Gas Properties and Gas Laws

1. Gas Properties and Gas Laws

2. 0 Gases may be… • Monoatomic Gas: Made of one atom, like He • Diatomic Gas: Made of two atoms, like Cl2 or H2 • *This is the case for Br, I, N, Cl, H, O, F • Also known as Miss BrINClHOF(Brinklehoff) • Polyatomic Gas: Made up of more than two atoms, like CO2, NO2, or CH4 (methane)

3. 0 Some unique properties of gases: • Gases have mass • It is easy to compress a gas • Gases fill their containers completely • Gases diffuse through each other easily • Gases exert pressure on their surroundings • The pressure of a gas depends on its temperature

4. 0 Gases Behaviors: • Gases are composed of a large number of particles that behave like hard, spherical objects in a state of constant, random motion. • Basically, gas particles are like billiard balls in a 3-D pool table, and they are all moving all over the place all the time in different directions

5. 0 Gas Molecule Movements • These particles move in a straight line until they collide with another particle or the walls of the container. • Then they bounce off, and move again: these collisions are elastic • Gas Molecule Motion

6. 0 Other Things to Consider about Gas Molecule Movement • There is no force of attraction between gas particles or between the particles and the walls of the container. • Keep in mind that things aren’t repelled, either….no attraction, no repulsion…

7. 0 Other Things to Consider about Gas Molecule Movement • Collisions between gas particles or collisions with the walls of the container are perfectly elastic. None of the energy of a gas particle is lost when it collides with another particle or with the walls of the container. • This is why gases take the shape of their container! • The energy of the system is constant as long as the pressure and temperature remain constant.

8. 0 Kinetic Energy and Gas • The average kinetic energy of a collection of gas particles depends on the temperature of the gas and nothing else. • Think back to the fact that temperature is a measure of Kinetic Energy (the random motion of molecules)

9. 0 Gas Volume • These particles are much smaller than the distance between particles. Most of the volume of a gas is therefore empty space. • Compared to the container, the volume of the gas is zero. So, we say the volume of the container is the volume of the gas • The volume of the gas in an empty soda bottle is?

10. 0 Kinetic Molecular Theory of Gases (KMT) • Gases consist of very small particles , each of which has a mass. • The distance separating gas particles is very large so much so that we say the volume of the gas is negligible as compared to the volume of the container (the gas itself has no volume) • Gases exert no force on one another • Gas particles are in random, rapid, constant motion • Collisions with other gas particles or the walls of the container are elastic (no energy lost) • The average KE of a gas depends on the temperature of the gas

11. 0 Measuring Gases We measure gases in several ways… • Volume =V • Temperature =T • Pressure =P • Number of Moles =n

12. What is Temperature? • Temperature is a measure of heat; more specifically it is the (average) measure of the random kinetic energy of the molecules in an object • Kinetic energy: Energy of motion • More motion = More KE = Higher temperatures • Less Motion= Lower KE = Lower temperatures

13. 0 Temperature (T) • For most scientists, the Celsius scale is used • However, we need to use the Kelvin scale for gas laws

14. Why? • Why this strange and bizarre scale that uses a boiling point of 373K and a freezing point of 273K for water? • Well, it’s because our “normal” temperature scales are based upon numbers that make sense to use (or not) • (like freezing at 0°C and boiling at 100 °C) or are a bit more convoluted (like the Fahrenheit scale, where zero comes from the temperature of ice, water and NH4Cl and body temperature was 98 °F and still water with ice was 32 °F. )

15. An Absolute Temperature Scale • The Kelvin scale bases temperature on an absolute scale, where temperatures correspond to the amount of motion of the particles • Absolute zero (O K) is when there is no molecular motion (at all) • Scientists have gotten close to zero K, but not quite there. • It exists naturally in deep space

16. So why do we need to use Kelvin again? • Calculations using temperature of zero could be undefined or have no value (which really can’t be) • Can’t have negative volumes in our equations, because that is impossible (from using negative temperatures values in the variables) • The Kelvin scale avoids all of these issues

17. 0 The Kelvin Scale • Is based in Absolute Zero, which is -273°C • 0K= -273°C • 273K=0°C To convert between K and °C, °C + 273 =K or K -273 = °C It’s that simple, which is good since no gas laws calculations can use °C

18. 0 Volume (V) • We usually measure volume in Liters (L), but sometimes in other metric units 1L = 1000mL 1L = .001m3 We will use these conversions- be sure to know them!

