Presentation is loading. Please wait.

Presentation is loading. Please wait.

Mixtures of Gases Dalton's law of partial pressure states: –the total pressure of a mixture of gases is equal to the sum of the partial pressures of the.

Similar presentations


Presentation on theme: "Mixtures of Gases Dalton's law of partial pressure states: –the total pressure of a mixture of gases is equal to the sum of the partial pressures of the."— Presentation transcript:

1

2 Mixtures of Gases Dalton's law of partial pressure states: –the total pressure of a mixture of gases is equal to the sum of the partial pressures of the component gases.

3 Dalton's Law of Partial Pressure P T = P 1 + P 2 + P 3 + …….

4 Partial Pressure in terms of mole fraction OR X A P total = P A (X A = mole fraction of A and P A = partial pressure of gas A)

5 Mole fraction What is the mole Fraction of Gas A in mixture I? What is the mole fraction of Gas B in mixture II?

6 Example: If there are 3 moles of gas A, 4 moles of gas B and 5 moles of gas C in a mixture of gases and the pressure of A is found to be 2.5 atm, what is the total pressure of the sample of gases? X A = 3= 0.2 3+4+5 P A = 2.5 atm P T = P A / X A = 2.5/0.2 = 12.5 atm

7 2KClO 3 (s) 2KCl (s) + 3O 2 (g) Bottle full of oxygen gas and water vapor P T = P O + P H O 22

8 Graham’s Law of Diffusion Graham’s law states that the rates of effusion of two gases are inversely proportional to the square roots of their molar masses at the same temperature and pressure:

9 Graham’s Law of Effusion The velocity of effusion is also inversely proportional to the molar masses:

10 Graham’s Law of Diffusion But the time required for effusion to take is directly proportional to the molar masses: The density of the gas is also directly proportional to the molar masses:

11 Kinetic Molecular Theory Deductions Postulates Evidence/deduction 1. Gases are tiny molecules in mostly empty space. The compressibility of gases. 2. There are no attractive forces between molecules. Gases do not clump. 3. The molecules move in constant, rapid, random, straight-line motion. Gases mix rapidly. 4. The molecules collide classically with container walls and one another. Gases exert pressure that does not diminish over time. 5. The average kinetic energy of the molecules is proportional to the Kelvin temperature of the sample. Charles’ Law

12 Graham’s Law of Diffusion Compare the rate of effusion for hydrogen and oxygen gases.

13 Deviations from Ideal Behavior of Gases Deviation from ideal behavior is large at high pressure and low temperature At lower pressures and high temperatures, the deviation from ideal behavior is typically small, and the ideal gas law can be used to predict behavior with little error.

14 Deviation from ideal behavior as a function of temperature As temperature is decreased below a critical value, the deviation from ideal gas behavior becomes severe, because the gas CONDENSES to become a LIQUID.

15 J. D. van der Waals corrected the ideal gas equation in a simple, but useful, way (a) In an ideal gas, molecules would travel in straight lines. (b) In a real gas, the paths would curve due to the attractions between molecules.

16 Real Gases No such thing as an ideal gas Real gases begin to behave like ideal gases under ideal conditions. –at low pressures –At high temperatures

17 Real Gases Look at real gas behavior –Graph of PV/nRT vs P –For ideal gases, PV / nRT = 1 at any pressure –For real gases, PV / nRT approaches 1 at very low pressures (below 1 atm)

18 Real Gases What is the effect of temperature when plotting PV / nRT vs. P? –PV / nRT approaches 1 at low pressure and at high temperatures

19 Real Gases Johannes van Der Waals –Developed an equation for real gases –Received a Nobel prize for his work

20 Ideal Gases vs. Real Gases Volumeless Do not interact with each other Finite volumes Particles do take up space Volume of the gas is actually less than the volume of the container Particles do attract each other

21 van der Waals Equation Correction factors for the ideal gas law Correct for the volume: –The actual volume of a real gas is V – nb V = volume of the container n = # moles of gas particles b = constant, determined using experimental results

22 van der Waals Equation Correction factors for the ideal gas law Correct for the attractive forces between particles –Attractive forces would result in fewer, as well as slightly weaker collisions, resulting in less pressure.

23 van der Waals Equation P obs = observed pressure P’ = pressure expected from the ideal gas law P obs = P’ – correction factor

24 van der Waals Equation The correction factor for the attractive forces would also have to be experimentally determined. Depends on –concentration of gas molecules (moles/liter or n/V) more gas molecules, more interactions Correction factor: a(n/V) 2 –a = proportionality constant

25 van der Waals Equation P obs = nRT – a (n/V) 2 V – nb Rearrange to get van der Waals equation: [P obs + a(n/V) 2 ] x (V – nb) = nRT ( P corrected. V corrected = nRT)

26 van der Waals Equation A real gas becomes more like an ideal gas at low pressure… –Low pressure implies a large volume for the gas particles…the volume of the gas becomes the volume of the container as the gas particles (nb becomes very small) get farther apart –note that b is smaller when gas particles are smaller (b for He is 0.0237 L/mol while b for Xe is 0.0511 L/mol)

27 van der Waals Equation A real gas becomes more like an ideal gas at high temperature… High temperature means the gas particles have high kinetic energy and are moving past each other with greater speeds, giving the particles less of a chance to feel any attractive force. P obs approaches P ideal

28 Real Gases and Ideal Gases In summary, a real gas approaches the behavior of an ideal gas –at low pressure (large container) –at high temperature –when the gas experiences few attractive forces (the more nonpolar the particle, the weaker the attractive forces)


Download ppt "Mixtures of Gases Dalton's law of partial pressure states: –the total pressure of a mixture of gases is equal to the sum of the partial pressures of the."

Similar presentations


Ads by Google