Zumdahl • Zumdahl • DeCoste World of CHEMISTRY Chapter 10 Energy 10.1 The Nature of Energy • Objective: To understand the general properties of energy Copyright © Houghton Mifflin Company 10-3 10.1 The Nature of Energy • Energy • The ability to do work or produce heat • Potential Energy • Energy due to position or composition • Movement of water from high to low to do work • Attractive and repulsive forces used to drive a chemical reaction • Example – combustion of gasoline • Kinetic Energy • Energy do to the motion of the object Copyright © Houghton Mifflin Company 10-4 Law of Conservation of Energy • Energy can be converted from one form to another but can neither be created or destroyed. • Energy on the universe is constant Copyright © Houghton Mifflin Company 10-5 Work • Work • Force acting over a distance • Example: a ball rolling down hill. Copyright © Houghton Mifflin Company 10-6 What happens if we change the surface of our hill? 1. Does ball A lose more energy? 2. What changes? 1. The amount of heat released 2. The amount of force (work) applied 3. Regardless of the amount of heat or work the energy change is constant. Copyright © Houghton Mifflin Company 10-7 . • The change in Energy is independent of it pathway. • Work and Heat are dependent of its pathway. Copyright © Houghton Mifflin Company 10-8 State Function • A State Function is a property of the system that changes independently of its pathways (heat and work are not state functions, they are dependent upon the pathway in which the reaction proceeds). • Example of State Function • Displacement; Energy change Copyright © Houghton Mifflin Company 10-9 10.2 Temperature and Heat Objective: To understand the concept of Temperature and Heat Copyright © Houghton Mifflin Company 10-10 What does temperature of a substance tell us about that substance? • Temperature is • a measure of the random motion of the components of a substance. • Example: Ice →liquid H2O →gaseous H2O • Heat can be defined as • a measure of the random motion of the components of a substance. • . Copyright © Houghton Mifflin Company 10-11 Figure 10.2: Equal masses of hot and cold water. Suppose we place 1.00 Kg hot water next to 1.00 Kg of cold water in an insulated box. What do you expect to happen? Assuming no energy is lost to the air how can we determine the final temp. of the two samples? Copyright © Houghton Mifflin Company 10-12 Figure 10.3: H2O molecules in hot and cold water. Copyright © Houghton Mifflin Company 10-13 • Remembering that heat is the measure of energy flow do to temperature difference: Tfinal = Thot initial + Tcold initial = 90° C + 10°C = 50 2 2 Copyright © Houghton Mifflin Company 10-14 Figure 10.4: H2O molecules in same temperature water. Copyright © Houghton Mifflin Company 10-15 Review • Temperature • the measure of the random motions of the components • Heat • the flow of energy due to temperature differences • Thermal Energy of an object • The random motions of the components of the object Copyright © Houghton Mifflin Company 10-16 10.3 Exothermic and Endothermic Objective: To consider the direction of energy flow as heat Copyright © Houghton Mifflin Company 10-17 What are the energy changed that accompany chemical reactions? • When a process results in the evolution of heat, it is said to be • Exothermic: energy flows OUT of a system • When a process results absorbs energy from its surrounding it is said to be • Endothermic • When heat flows into a system it is said to be endothermic Copyright © Houghton Mifflin Company 10-18 Key Terms • System • The portion of the universe that we single out to study • Surroundings • The surroundings include everything else in the universe. Copyright © Houghton Mifflin Company 10-19 Endothermic Reactions • Example: Boiling water to form steam • Where does the energy (absorbed as heat) come from in an endothermic reaction? • The energy is the difference between the potential energy between the reactants and the products Copyright © Houghton Mifflin Company 10-20 If energy can neither be created or destroyed, where does the change in energy come from? • In an Endothermic Reactions: • The energy gained by a system must equal the energy lost by the surroundings. • In an Exothermic Reaction: • the energy lost by a system must equal the energy gained by the surroundings Copyright © Houghton Mifflin Company 10-21 Examples: Endothermic or Exothermic? 1. Your hands get cold when you touch ice? Exothermic 2. Ice melts when you touch it. Endothermic 3. Ice cream melts Endothermic 4. Propane is burning in a propane torch Exothermic Copyright © Houghton Mifflin Company 10-22 5. Water drops on your skin evaporates Endothermic 6. Two chemicals mixed in a beaker give off heat. Exothermic Copyright © Houghton Mifflin Company 10-23 Figure 10.5: The energy changes accompanying the burning of a match. Copyright © Houghton Mifflin Company 10-24 Focus Questions 1. Explain why energy is a state function, but heat and work are not. 2. What is probably the most important characteristic of energy? 3. What is the difference between temperature and heat? 1. Heat is the flow of energy due to temp. difference. 