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Gas Laws. Part 1: Kinetic Theory (most of this should be review)

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Presentation on theme: "Gas Laws. Part 1: Kinetic Theory (most of this should be review)"— Presentation transcript:

1 Gas Laws

2 Part 1: Kinetic Theory (most of this should be review)

3 Kinetic Theory of Matter  All matter is moving.  Kinetic Energy is the energy of motion.  Temperature is a measure of Kinetic Energy.  Higher temperature indicates more motion.  Motion stops at 0 K (-273˚C)

4 Kinetics of Phases  Solids the particles have strong Inter- molecular forces (IMF) with each other but vibrate in place.  Liquids have some IMF but can change position relative to each other.  Gases have very low IMF and have very little interaction with one another.

5 So...  Solids have a definite shape and volume.  Liquids have definite volume but not definite shape (take the shape of their container)  Gases have no definite shape or volume (expand to fill size and shape of container).

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7 Temperature  Measure of the average kinetic energy.  Some particles can be moving very fast.  Some will move very slowly.  Most are average.

8 Vapor Liquid Equilibrium  Stoppered flask, particles cannot escape.  Open beaker they can – eventually will evaporate.

9 Part II: Properties of Gases

10 Air Pressure is Due to Gravity  Remember STP?  Standard Air Pressure is measured at Sea Level: 101.3KPa

11 Compressibility  Gas molecules are very small  The spaces between them are very large  The molecules can be forced closer together  They can absorb a lot of energy  E.g. car air bags

12 Intermolecular Forces  The molecules are randomly moving very fast  They move in straight-line paths  Only change direction when they bump into something  The molecules are SO far apart that the IMF are considered to be zero

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14 Variables in the Gas Formulas  P = pressure in kilopascals (kPa)  V = volume of the gas in litres (L)  T = temperature in kelvins (K)  n = number of moles

15 Δ Moles, Δ Pressure  Volume remains constant  Temperature remains constant  Doubling the number of gas particles (moles) doubles the pressure

16 Δ Volume, Δ Pressure  Temperature remains constant  Number of particles (moles) remains constant  Decreasing the volume by half will double the pressure

17 Δ Temperature, Δ Pressure  Volume remains constant.  Number of moles remains constant  Doubling the temperature will double the pressure

18 Part III: Gas Laws

19 Boyle’s Law  Temperature remains constant  Pressure goes up, volume goes down  Pressure goes down volume goes up

20 Inverse relationship creates a curve, not a line…

21 Charles’s Law  Pressure is constant  Temperature goes up, volume goes up  Temperature goes down, volume goes down.

22 The Mylar Balloon on a cold day…  Demo

23 Gay-Lussac’s Law  Volume is constant  Temperature increases, pressure increases  Temperature decreases, pressure decreases.

24 Ideal Gas Law  PV=nRT where R is the gas law constant 8.31 L kPa Ideal Gases  Follow the law precisely  The particles must have no volume  Must have no IMF  No ideal gases exist

25 Guess where we find this…

26 The most ideal gases are H 2 and He

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