Kinetic-Molecular Theory: Non-Ideal Gases Overview

Overview/Topics
1.
Kinetic-Molecular Theory of Gases
2.
Boltzmann-Maxwell Distributions
3.
Ideal Gases vs Non-Ideal Gasses
4.
Non-Ideal Gas Correction factors
Skills to Master
1.
HW 8d
Read
OER 8.5-8.6
 
CHE 111 Fall 2020
Lecture 8d – KM Theory and Non-Ideal Gases
Kinetic-Molecular (KM)
Theory of Gases
 
“The why behind the math”
 
1.
Move in straight lines, collide frequently
2.
Distance between particles is large
(volume is mostly 
empty
 space)
3.
Pressure is caused by collisions between
particles and container walls
4.
No attractive 
forces between particles
therefore collisions are 
elastic
 (no loss of
energy)
5.
Kinetic Energy (KE) is same for all gases
and 
α
 Temperature (K)
 
KE (E
K
) = Kinetic Energy (J)
        m = mass (Kg)
 
u = speed (m/s)
Empty Space
Elastic
Collisions
No Attractive
Forces
Boyle’s Law
 
Volume 
increases
 therefore the frequency of collisions with the walls decreases and
pressure 
decreases
Charles's Law
 
Increasing
 the temperature increases the KE of the molecules which increases the
frequency of collisions and therefore the  pressure.
 
To keep pressure constant the volume must 
increase
 which will result in fewer collision
and a larger surface area both of which would decrease the pressure.
Gay-Lussac’s/Amonton’s Law
 
Increasing the temperature increases the KE of the molecules which result in an increase
in collision and harder collision both of which increase the pressure
Avogadro’s Law
 
Increasing
 the number of mols of gas will increase the number of collisions, thus to keep
pressure and temperature constant the volume must 
increase
 (to decrease the number
of collisions and KE of the collisions)
Daltons’s Law of Partial Pressure
 
Since gas molecules do not interact (ie no IMF’s) than the identity of the gas
molecule hitting the container is irrelevant
KMT→ Ideal Gas Law
 
https://www.youtube.com/watch?v=njQms6VF63o
We don’t need to “know” the
ugly truth, just be able to use it
 
https://www.youtube.com/watch?v=1S2qQc8XTlQ
 
KE (E
K
) = Kinetic Energy (J)
        m = mass (Kg)
 
u = speed (m/s)
Root Mean Square Velocity
 
Due to large number of molecules
use the average speed and KE
OR
Cheat Sheet to
the Rescue!
 
Average velocity of a gas molecule
Speed DP T
Speed IP MW
Example:
 
What is the speed of an “average” Helium atom in the sun (T= 10,000. K)?
Boltzmann Maxwell
Distributions
Speed DP T
Speed IP MW
Curves are not symmetrical therefore…
U
mp
 < u
av
 < u
rms
Speed DP T
Speed IP MW
Boltzmann Maxwell
Distributions
Escape Velocity
Curves are not symmetrical therefore…
U
mp
 < u
av
 < u
rms
Empty Space
Elastic
Collisions
No Attractive
Forces
Crowded
Attractive
Forces
Inelastic
Collisions
Fails
High P
Low T
Works
Low P
High T
Effect of Pressure
on an “Ideal” Gas
Why the Ideal
Gas Law Fails
High Pressure – molecules take up space V
ideal
 
<
 V
real
 
<
 b – size of molec.
n – mols
At 500 atm
V
atoms 
= 20%
Why the Ideal
Gas Law Fails
Low T - Attractive Forces (IMF’s) – decrease #/KE of collisions P
ideal
 > P
real
 
<
 a 
 
– strength of IMF
n/V – density
Van der Waal’s
Equation
 
Johannes van der Waals
(1837-1923)
If n is 
small
correction is
small
Cheat Sheet!
a – strength of IMF
b – size of molecule
If V is 
large
correction is
small
Example:
 
A 5.00 L flask contains 6.00 mols of O
2
 gas at 250. °C.
 
(a)
Calculate the pressure using the “Ideal” gas law
(b)
Calculate the pressure using the van der Waals
equation
Fails
Low T
High P
Low V
Mean Free Path
 
o
How often do collisions occur?
o
How far between collisions?
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Kinetic-Molecular Theory of Gases, Boltzmann-Maxwell Distributions, and the comparison between Ideal and Non-Ideal Gases. Understand correction factors and laws like Boyle's Law, Charles's Law, and Avogadro's Law. See how the concepts of pressure, volume, temperature, and collisions shape the behavior of gases.