2. Temperature is the measurement of random motion Copyright © Houghton Mifflin Company 10-25 10.4 Thermodynamics Objective: To understand how energy flow affects internal energy Copyright © Houghton Mifflin Company 10-26 First Law of Thermodynamics • The energy of the universe is constant • The internal energy, E, of a system can be defined as the sum of the kinetic and potential energies of all particles in the system. Copyright © Houghton Mifflin Company 10-27 ∆ E=q+w ∆ (delta) means a change in the function that follows q represents heat w represents work E represent the internal energy Copyright © Houghton Mifflin Company 10-28 Thermodynamic Quantities Consist of 2 Parts 1. A number giving the magnitude of the change 2. Sign indicating the direction of the flow of energy The sign represents the systems point of view + indicated energy flows into a system - indicates energy flows out of a system Copyright © Houghton Mifflin Company 10-29 Common Units of Energy • Calorie (metric unit) • The amount of energy (heat) required to raise the temperature of one gram of water by one Celsius degree • Joule (an SI unit) • 1 calorie = 4.184 joules • 1 cal = 4.184 J Copyright © Houghton Mifflin Company 10-30 • If 1 cal/4.184 J is required to change 1.0g of water by 1° C we can assume that it will take twice as much energy to change 2 g of water by 1 ° C How much energy (heat) in joules is required to raise the temperature of 7.40 gram of water from 29 ° C to 46 ° C ? Copyright © Houghton Mifflin Company 10-31 10.5 Measuring Energy Changes Objective: To understand how heat is measured Copyright © Houghton Mifflin Company 10-32 Conversion between calories and joules • Express 60.1 cal of energy in units of joules 60.1 cal X 4.184 J = 251 J 1cal How many calories of energy correspond to 28.4 J? 28.4J X 1 cal = 6.67 cal 4.184 J Copyright © Houghton Mifflin Company 10-33 Specific Heat Capacity • The amount of energy required to change the temperature of one gram of a substance by one Celsius degree. Copyright © Houghton Mifflin Company 10-34 The Energy (heat) Required to change the temperature of a substance depends on: 1. The amount of substance being heated (number of grams). 2. The temperature change (number of degrees) *Note: different substance behave differently to being heated. Some substances require large amounts of energy to change temperature , whereas others require less. 10-35 Calculations Involving Specific Heat Capacity pg. 298 1. What quantity in joules is required to heat a piece of iron weighing 1.3 g from 25°C to 46°C? 1. What is the answer in calories? 2. A 5.63 sample of solid gold is heated from 21°C to 32°C. How much energy in joules is required? Copyright © Houghton Mifflin Company 10-36 Q=sXmX∆T • • • • Q = Energy required S = specific heat of capacity M = mass in grams ∆ T = change in temperature Copyright © Houghton Mifflin Company 10-37 Quiz 10.1 – 10.3 1. The portion of the universe that we single out to study is known as:__________ 2. A measure of the random motion of the components of a substance is known as_____ 3. Explain why energy is a state function, but heat and work are not. 4. The flow of energy due to temperature differences is known as___________. 5. __________is the ability to do work or produce heat Copyright © Houghton Mifflin Company 10-38 10.6 Thermochemistry (Enthalpy) Objective: To consider the heat (enthalpy) of chemical reactions Copyright © Houghton Mifflin Company 10-39 Enthalpy • At constant pressure, the change in enthalpy (∆ H) is equal to the energy that flows as heat. • ∆ Hp= heat • Where “p” indicates that the process occurred under conditions of constant pressure. Copyright © Houghton Mifflin Company 10-40 Practice problem pg 302 • When 1 mol of methane is burned at constant pressure, 890 kJ of energy is released as heat. Calculate the ∆ H for a process in which 5.8 grams sample of methane is burned at constant pressure. Copyright © Houghton Mifflin Company 10-41 Calorimeter • A calorimeter is a device used to determine the heat associated with a chemical reaction. Copyright © Houghton Mifflin Company 10-42 Figure 10.6: A coffee-cup calorimeter. Copyright © Houghton Mifflin Company 10-43 10.7 Hess’s Law Objective: To understand Hess’s Law Copyright © Houghton Mifflin Company 10-44 Enthalpy is a state function • The change in enthalpy for a given process is independent of the pathway for the process • In going from a particular set of reactants to products the change in enthalpy is the same whether the reaction takes place in one step or in a series of steps. Copyright © Houghton Mifflin Company 10-45 Characteristics of Enthalpy Changes 1. If a reaction is reversed, the sign of ∆ H is also reversed. 2. The magnitude of ∆ H is proportional to the quantities of reactants and products in the reaction. If the coefficients in a balanced reaction are multiplied by an integer, then the value of ∆ H must also be multiplied by the same inetger. Copyright © Houghton Mifflin Company 10-46 1. If enthalpy is the heat for a reaction, it must have a sign as well as a magnitude. What sign for an exothermic reaction have? Why? 2. Suppose you ran a chemical reaction in a calorimeter. If the temperature of the solution goes from 27 °C to 36°C for a 5.0g sample, how would you determine the energy produced by the reaction? 