unit 8 kinetic theory of gases - · pdf fileobjectives 4 define kinetic theory of gases...
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Unit 8 Kinetic Theory of Gases Chapter 13-14
This tutorial is designed to help students understand scientific measurements.
Objectives for this unit appear on the next slide.
◦ Each objective is linked to its description.
◦ Select the number at the front of the slide to go directly to its description.
Throughout the tutorial, key words will be defined.
◦ Select the word to see its definition.
Objectives
4 Define kinetic theory of gases including collisions
5 Define pressure, including atmospheric pressure, vapor pressure, pressure differentials, and how a barometer works
6 Describe boiling points, including normal boiling points, using vapor pressure graphs, explaining the difference between boiling and evaporation, and how intermolecular forces and molecular weight determine evaporation rates
7 Define and use data based on the triple point phase diagram
8 Define and know the variables of the Gas Laws, including Boyle’s Law, Charles’ Law, Gay-Lussac’s Law, and the combined gas law
9 State Avogadro’s Principle
10 Use the ideal gas law to solve problems and know the variables of the ideal gas law
11 State and use Dalton’s Law of Partial Pressures
12 State and use Graham’s Law of effusion and define diffusion
4 The Kinetic Theory
Particles at the molecular level have been
described previously.
It has been stated that these particles are
in a constant state of motion and are
attracted to each other through
intermolecular forces.
The kinetic theory as described on the
next slide is specific to gases.
Kinetic Theory of Gases
There are five parts to the kinetic theory
of gases.
1. Gases will fill the entire volume allowed.
• This means that is 10 oxygen molecules are
released in a classroom, they will arrange
themselves equally throughout that space. If
the same 10 were released in a gymnasium,
they will do the same.
Kinetic Theory of Gases
2. Gases can be compressed.
The volume a gas holds can be
increased or decreased.
3. The motion of gases is random.
Gas molecules will travel in straight
lines until they run into an object.
4. Gas molecules have elastic collision.
When gas molecules collide, there is
no loss in kinetic energy.
Kinetic Theory of Gases
5. The kinetic energy of a gas molecule is
measured by temperature.
As the temperature increases, gas
molecules move faster, and as the
temperature decreases, gas molecules
move slower.
Kinetic Theory of Gases
A quick recap:
1. Gases fill the entire volume allowed.
2. Gases can be compressed.
3. The motion of a gas is random.
4. Gases have elastic collisions.
5. The kinetic energy of gases is measured
with temperature.
The link below is for a simulator that demonstrates some of these ideas.
http://phet.colorado.edu/en/simulation/gas-properties
5 Pressure
Pressure is a measure of force per unit surface area.
◦ For instance, assume you are standing. You are exerting a force on the floor. The surface area is the size of both of your feet. If you stand on only one foot, the force would be the same but the surface area is halved so the pressure doubles.
When referring to gases, pressure is the measure of the force exerted when two gas particles collide.
Air Pressure and Vapor Pressure
The molecules that make of the air
around you are constantly colliding with
each other and the objects in the room
(including you).
These collisions make up air pressure.
Vapor pressure is the pressure exerted by
the air on a liquid.
Measuring pressure
Atmospheric pressure is determined using an instrument known as a barometer.
The barometer is filled with mercury because of its density.
As atmospheric pressure pushes down on the mercury, it forces the mercury up the column.
Atmospheric pressure is measured by the distance the mercury is displaced.
Mercury
760
mm
Atmospheric
Pressure
Pressure
The barometer was invented by a
scientist by the name of Torricelli.
◦ Pressure is often given with units of mm Hg
but the torr is used as well.
To make the numbers easier to work
with, atmospheric pressure was set equal
to 1 atm (atmosphere)
Units of Pressure
There are several units for pressure and all are used.
Therefore the following values are equal to atmospheric pressure:
1 atm = 101.325 kPa (kiloPascals)
101,325 Pa (Pascals)
760 mm Hg
760 torr
6 Temperature vs. Heat
The last part of the kinetic theory
mentioned temperature.
Temperature is often confused with heat but
the two are quite different.
Temperature is a measure of the average
kinetic energy of molecules.
Heat is the measure of the total kinetic energy
of molecules.
Temperature vs. Heat
All molecules are in a state of motion.
The motion is measured by kinetic energy.
However, not all molecules are moving at
the same speed and thus do not have the
same kinetic energy.
The average is taken to determine the
speed of the majority of the molecules.
The total is determined for a purpose
that will be discussed in Unit 9.
Temperature
The average kinetic energy is reported in
three different scales.
◦ Fahrenheit (°F)
◦ Celsius (°C)
◦ Kelvin (K)
Each scale is used by certain individuals
about the world.
The scientific community prefers Celsius
or Kelvin.
Temperature
The Celsius scale was designed to have the
boiling point of water be 100°C while the
freezing point of water would be 0°C.
The Kelvin scale was designed using the same
increments as Celsius but instead placed zero at
absolute zero.
