is being absorbed

• try not to miss out any part

Page 47: 3.2 Thermal Properties of Matter

Methods of finding Latent Heat Using similar methods as for

specific heat capacity The latent heat of fusion of

ice can be found by adding ice to water in a calorimeter

Page 48: 3.2 Thermal Properties of Matter

Apparatus

Block of ice

ThermometerCalorimeterWaterBlock of iceInsulation

Page 49: 3.2 Thermal Properties of Matter

The change in temperature is recorded and from this the latent heat of fusion of the ice can be found

Energy gained by block melting = Energy lost by liquid and calorimeter

mb Lb = mw cw Tw + mc cc Tc

the SHC of water and the calorimeter are needed

Page 50: 3.2 Thermal Properties of Matter

The latent heat of vaporisation of a liquid could be found by an electrical method

Page 51: 3.2 Thermal Properties of Matter

Latent Heat of Vaporisation

InsulationThermometer

Heating coilLiquid in Calorimeter

To joulemeteror voltmeterand ammeter

Page 52: 3.2 Thermal Properties of Matter

The initial mass of the liquid is recorded

The change in temperature is recorded for heating the liquid to boiling

The liquid is kept boiling The new mass is recorded Energy supplied by heater = energy

to raise temperature of liquid + energy use to vaporise some of the liquid

(The calorimeter also needs to be taken in to account.

V I t = ml clTl+ me Le + mc ccTc

Page 53: 3.2 Thermal Properties of Matter

Pressure

Pressure can be explained by the collisions with the sides of the container

If the temperature increases, the average KE of the particles increases

The increase in velocity of the particles leads to a greater rate of collisions and hence the pressure of the gas increases as the collisions with the side have increased

Also the change in momentum is greater, therefore greater force

Page 54: 3.2 Thermal Properties of Matter

Pressure continued

When a force is applied to a piston in a cylinder containing a volume of gas

The particles take up a smaller volume

Smaller area to collide with And hence collisions are

more frequent with the sides leading to an increase in pressure

Page 55: 3.2 Thermal Properties of Matter

Also, as the piston is being moved in

It gives the particles colliding with it more velocity

Therefore they have more KE Therefore the temperature of the

gas rises.

Page 56: 3.2 Thermal Properties of Matter

Collisions

Because the collisions are perfectly elastic

There is no loss of KE as a result of the collisions

Page 57: 3.2 Thermal Properties of Matter

An Ideal Gas

Is a theoretical gas that obeys the gas laws

And thus fit the ideal gas equation exactly

Page 58: 3.2 Thermal Properties of Matter

Real Gases

Real gases conform to the gas laws under certain limited conditions

But they condense to liquids and then solidify if the temperature is lowered

Furthermore, there are relatively small forces of attraction between particles of a real gas

This is not the case for an ideal gas

Page 59: 3.2 Thermal Properties of Matter

The Kinetic Theory of Gases When the moving particle

theory is applied to gases it is generally called the kinetic theory

The kinetic theory relates the macroscopic behaviour of an ideal gas to the microscopic behaviour of its molecules or atoms

Page 60: 3.2 Thermal Properties of Matter

Macroscopic Behaviour The large number of particles

ensures that the number of particles moving in all directions is constant at any time

Page 61: 3.2 Thermal Properties of Matter

Boyle’s Law

States that the pressure of a fixed mass of gas is inversely proportional to its volume at constant temperature

P 1/V or PV = constant

When the conditions are changed

P1V1 = P2V2

Page 62: 3.2 Thermal Properties of Matter

The Experiment

Air fromfoot pump

Bourdon Pressuregauge

Volume of dry air

oil

Page 63: 3.2 Thermal Properties of Matter

What to do

A column of trapped dry air in a sealed tube by the oil

The pressure on this volume of air can be varied by pumping air in or out of the oil reservoir to obtain different pressures

Wait to allow the temperature to return to room temperature

Page 64: 3.2 Thermal Properties of Matter

The Results

P

V

P

1/ V

PV

P

Page 65: 3.2 Thermal Properties of Matter

Charles’ Law

States that the volume of a fixed mass of gas is directly proportional to its absolute temperature at constant pressure

V T or V/T = constant

When the conditions are changed

V1/T1 = V2/T2

Page 66: 3.2 Thermal Properties of Matter

The ExperimentTap 1

Tap 2 Tap 3

Water reservoir

Fixed massof gas

Mercury in U tube

Page 67: 3.2 Thermal Properties of Matter

What to do

Fill the mercury column with mercury using the right hand tube (tap 1 open, tap 2 closed)

