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Gases: Kinetic Molecular Theory, Ideal and Real Gases

Explore the properties and behaviors of gases in this chapter. Learn about the Kinetic Molecular Theory, ideal and real gases, as well as the greenhouse effect and the ozone layer. Discover Pascal's Principle, pressure units, and the gas constant. Dive into the laws of Charles, Boyle, and Avogadro to understand the ideal gas law.

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Gases: Kinetic Molecular Theory, Ideal and Real Gases

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  1. Chapter 10: Page 300-330 Chapter 11: Page 332-359 Chapter 10 & 11: Gases Chlorine gas was used as a weapon in WWI

  2. Kinetic Molecular Theory • all matter is made up of particles (atoms) in random and constant motion. (colliding) • Gases have very low density • particles are spaced far apart. • Gases are compressible. • Extreme pressures-gases will compress until they become liquids (or solids, CO2). • Adding heat to a system • increases the temperature … • Temperature = measure of the average kinetic energy of the particles. • Increasing the pressure of a gas, • increases the density of the gas - the number of particles in a given space.

  3. Ideal and Real Gases Ideal gasses • Ideal Gas: • Imaginary, perfect gas – makes calculations easier • Real Gas: • Gas that actually behaves in reality… • When compressed, real gases will form liquids, and even exhibit liquid-like behaviors when still in gas form. • Real gas molecules interact with each other -causing them to travel in non-linear paths and collide “inelastically.” • With real gases, the size of the gas molecules effects their behavior. Real Gasses 

  4. Gases in our atmosphere • Nitrogen-78% • Oxygen-21% • Argon-<1% • Trace amounts of CO2, Ne, He, CH4, Kr, H2, O3, and others. • Some gases function as greenhouse gases, and work to hold heat on the earth’s surface. • Some gases function to block harmful UV radiation energy from the sun.

  5. The Greenhouse Effect • The sun’s energy travels through space and warms the surface of the earth. • Some of the energy is reflected back into space. • Greenhouse Gases • trap heat that would leave the atmosphere. • H2O, CH4, and CO2 are common greenhouse gases. • “Global Warming” • Theory that increasing levels of Greenhouse gasses is causing the global average temps to increase.

  6. The Ozone Layer (O3) Page 778 for more info • Ozone is • a corrosive poisonin the Troposphere(where we live) • frequently created and given off from free electrical ionization. • Ozone • Absorbs harmful Ultraviolet (UV) energy in the stratosphere, 11km (6 miles) above us. • Note: the Ozone layer is less than 1mm thick! • It is always moving, like a cloud, due to weather patterns and climate variations.

  7. Pascal’s Principle and Pressure F = Force a = area • French physician, Blaise Pascal, showed that • fluids (including gasses) exert a uniform pressure on all the surfaces that they contact. • Exerting a force on the top surface of a gas, causes that force (pressure) to be exerted on all the walls of its container. • Pressure is due to the particles of a gas striking a surface. We can detect pressure from billions upon billions of gas molecules striking a surface at any point in time.  Which exerts a greater pressure? 

  8. Pressure units… • The SI unit of pressure is the Pascal, Pa, equaling one newton per square meter. • Earth’s air pressure at sea level ~ 100,000 Pa. 100kPa • PSI (US) • Pound per square inch. Atmospheric pressure at sea level is about 14.5 PSI. • mmHg (EU, Asia) (AKA: Torr) • Millimeters of mercury. • Atmospheric pressure is 760 mmHg at sea level. • This has to due with the height of a column of liquid mercury raised in a barometer. • inHg • Inches of mercury. Used only in meteorology. • Atmospheric pressure is apx 30inHg.