Temperature
It is important to be able to convert from
one scale to another so the following
equations were determined:
◦ °F =°C9
5+ 32
◦ °C=(°F − 32) 𝑥 5
9
◦ K = 273.15 + °C
Boiling Points
Boiling is the process of taking a liquid to
the gaseous state.
This process occurs by adding heat to the
liquid.
However, there are additional factors that
can affect the boiling point.
◦ These include intermolecular forces and
vapor pressure.
Intermolecular Forces
When heat is added to a liquid, the particles in that liquid gain kinetic energy.
Gaining kinetic energy means that they are moving faster.
It is the intermolecular forces that hold the molecules close together.
With enough kinetic energy, a molecule can overcome the intermolecular forces and break free.
The stronger the intermolecular force, the more kinetic energy will be required to break free.
Boiling versus Evaporation
It also depends on where the heat is
added as to how easy it will be to
overcome the intermolecular force.
Both boiling and evaporation are ways to
bring a liquid to a gas but each can occur
at different temperatures.
Evaporation
When considering evaporation, the heat comes from a source above the liquid.
This means the particles on the top of the liquid gain kinetic energy (shown in red)
Once they gain enough energy, they can break free of the intermolecular forces.
Notice, it is only the top that increases kinetic energy while the rest of the molecules remain the same.
This is why the temperature of the liquid does not have to greatly increase during evaporation.
Heat
Boiling In comparison to evaporation, boiling adds heat to the bottom of the liquid.
Since the bottom particles have to work their way to the top, it is more difficult to overcome the intermolecular forces.
In order to overcome the intermolecular forces, all particles will need to gain kinetic energy.
Because all particles must gain energy, the temperature increases.
This is also why boiling proceeds faster than evaporation.
Vapor Pressure
The other factor effecting the boiling point is vapor pressure.
Vapor pressure is the pressure from the atmosphere above a liquid.
The gas particles above a liquid can prevent molecules that have enough energy to break free from the intermolecular forces from becoming a gas.
The image on the next slide illustrates this idea.
Vapor Pressure
Gas Particles
The particle escapes
but transfers its
energy to a gas
particle.
The particle falls
back to the liquid.
Vapor Pressure
If there were less particles above the
liquid, it would be easier to boil.
The boiling point at one atmosphere is
considered to be the normal boiling
point.
A vapor pressure diagram can help
determine the boiling point.
Vapor Pressure Diagrams
Vapor pressure diagrams show the relationship between vapor pressure and the boiling point.
The red line below represents the normal boiling point.
Notice, it is easier to boiling if there is a smaller vapor pressure. ◦ This liquid would boil at 62°C if the pressure of 0.18 atm. The
normal boiling point is 101°C at 1 atm.
0.00
0.20
0.40
0.60
0.80
1.00
0 20 40 60 80 100 120
Pre
ssu
re (
atm
)
Temperature (C)
Vapor Pressure Diagram
Standard Temperature and Pressure
(STP) For the purposes of scientific consistency,
a select temperature and pressure were
selected.
This way, all experiments could be
repeated at the same atmospheric
conditions.
STP is 1 atm of pressure and 0°C.
7 Triple Point Diagrams
The vapor pressure diagram shows a portion of a larger diagram known as the triple point diagram.
This diagram represents the three types of matter and their relationships to pressure and temperature.
The following slide shows a possible triple point diagram.
◦ There are six phase changes that occur as you cross each line form one phase to the next.
◦ The triple point is denoted with a blue dot.
0.00
0.20
0.40
0.60
0.80
1.00
1.20
0 20 40 60 80 100 120
Pre
ssu
re (
atm
)
Temperature (C)
Triple Point Diagram
Liquid
Gas
Solid
Freezing
Condensation
Vaporization
Triple Pt.
Critical Point
Melting
Sublimation
Deposition
Triple Point Diagrams
The triple point indicates a point where
all three phases are present at the same
time.
◦ It only occurs at one temperature and
pressure for each substance.
The critical point is also marked. The
critical point indicates where the kinetic
theory does not accurately describe the
properties of this chemical.
8 Gas Laws
Temperature, pressure, and volume have a
distinct affect on gases.
It was determined that these three
variables have distinct relationships.
These relationships are known as the gas
laws.
Boyle’s Law
Boyle’s Law describes the relationship
between pressure and volume.
The relationship is inverse which means as
one increases, the
other decreases.
The equation for
Boyle’s Law is:
P1V1=P2V2
0
0.5
1
0 2 4 6 8 10 12
Pre
ssu
re (
atm
)
Volume (L)
Boyle's Law
Charles’ Law
Charles’ Law describes the relationship
between temperature and volume.
The relationship is direct which means as
one increases, the
other increases.
The equation for
Charles’ Law is:
V1÷T1=V2÷T2
0
2
4
6
8
10
12
14
250 270 290 310 330 350
Vo
lum
e (
L)
Temperature (K)
Charles' Law
Gay-Lussac’s Law
Gay-Lussac’s Law describes the relationship
between pressure and temperature.
The relationship is direct which means as
one increases, the
other increases.