19. 0 Pressure (P) • Gas pressure is created by the molecules of gas hitting the walls of the container. This concept is very important in helping you to understand gas behavior. Keep it solidly in mind. This idea of gas molecules hitting the wall will be used often. • Pressure is force measured over an area P=Force/ area and yes, Physics children, Force = mass (acceleration)

20. 0 Units of Pressure • atmospheres (atm) • millimeters of mercury (mm Hg) • Pascals (= Pa) • kiloPascals (= kPa) • Standard pressure is defined as: 1 atm 1atm =760.0 mm Hg 1 atm=101.325 kPa

21. Measuring Pressure of Gases 0 • Manometers-Measure the pressure of a gas as compared to the outside world

22. 0 Moles (n) • We’ve been here before. Calm down about it. • Remember that 1 mole is 6.02E23 pieces of something- in this case, usually molecules of gas (but sometimes atoms, if not a diatomic gas). • Also, 1 mol gas at STP (Standard Temp/Pressure) = 22.4L • “= “means occupies, takes up, etc

23. 0 Boyle’s Law • Relates pressure and volume, while temperature and number of moles are constant (so they do not appear in the equation)

24. 0 Boyle’s Law: P1V1=P2V2 • In a closed rigid containerof a gas at a constant temperature, the pressure times the volume remains constant (P1V1=k) • Pressure and volume are inversely related • The P1 is the pressure at the first volume (V1), while P2 is the pressure at the second volume (V 2).

25. Boyle’s Law: P1V1=P2V2 0 • The product of pressure and volume remains constant as long as the temperature remains constant. (The number of moles must also remain constant.) Volume Pressure • When volume is high, pressure is low • When the volume is low, pressure is high

26. 0 Using Boyle’s Law • If a balloon with a volume of 3L is under a pressure of 1 atmosphere, determine the new volume if the pressure is changed to .8 atm. • We are given P1,V1, and P2. We are asked to find V2 • Two key words here are new and changed- to ID these measurements as linked (having the same subscript) • What is the new volume?

27. 0 Charles’ Law • Charles’ law relates volume and temperature, at a constant pressure and number of moles in a flexible container. Since the pressure and number of moles are constant, they do not appear in the equation.

28. 0 Charles’ law V1/T1=V2/T2 • In a closed container of a gas at a constant temperature, the pressure times the volume remains constant (P1V1=k) • The P1 is the pressure at the first volume (V1), while P2 is the pressure at the second volume (V 2).

29. 0 Charles’ Law • V1/T1=V2/T2 can be rearranged to read • V1T2=V2T1 • Why would we care to rearrange this? This means no division in the equation. You can use it either way, just remember that they are DIRECTLY PROPORTIONAL.

30. 0 Charles’ Law • As the temperature increases, the volume increases. • As the temperature decreases, the volume decreases. • Temperature and volume are proportionally related.

31. 0 Chuck’s law (still…) • Think again about temperature- it is the KE of the gas particles. • Think about what the volume is a result of: the force that the gas molecules are exerting of the container • Think about how if something hits another thing at a higher speed- it hits with more force. More force is pushing harder. Pushing harder means further. This means greater volume when we are dealing with a flexible container!

32. 0 Gay Lussac’s Law • Relates pressure and temperature, when volume is kept constant (P1/T1=k) • P1/T1= P2/T2 Or • P1T2=P2T1

33. 0 Combined Gas Law (Putting it all together) • (P1V1)/ T1=(P2V2)/T2 • Takes all other gas laws into account, even if you can’t see them here (they cross out of the equation) • When in doubt about most of the guy’s laws, you can use this one, because when the pressure, volume, or temperature is constant, you have the law you need.