Unit 3: Properties of Substances and Mixtures

Ideal Gas Law, Kinetic Molecular Theory, and Deviations (3.4, 3.5, 3.6)

Welcome to one of the most mathematical but rewarding parts of AP Chemistry! While solids and liquids are stuck close together, gas particles are the "free spirits" of the chemical world. They fly around, bounce off walls, and follow a surprisingly simple set of rules. In this chapter, we will learn how to predict gas behavior using math, understand what’s happening at the particle level, and discover why real gases don't always behave perfectly.


3.4 The Ideal Gas Law

The Ideal Gas Law is a mathematical "master equation" that relates the four main physical properties of a gas: Pressure (\( P \)), Volume (\( V \)), Amount in moles (\( n \)), and Temperature (\( T \)).

The Master Equation

\( PV = nRT \)

  • \( P \): Pressure (usually in \( \text{atm} \), \( \text{torr} \), or \( \text{mmHg} \))
  • \( V \): Volume (must be in \( \text{L} \) for the standard constant)
  • \( n \): Moles (the amount of gas)
  • \( R \): The Universal Gas Constant (check your formula sheet!)
    • \( R = 0.08206 \text{ L atm mol}^{-1} \text{ K}^{-1} \)
    • \( R = 62.36 \text{ L torr mol}^{-1} \text{ K}^{-1} \)
  • \( T \): Temperature (MUST ALWAYS BE IN KELVIN! \( K = ^\circ\text{C} + 273.15 \))

Quick Review: STP
Standard Temperature and Pressure (STP) is defined as \( 273.15 \text{ K} \) and \( 1.0 \text{ atm} \). At STP, one mole of any ideal gas occupies exactly \( 22.4 \text{ L} \). This is a great shortcut for calculations!

Dalton’s Law of Partial Pressures

If you have a mixture of gases, they don't get in each other's way. The total pressure is just the sum of the pressures each gas would exert if it were alone.

\( P_{total} = P_1 + P_2 + P_3 + ... \)

Mole Fraction (\( X \)): This represents the ratio of moles of one gas to the total moles.
\( X_i = \frac{n_i}{n_{total}} \)

You can find the partial pressure of a specific gas by multiplying its mole fraction by the total pressure:
\( P_i = X_i \times P_{total} \)

Analogy: If a pizza has 8 slices and 2 are pepperoni, the "pepperoni fraction" is \( 2/8 \) or \( 0.25 \). If the whole pizza costs \$20, the "partial cost" of the pepperoni slices is \( 0.25 \times \$20 = \$5 \). Partial pressure works the same way!

Key Takeaway: When solving gas law problems, always check your units first—especially Temperature. If it's not in Kelvin, the math won't work!


3.5 Kinetic Molecular Theory (KMT)

If the Ideal Gas Law is the math, KMT is the logic behind it. KMT explains how individual particles behave to create the pressure and temperature we measure.

The 4 Main Assumptions of KMT

  1. Random Motion: Particles are in continuous, random, straight-line motion.
  2. Negligible Volume: The actual gas particles are so small compared to the empty space between them that their individual volume is assumed to be zero.
  3. No Forces: There are no attractive or repulsive forces between particles (no "stickiness").
  4. Elastic Collisions: When particles hit each other or the walls, they don't lose energy; they just bounce off.

Temperature and Kinetic Energy

Temperature is just a measure of the average kinetic energy of the particles.
\( KE_{avg} = \frac{3}{2} RT \)

Important Note: If two different gases (like \( \text{He} \) and \( \text{Ar} \)) are at the same temperature, they have the same average kinetic energy. However, because \( \text{Ar} \) is heavier, its particles must move slower than the light \( \text{He} \) particles to have that same energy.

Maxwell-Boltzmann Distributions

This is a graph that shows the distribution of speeds for gas particles.
Think of it like a "speed trap" on a highway: most cars go the speed limit, some go very slow, and a few go very fast.

  • As Temperature Increases: The curve flattens out and shifts to the right. More particles move at higher speeds.
  • As Molar Mass Increases: Heavier gases move slower. Their curve is tall and skinny on the left side of the graph. Lighter gases move faster and have a flatter curve to the right.

Key Takeaway: Higher temperature = higher average speed. Higher mass = lower average speed (at the same temp).


3.6 Deviations from Ideal Gas Law

In the real world, gases aren't always "ideal." They start to act "weird" (non-ideal) under two specific conditions: High Pressure and Low Temperature.

1. The "Crowded Room" Effect (High Pressure)

At very high pressures, the gas particles are shoved close together. Remember how KMT said particle volume is negligible? At high pressure, this is no longer true! The particles take up a significant portion of the container's volume.
Result: The actual volume of a real gas is often larger than the Ideal Gas Law predicts.

2. The "Sticky Particle" Effect (Low Temperature)

At low temperatures, particles slow down. When they pass each other, the Intermolecular Forces (IMFs) (which we learned about in Topic 3.1) actually start to matter. The particles "cling" to each other slightly instead of bouncing off perfectly.
Result: Because particles are "clinging" together, they hit the walls of the container less often and with less force. The actual pressure is lower than predicted.

Which gases deviate the most?

  • Stronger IMFs: Gases with strong attractions (like polar molecules or large molecules with high London Dispersion Forces) deviate more than small, nonpolar atoms like \( \text{He} \).
  • Larger Size: Larger atoms/molecules deviate more because they take up more space (volume).

Quick Review Box: Non-Ideal Behavior
Gases act MOST IDEAL at: High Temperature and Low Pressure.
Gases act LEAST IDEAL at: Low Temperature and High Pressure.
Memory Trick: To be "Ideal," a gas needs to be "HOT and LONELY" (High Temp, Low Pressure).

Key Takeaway: Real gases deviate from ideal behavior because real particles do have volume and do attract each other.


Common Mistakes to Avoid

  • Units: Forgetting to convert \( ^\circ\text{C} \) to \( \text{K} \). This is the #1 error on the AP exam!
  • Gas Constant (\( R \)): Using the wrong \( R \) value. Match the units of your pressure (\( \text{atm} \) vs \( \text{torr} \)) to the \( R \) on your equation sheet.
  • Average KE vs Speed: Remembering that different gases at the same Temperature have the same Kinetic Energy, but NOT the same Speed.
  • Deviation Logic: Thinking that high pressure makes a gas more ideal. It's the opposite! High pressure makes it crowded and non-ideal.

Don't worry if the Maxwell-Boltzmann graphs look confusing at first—just remember that the area under the curve represents the total number of particles, which stays constant. If the peak moves right, it must also get shorter!