The equation for
Gay-Lussac’s Law is:
P1÷T1=P2÷T2
0
0.2
0.4
0.6
0.8
1
1.2
1.4
250 270 290 310 330 350
Pre
ssu
re (
atm
)
Temperature (K)
Gay-Lussac's Law
Gas Laws
The three gas laws described require
certain units to be used.
◦ Volume = liters
◦ Temperature = Kelvin
◦ Pressure = kPa or atm
The three can also be combined.
Combined Gas Law
As that all three variables can be difficult
to hold constant, the three gas laws can
be combined to create the combined gas
law.
𝑃1𝑉1
𝑇1=
𝑃2𝑉2
𝑇2
Gas Law Recap
Gas Law Boyle’s Charles’ Gay-
Lussac’s Combined
Equation P1V1=P2V2 𝑉1
𝑇1=
𝑉2
𝑇2
𝑃1
𝑇1=
𝑃2
𝑇2
𝑃1𝑉1
𝑇1=
𝑃2𝑉2
𝑇2
Relationship Inverse Direct Direct
Constant Temperature Pressure Volume Nothing
9 Avogadro’s Principle
Up to this point, we have examined gases under the assumption that we always held the same number of moles in the container.
This is not always the case.
Just as a relationship was determined between pressure, volume, and temperature, a relationship was determined between the number of moles and volume.
Avogadro’s Principle
According to Avogradro’s Principle, if the
number of moles increase, the volume
also must increase assuming constant
temperature and pressure.
𝑉1
𝑛1=
𝑉2
𝑛2
n = moles
Avogadro’s Principle
Using this principle, it was determined
that at STP (standard temperature and
pressure), one mole of a gas would always
take up the same volume.
At 0°C and 1 atm, 1 mole will take up 22.4
liters.
10 Ideal Gas Law
With the inclusion of the mole into the
relationships of gases, it could be added
to the combined gas law as well.
𝑃𝑉
𝑇= 𝑘
𝑉
𝑛= 𝑘
𝑃𝑉
𝑛𝑇= 𝑘
K represents a constant
Ideal Gas Law
Upon further analysis, it was determined that the constant could be calculated and was the same for each container.
Assume STP conditions:
◦ 1 Mole 𝑃𝑉
𝑛𝑇= 𝑘
◦ 22.4 Liters
◦ 273.15 K 1 𝑎𝑡𝑚 𝑥 22.4 𝐿
1 𝑚𝑜𝑙𝑒 𝑥 273.15 𝐾= 𝑘
◦ 1 atm
k = 0.0821 𝑎𝑡𝑚 𝑥 𝐿
𝑚𝑜𝑙𝑒 𝑥 𝐾
Ideal Gas Law
The constant was changed to R and
requires specific units to be used.
There are two commonly used values for
R: 0.0821 𝑎𝑡𝑚 𝑥 𝐿
𝑚𝑜𝑙𝑒 𝑥 𝐾 or 8.314
𝑘𝑃𝑎 𝑥 𝐿
𝑚𝑜𝑙𝑒 𝑥 𝐾
Required Units:
Volume: Liters Amount: moles
Temperature: Kelvin Pressure: atm or kPa
Ideal Gas Law
The equation for the Ideal Gas Law is:
PV=nRT
The value of R is chosen based on the units
on the pressure.
11 Dalton’s Law of Partial Pressures
When gases were discussed in Unit 10, it
was mentioned that pressure was
measured with the collisions gas particles
underwent.
The total pressure is a sum of all of those
collisions.
Therefore, Dalton’s Law states that the
pressure of each gas can be added to
determine the total pressure.
Dalton’s Law of Partial Pressures
Though Dalton’s Law seems fairly basic, it
is extremely useful when collecting a gas.
When most experiments are performed,
the gases produced are allowed to
escape.
However, if it is the gas that needs to be
analyzed, the gas most be collected.
The collection of this gas is typically done
over water.
Collecting a Gas over Water
Collecting a gas over water requires a sealed container with a tube into a tank of water.
In the tank of water, an inverted tube is filled with water.
As the reaction progresses, the gas produced follows the tube into the water chamber and up the inverted tube.
Dalton’s Law
Dalton’s Law comes into play because a
small amount of water with change to a
gas in the container.
Therefore, the gas collected and water
vapor combine to give the pressure.
That pressure is equal to the atmospheric
pressure outside of the tube.
Therefore, the following equation applies:
Patmosphere = Pgas + Pwater
12 Effusion and Diffusion
Graham’s Law of Effusion states that at the same temperature, a heavier molecule will move slower than a lighter molecule.
◦ Recall that temperature is the average kinetic energy of a molecule.
◦ Kinetic energy is calculated by taking the mass times the velocity squared (KE=mv2)
◦ The relationship between speed and mass is inverse.
Diffusion is the dispersion of molecules from areas of high concentration to areas of low concentration.
This concludes the tutorial on
measurements.
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Definitions-Select the word to return to the tutorial
Absolute zero – the temperature at which
molecules no longer move.
Intermolecular Forces – forces that hold
molecules together. These
include hydrogen bonding,
dipole forces, and London
forces