When describing an ideal gas, the following assumptions are made
The motion of all particles is random
All particles are in constant, random motion
All particles travel in straight lines
intermolecular (electrostatic) and gravitational forces are negligible
All particles of a particular gas are identical and perfect spheres
Internal energy of the gas is entirely kinetic
All collisions between particles and the walls of the container are completely elastic (no loss of kinetic energy)
Particles take up negligible volume (pressure is due to mobility)
Newton’s Laws of Motion apply
An object travelling at a constant velocity, or at rest, will remain at that constant velocity or at rest, unless acted upon by an external force. i.e., inertia
Force is equal to the product of mass and acceleration
Every action has an equal and opposite reaction
From Lucarelli
Gases are composed of particles in continuous rapid, random motion
Attraction and repulsion between particles in the gas is negligible
The particles of a gas are widely spaced such that the total volume of all the particles is negligible compared to the volume occupied by the gas
The average kinetic energy of the particles of a gas is proportional to its temperature, and is the same for all gases at the same temperature
Particle collisions are elastic (and collisions with the container walls)
i.e. over time, as particles collide, they do not lose speed or slow down, thus particles do not lose kinetic energy (i.e. cool down) due to their collisions
Gas Laws
Describe how gases behave
Can be predicted by the kinetic theory
Kinetic theory: all matter consists of tiny particles that are in constant motion
Real Gases
Do have volume
Attraction between particles
Can condense or solidify
Ideal Gases
No volume
No attraction between particles
Follows gas laws at all temperatures and pressures
Real gases differ most from ideal gases at low temperatures and high pressures
In order to completely describe a gas you need to measure 4 things
Pressure
Temperature
Volume
Number of particles
Gas Pressure
Pressure: force per unit area
Gas particles exert pressure when they collide with the walls of their container
The SI unit of pressure is the pascal (Pa)
However, there are several units of pressure
Pascal ()
Kilopascal (kPa)
Atmosphere (atm)
Temperature
Average kinetic energy is directly proportionate to the Kelvin temperature
At absolute 0 (0 degrees kelvin or -273.15 ˚ C), there is no molecular motion
Standard temperature and pressure:
0˚ C or 273.15 K
Standard pressure: 1 atm = 760 mm Hg = 760 torr = 101.3 kPa
Kelvin = 273.15 + ˚C
˚C = Kelvin - 273.15
Ideal Gas Laws
Given that the gas is ✨ideal✨
Boyle’s Law
The pressure of a gas increases as its volume decreases, and vice versa
P1V1=P2V2
tldr: pressure is inversely proportional to volume
As volume decreases, pressure increases
Particles travel less
More collisions with walls of container
More force per unit area exerted
Alternatively, more energy is required to compress the gas, and thus the container can compress
As volume increases, pressure decreases
Particles travel more
Less collisions with walls of container
Less force per unit area exerted
Alternatively, less energy is required to compress the gas, and thus the container can expand
We are assuming:
Constant mass
Constant temperature
Brownian Motion
Gas particles move in an irregular, seemingly random path
Example: smoke
When an air particle bombardes a smoke particle, the smoke particle moves to the original direction of the air particle
The air particle changes its direction to that of the smoke particle
Charle’s Law
At a constant pressure, the volume of a gas increases as the temperature of the gas increases, and the volume decreases when the temperature decreases
T1V1=T2V2
Why?
Temperature increases
Increases average kinetic energy
Increases the speed of the particles
More collisions with the walls of the container
The walls of a flexible container expand
Gay-Lussac’s Law
The pressure of a gas is directly proportional to its absolute temperature (Kelvin) at a constant volume
T1P1=T2P2
Combined Law
T1P1V1=T1P2V2
The Ideal Gas Equation
One more gas law exists for changes in the gas properties as well as the amount of gas present in moles
This law is referred to as the Ideal Gas Law because it accurately predicts gas properties of ideal gases
Most gases at moderate conditions behaving like an ideal gas
PV=nRT
P = pressure (kPa)
V = volume (L)
n = moles (mol)
R = 8.314 (universal gas constant)
0.08314 if using litres, atm, mole and kelvin temperature
T = temperature (K)
Avogardro’s Law
Equal volumes of gases at the same temperature and pressure contain eqaul number of molecules
1 mole of any gas takes up a volume of 22.71 L at STP
n=22.71V