With tap 1 open drain some mercury using tap 2, then close tap 1 and 2. To trap a fixed mass of gas

Fill the jacket with water (make sure tap 3 is closed)

Page 68: 3.2 Thermal Properties of Matter

and then

Change the temperature of the water by draining some water from tap 3 and adding hot water

Equalise the pressure by leveling the columns using tap 2

Read the volume from the scale

Page 69: 3.2 Thermal Properties of Matter

The Results

V

T K

V

T oCA value forabsolute zero

Page 70: 3.2 Thermal Properties of Matter

The Pressure Law

States that the pressure of a fixed mass of gas is directly proportional to its absolute temperature at constant volume

P T or P/T = constant

When the conditions are changed

P1/T1 = P2/T2

Page 71: 3.2 Thermal Properties of Matter

The Experiment

Bourdon gauge

Ice

WaterFixedMass ofgas

Heat

Page 72: 3.2 Thermal Properties of Matter

What to do

Change the temperature of the water by heating it

Record the pressure of the gas

Page 73: 3.2 Thermal Properties of Matter

The Results

P

T K

P

T oCA value forabsolute zero

Page 74: 3.2 Thermal Properties of Matter

Absolute Zero and the Kelvin Scale Charles’ Law and the Pressure

Law suggest that there is a lowest possible temperature that substances can go

This is called Absolute Zero The Kelvin scale starts at this

point and increases at the same scale as the Celsius Scale

Page 75: 3.2 Thermal Properties of Matter

Therefore -273oC is equivalent to 0 K

∆1oC is the same as ∆1 K To change oC to K, add 273 To change K to oC, subtract

273

Page 76: 3.2 Thermal Properties of Matter

Combining the Laws

The gas laws can be combined to give a single equation

For a fixed mass of gas its pressure times its volume divided by its absolute temperature is a constant

PV/T = k So that P1V1/T1 = P2V2/T2

Page 77: 3.2 Thermal Properties of Matter

The Ideal Gas Equation PV = nRT Where n is the number of

moles R is the universal gas

constant 8.31 J mol-1 K-1

Page 78: 3.2 Thermal Properties of Matter

An Ideal Gas

Is a theoretical gas that obeys the gas laws

And thus fit the ideal gas equation exactly

Page 79: 3.2 Thermal Properties of Matter

Real Gases

Real gases conform to the gas laws under certain limited conditions

But they condense to liquids and then solidify if the temperature is lowered

Furthermore, there are relatively small forces of attraction between particles of a real gas

This is not the case for an ideal gas

Page 80: 3.2 Thermal Properties of Matter

The Kinetic Theory of Gases When the moving particle

theory is applied to gases it is generally called the kinetic theory

The kinetic theory relates the macroscopic behaviour of an ideal gas to the microscopic behaviour of its molecules or atoms

Page 81: 3.2 Thermal Properties of Matter

The Postulates

Gases consist of tiny particles called atoms or molecules

The total number of particles in a sample is very large

The particles are in constant random motion

The range of the intermolecular forces is small compared to the average separation

Page 82: 3.2 Thermal Properties of Matter

The Postulates continued The size of the particles is

relatively small compared with the distance between them

Collisions of a short duration occur between particles and the walls of the container

Collisions are perfectly elastic

Page 83: 3.2 Thermal Properties of Matter

The Postulates continued No forces act between the

particles except when they collide

Between collisions the particles move in straight lines

And obey Newton’s Laws of motion

Page 84: 3.2 Thermal Properties of Matter

Macroscopic Behaviour The large number of

particles ensures that the number of particles moving in all directions is constant at any time

Page 85: 3.2 Thermal Properties of Matter

Pressure Pressure can be explained by

the collisions with the sides of the container

If the temperature increases, the average KE of the particles increases

The increase in velocity of the particles leads to a greater rate of collisions and hence the pressure of the gas increases as the collisions with the side have increased

Also the change in momentum is greater, therefore greater force

Page 86: 3.2 Thermal Properties of Matter

Pressure continued When a force is applied to

a piston in a cylinder containing a volume of gas

The particles take up a smaller volume

Smaller area to collide with

And hence collisions are more frequent with the sides leading to an increase in pressure

Page 87: 3.2 Thermal Properties of Matter

Also, as the piston is being moved in

It gives the particles colliding with it more velocity

Therefore they have more KE Therefore the temperature of the

gas rises.

Page 88: 3.2 Thermal Properties of Matter

Collisions

Because the collisions are perfectly elastic

There is no loss of KE as a result of the collisions