Unit 1 Kinetic Theory of Gases
KINETIC THEORY OF MATTER
Overview
- Presented by Mr. W. Williams.
STATES OF MATTER
COMPARING STATES
Properties of Different States
| Property | Solid | Liquid | Gas |
|---|
| Arrangement of Particles | Regular repeat pattern (Lattice) | Closely packed | Random arrangement |
| | Random | Very far apart |
| Motion | Vibrate in fixed position (restricted motion) | Move in clusters | Large amounts of kinetic energy |
| Forces of Attraction | Very strong | Moderate | Weak |
PROPERTIES OF GAS
Describing Gases
- Gases are characterized based on four properties:
- Pressure (P)
- Definition: The force exerted by gas against the walls of its container.
- Units: atmosphere (atm), mm Hg, torr, pascal.
- Volume (V)
- Definition: The space occupied by the gas.
- Units: liter (L), milliliter (mL).
- Temperature (T)
- Definition: Determines the kinetic energy and rate of motion of gas particles.
- Units: Celsius (°C), Kelvin (K).
- Amount (n)
- Definition: The quantity of gas present in a container.
- Units: grams (g), moles (n, required in calculations).
GAS LAWS
Boyle’s Law (BeT)
- Formula: At a fixed mass of gas at a constant temperature, the pressure (P) is inversely proportional to the volume (V).
- Equation: P imes V = ext{constant}
- Derived formula: P_1V_1 = P_2V_2
Examples Illustrating Boyle's Law:
- A sample of oxygen gas has:
- Volume, V_1 = 225 ext{ mL} at pressure, P_1 = 1.12 ext{ atm}.
- To find volume at pressure P_2 = 0.98 ext{ atm}:
- Use: P_1V_1 = P_2V_2.
- Calculation: V_2 = rac{P_1V_1}{P_2} = rac{1.12 imes 225}{0.98} = 257.14 ext{ mL}.
- A gas with:
- Volume, V_1 = 1 ext{ L} and pressure, P_1 = 400 ext{ kPa} is transferred to a volume, V_2 = 3 ext{ L}:
- Calculation: P_2 = rac{P_1V_1}{V_2} = rac{400 imes 1}{3} = 133.33 ext{ kPa}.
Charles’ Law (CeP)
- Formula: At a fixed mass of gas at a constant pressure, the volume (V) is directly proportional to the temperature (T).
- Equation: rac{V_1}{T_1} = rac{V_2}{T_2}.
- Remember to convert temperatures to Kelvin:
- T(K) = T(°C) + 273.
Examples Illustrating Charles’ Law:
- Volume of gas at 20 °C (293 K) is 600 mL, find volume at 60 °C (333 K):
- Calculation: V_2 = rac{V_1 imes T_2}{T_1} = rac{600 imes 333}{293} = 681.9 ext{ mL}.
- Weather balloon:
- Initial conditions: V_1 = 5000 ext{ cm}^3, T_1 = 32°C (305 K); find temperature when volume is V_2 = 4400 ext{ cm}^3:
- Calculate: T_2 = rac{V_2 imes T_1}{V_1} = rac{4400 imes 305}{5000} = 268.4 K (-4.6 °C).
Pressure Law
- Formula: At a constant volume, the pressure (P) is directly proportional to the temperature (T).
Combined Gas Law
- Formulation: rac{P_1V_1}{T_1} = rac{P_2V_2}{T_2}.
Examples Illustrating Combined Gas Law:
- A gas has volume of 800.0 mL at -23.0 °C and pressure of 300.0 torr; find its volume at 227.0 °C and 600.0 torr:
- Use: V_2 = rac{P_1V_1T_2}{P_2T_1}.
- Calculation results: Should lead to recalculating volume.
- Balloon initially in a freezer:
- Initial volume 9.40 L, pressure 0.939 atm, need to find initial temperature for volume 10.0 L at pressure 1.00 atm:
- T_1 = rac{P_2V_2T_1}{P_1V_1}
- Results yield: T_1 = 263 K.
IDEAL GASES
Assumptions of Ideal Gases (VMIKE)
- Volume: The volume of individual gas molecules is negligible compared to the total volume.
- Motion: Molecules are in constant, random motion.
- Interatomic Forces: Negligible forces between molecules except during collisions.
- Kinetic Energy: Average kinetic energy depends only on temperature.
- Elastic Collisions: Collisions of gas particles with container walls are perfectly elastic.
Real Gases vs. Ideal Gases
| Real Gases | Ideal Gases |
|---|
| Volume | ✓ | |
| Motion | | ✓ |
| Interatomic Forces | ✓ | |
| Kinetic Energy | | ✓ |
| Elastic Collisions | | ✓ |
Conditions Where Real Gases Behave Like Ideal
- High Temperatures and Low Pressures:
- At high temperatures, particles possess more kinetic energy and move faster.
- At low pressures, particles are further apart, weakening interatomic forces.
Conditions Where Real Gases Deviate From Ideal
- Low Temperatures and High Pressures:
- At low temperatures, particles have less kinetic energy, moving slower.
- At high pressures, particles are closer together, strengthening interatomic forces.
Ideal Gas Equation
- Formulation: PV = nRT
- Where:
- P = pressure (Pa)
- V = volume (m³)
- n = number of moles
- R = gas constant (8.31 J K⁻¹ mol⁻¹)
- T = temperature (K)
Conversions and Applications
- Moles: n = rac{m}{M_r}
- Substituting into ideal gas equation:
- For pressure in kPa, volume must be in