  • Kinetic-Molecular Theory
  • Non-Ideal Gases
  • Ideal Gases
  • Gas Laws
  • Collision Frequency

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  1. CHE 111 Fall 2020 Lecture 8d KM Theory and Non-Ideal Gases Overview/Topics Skills to Master 1. Kinetic-Molecular Theory of Gases 2. Boltzmann-Maxwell Distributions 3. Ideal Gases vs Non-Ideal Gasses 4. Non-Ideal Gas Correction factors 1. HW 8d Read OER 8.5-8.6

  2. Kinetic-Molecular (KM) Theory of Gases The why behind the math Empty Space 1. Move in straight lines, collide frequently 2. Distance between particles is large (volume is mostly empty space) 3. Pressure is caused by collisions between particles and container walls 4. No attractive forces between particles therefore collisions are elastic (no loss of energy) 5. Kinetic Energy (KE) is same for all gases and Temperature (K) No Attractive Forces ?? =1 Elastic Collisions 2??2 KE (EK) = Kinetic Energy (J) m = mass (Kg) u = speed (m/s)

  3. Boyles Law Volume increases therefore the frequency of collisions with the walls decreases and pressure decreases Charles's Law Increasing the temperature increases the KE of the molecules which increases the frequency of collisions and therefore the pressure. To keep pressure constant the volume must increase which will result in fewer collision and a larger surface area both of which would decrease the pressure. Gay-Lussac s/Amonton s Law Increasing the temperature increases the KE of the molecules which result in an increase in collision and harder collision both of which increase the pressure

  4. Avogadros Law Increasing the number of mols of gas will increase the number of collisions, thus to keep pressure and temperature constant the volume must increase (to decrease the number of collisions and KE of the collisions) Daltons s Law of Partial Pressure Since gas molecules do not interact (ie no IMF s) than the identity of the gas molecule hitting the container is irrelevant

  5. https://www.youtube.com/watch?v=njQms6VF63o https://www.youtube.com/watch?v=1S2qQc8XTlQ KMT Ideal Gas Law We don t need to know the ugly truth, just be able to use it

  6. Average velocity of a gas molecule Root Mean Square Velocity ?? =1 ?? =3 KE (EK) = Kinetic Energy (J) m = mass (Kg) u = speed (m/s) 2??2 2?? Due to large number of molecules use the average speed and KE KE =1 2mu2=3 2RT OR M = Molecular Weight R = 8.31 J/mol K 1/2 Speed DP T Speed IP MW 3?? ?= 3?? ? uRMS = 1 J = ???2 ?2 Cheat Sheet to the Rescue!

  7. Example: What is the speed of an average Helium atom in the sun (T= 10,000. K)?

  8. Speed DP T Speed IP MW Boltzmann Maxwell Distributions Curves are not symmetrical therefore Ump < uav < urms

  9. Speed DP T Speed IP MW Boltzmann Maxwell Distributions

  10. Escape Velocity Curves are not symmetrical therefore Ump < uav < urms

  11. Works Low P High T Crowded Empty Space Attractive Forces No Attractive Forces Elastic Collisions Inelastic Collisions Fails High P Low T

  12. Effect of Pressure on an Ideal Gas

  13. At 500 atm Vatoms = 20% Why the Ideal Gas Law Fails High Pressure molecules take up space Videal< Vreal V?????=nRT V????=nRT b size of molec. n mols < P + nb P

  14. Why the Ideal Gas Law Fails Low T - Attractive Forces (IMF s) decrease #/KE of collisions Pideal > Preal P?????=nRT < 2 P????=nRT ? ? a V V a strength of IMF n/V density

  15. Van der Waals Equation Johannes van der Waals (1837-1923) If n is small correction is small If V is large correction is small ??? ? ?? ??2 P= ?2 Cheat Sheet! a strength of IMF b size of molecule

  16. ??? ? ?? ??2 Example: P= ?2 A 5.00 L flask contains 6.00 mols of O2 gas at 250. C. (a) Calculate the pressure using the Ideal gas law (b) Calculate the pressure using the van der Waals equation Fails Low T High P Low V

  17. Mean Free Path o How often do collisions occur? o How far between collisions?

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