  9. And finally… • And, finally…the atmosphere, atm • the pressure exerted by the atmosphere at sea level, at 00C. (This creates STP…) • Standard Temperature and Pressure: • STP • usually used when referring to reactions with gases. STP is defined as: • 1 atm and 273.15 K • 101 kPa and 273.15 K • 760 mmHg and 273.15 K When doing work with gases, select the STP that matches the pressure you are using. (atm in this class)

  10. Charles’ Law Simulation. constant volume • French chemist, Jacque Charles, showed that at constant pressure, • temperature and volume varied proportionally. That is… • V / T=k(k = some constant #) • We tend to write Charles’ Law as the volumes and temperatures under two conditions: c 1780’s

  11. Boyle’s Law We’re leaving one law out… can you guess what it is? • A young, adventurous, British aristocrat named Robert Boyle found that • when temperature is kept constant, volume varies inversely proportional with pressure. That is: • P V = k (constant) • We tend to write Boyle’s Law as the volumes and pressures under two conditions: c 1660’s

  12. Charles’ Law + Boyle’s Law + Avogadro’s Law=THE IDEAL GAS LAW • R is the “gas constant” and numerically depends upon the pressure units used. Pressure Volume (in Liters) Moles Constant Temperature (in Kelvin)

  13. The Gas Constant • The Gas Constant is the numerical bridge between number of moles of a gas, its temperature, and volume or pressure. • R = 8.314 L٠kPa / mol٠K • R = 0.0821 L٠atm / mol٠K • Note that the first constant is in KILO Pascals. When given Pascals, you must first convert to kilopascals. • Our calculations will be done in Atm

  14. Dalton’s Law of Partial Pressures • The total pressure in a system is the sum of the individual pressures exerted by each gas. • So, if gas A exerts a pressure of 2 units, and gas B exerts a pressure of 3 units, the total pressure of a system of equal parts of A and B, would be ? • Total= A + B……..2 + 3 = 5 units. • In our atmosphere, Oxygen is about 21%. If we have a sample of air at 1 atm, what is the pressure due to oxygen?

  15. Graham’s Law of Gas Effusion • Effusion • motion of a gas through an opening in a container. • notDiffusion - dispersing from higher concentration to lower concentration. • Rates (speeds) of effusion are related to the molar mass of a gas. • The higher the molar mass, the slower the gas will effuse. • This is a property of real gases

  16. Graham’s Law of Gas Effusion • At the same temperature… • The higher the molar mass, the slower the gas will effuse. • Graham’s Law of Effusion: Molar mass velocity Molar mass velocity Gas AvsGas B

  17. Vapor Pressure Page 324 • All liquids exert a vapor pressure. • Vapor pressure = liquid’s molecules  gas phase. • Higher temperatures  greater molecular speed  greater vapor pressure. • Morevolatile liquids exert a greater vapor pressure than do less volatile liquids. • Can you explain why this is? • In lab: we collect gasses over water. There is a small amount of water vapor in our gas samples, due to water’s vapor pressure.

  18. Phase Diagrams Example on page 381 • Phase diagrams • predict if a substance will be a solid, liquid or gas • depends upon the pressure and temperature of the substance. • Triple Point • point where solid, liquid, and gas all exist – for water, 00C. Notice, that as you increase pressure, the boiling point of water increases-this is why a pressure cooker works. What about Denver, the “mile-high city?” End of Gases lecture, Chapters 10,11, problems following

  19. In-chapter problems: • Page 327, #5,7,8What is Pressure? • Page 327, #11-14Pressure Units • Page 327, #17-19Pressure Conversions • Page 330, #20-24eBoyle’s Law • Page 330, #25-27Charles’ Law • Page 330, #31-35oCombined Law • Page 331, #39,40Dalton’s Law of Partial Pressures • Page 357, #9-13oAvogadro’s Molar Gasses • Page 358, #17-20Ideal Gas Law • Page 358, #23-29oIdeal Gas Law and Stoichiometry • Page 359, #39-42 Graham’s Law of Gas Effusion End of Gases Unit, Chapters 10,11

  20. CCSD Syllabus Objectives • 11.1: Kinetic Molecular Theory • 11.2: Physical Properties of Gasses • 11.3: STP • 11.4: Volume-Temp relationships • 11.5: Volume-Pressure relationships • 11.6: Density-Volume-Pressure-Temperature • 11.10: Ideal Gas Law • 11.11: Graham’s Law • 11.12: Ideal Gas vs Real Gas • 12.3: Evaporation, Condensation, Sublimation • 21.1: Environmental Chemistry

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