3.What is Hess’s Law and why is it useful? Copyright © Houghton Mifflin Company 10-47 4. The enthalpy of a combustion of solid carbon to form carbon dioxide is -393.7 kJ/mol °C, and the enthalpy of combustion of carbon monoxide to form carbon dioxide is -283.3 kJ/mol °C. Using this data, calculate the change in enthalpy for the reaction: 2C(s) + O2 (g) → 2 CO (g) Copyright © Houghton Mifflin Company 10-48 10.8 Quality Versus Quantity of Energy Objective: To see how the quantity changes as it is used Copyright © Houghton Mifflin Company 10-49 If energy is conserved, why are we concerned about having enough energy to use? • Suppose we drive from Evansville to Indianapolis – we put gas in our car to do work. • The energy in the bonds react with oxygen (combust – bond are broken) and energy is released to do work. • During this process we release energy in the form of heat (i.e. the quantity of heat is transferred , thus conserved). Copyright © Houghton Mifflin Company 10-50 What happens to the quality of the energy? C8H18(l) + O2(g) → CO2 (g) + H2O (g) + energy • Which energy is easier to use? • When we utilize energy to do work we degrade its usefulness (quality). Copyright © Houghton Mifflin Company 10-51 “heat death” of the Universe • Eventually all energy of the universe will be spread out evenly throughout the universe and everything will be the same temperature – at this point the energy will no longer be able to do work. • The Universe will be ‘dead’ Copyright © Houghton Mifflin Company 10-52 10.9 Energy and Our World Objective: To consider the energy resources of our world Copyright © Houghton Mifflin Company 10-53 Where does our energy ultimately come from? • By the process of photosynthesis plants store energy which then can be converted over millions of years to fossil fuels. Copyright © Houghton Mifflin Company 10-54 Figure 10.7: Energy sources used in the United States. Copyright © Houghton Mifflin Company 10-55 Petroleum and Natural Gas • Petroleum and Natural gas is most likely formed from the remains of marine organism that lived more than 500 million years ago • Petroleum is a thick dark liquid composed of hydrocarbons. • Natural Gas consist mostly of methane Copyright © Houghton Mifflin Company 10-56 Coal • Coal is formed from the remains of plants that were buried and subjected to high pressure and heat over long periods of time. • The energy available from the combustion of coal depends upon the grade of coal. The more carbon in the coal the higher the energy yield. Copyright © Houghton Mifflin Company 10-57 Coal supplies 20% of our energy in the US What are the problems associated with coal? 1. expensive and dangerous to mine 2. Strip mining of fertile farmland 3. Burning of coal released Sulfur Dioxide. 4. Combustion of coal releases high levels of carbon dioxide, which in turns effects the earths temperature. Copyright © Houghton Mifflin Company 10-58 Figure 10.8: The earth’s atmosphere. Copyright © Houghton Mifflin Company 10-59 Effects of Carbon Dioxide on Climate The Greenhouse Effect • The temperature of the earth is controlled to a significant extend by the CO2 and H2O content of the atmosphere. Connection: What happened when the production of heat when the moisture in the earths atmosphere increases (humidity)? Copyright © Houghton Mifflin Company 10-60 Figure 10.9: The atmospheric CO2 concentration over the past 1000 years. Copyright © Houghton Mifflin Company 10-61 New Energy Sources • • • • • Solar Nuclear Wind Biomass Synthetic fuels Copyright © Houghton Mifflin Company 10-62 10.10 Energy as a Driving Force Objective: To understand energy as a driving force for natural processes Copyright © Houghton Mifflin Company 10-63 Why do thing occur? Why do some reactions in nature proceed in a particular direction? Wood + O2(g) → CO2 (g) + H2) (g) + energy + ashes Why doesn’t the reverse happen? Copyright © Houghton Mifflin Company 10-64 2 Factors That are important to Driving Forces • Energy Spread • Matter Spread Copyright © Houghton Mifflin Company 10-65 Energy Spread • Energy Spread means that in a given process, concentrated energy is dispersed widely. • This distribution always happens every time an exothermic reaction occurs. • The energy that flows into the surroundings through heat increases the thermal motions of the molecules in the surroundings. Copyright © Houghton Mifflin Company 10-66 Matter Spread • Matter spread says that molecules of a substance are spread out and occupy a large volume. Copyright © Houghton Mifflin Company 10-67 Entropy • Entropy (S) is the natural tendency of the world to become disordered. • As randomness increases, S increases. Copyright © Houghton Mifflin Company 10-68 Figure 10.10: Comparing the entropies of ice and steam. Which has Greater entropy? Ice or steam? Copyright © Houghton Mifflin Company 10-69 What happens to the disorder of the universe as energy spread and matter spread occur during a reaction? • ENERGY SPREAD→ Faster random motions of the molecules in surroundings • MATTER SPREAD → Components of matter are dispersed – they occupy a larger volume. Copyright © Houghton Mifflin Company 10-70 1. If energy is conserved, how can there be an “energy crisis” 2. What is “cracking” of petroleum products? How did it help increase production of gasoline? 3. What is the greenhouse effect and what are the key molecules that cause it? 4. What driving force must be predominant for an endothermic reaction to occur? Why? Copyright © Houghton Mifflin Company 10-71