Introductory Chemistry: A Foundation, 6th Ed. Introductory Chemistry, 6th Ed. Basic Chemistry, 6th Ed. by Steven S. Zumdahl & Donald J. DeCoste University of Illinois Chapter 10 Energy Energy and Energy Changes • Energy: ability to do work or produce heat – Chemical, mechanical, thermal, electrical, radiant, sound, nuclear – Potential and kinetic • Energy may affect matter. – e.g. Raise its temperature, eventually causing a state change, or cause a chemical change such as decomposition • All physical changes and chemical changes involve energy changes. Copyright © Houghton Mifflin Company. All rights reserved. 10 | 3 Energy and Energy Changes • Potential Energy: energy due to composition or position • Kinetic Energy: energy due to motion – - ½ mv2 Copyright © Houghton Mifflin Company. All rights reserved. 10 | 4 Energy and Energy Changes (cont.) • Law of Conservation of Energy: energy can be converted from one form to another, but cannot be created or destroyed Copyright © Houghton Mifflin Company. All rights reserved. 10 | 5 Work and Energy • Work: force acting over a distance – w=f•d – Work done on a system will increase the energy of the system, whereas work done by the system will decrease the energy of the system • State function: a property that changes independent of pathway Copyright © Houghton Mifflin Company. All rights reserved. 10 | 6 Temperature and Heat • Heat: a flow of energy due to a temperature difference • Temperature: a measure of the random motions of the components of a substance Copyright © Houghton Mifflin Company. All rights reserved. 10 | 7 Temperature and Heat (cont.) Copyright © Houghton Mifflin Company. All rights reserved. 10 | 8 Exothermic vs. Endothermic • System: that part of the universe that we wish to study • Surroundings: everything else in the universe • Exothermic process: is any process that gives off heat – transfers thermal energy from the system to the surroundings. Example: when a match is struck, it is an exothermic process because energy is produced as heat. and 2H2 (g) + O2 (g) 2H2O (l) + energy • Endothermic process: absorbs heat - Example: melting ice to form liquid water is an endothermic process because the ice absorbs heat in order to melt energy + H2O (s) H2O (l) Copyright © Houghton Mifflin Company. All rights reserved. 10 | 9 Exothermic Process Copyright © Houghton Mifflin Company. All rights reserved. 10 | 10 Enthalpy (H) is used to quantify the heat flow into or out of a system in a process that occurs at constant pressure. DH = H (products) – H (reactants) DH = heat given off or absorbed during a reaction at constant pressure Copyright © Houghton Mifflin Company. All rights reserved. 10 | 11 Thermochemical Equations Is DH negative or positive? System absorbs heat Endothermic DH > 0 6.01 kJ are absorbed for every 1 mole of ice that melts at 00C and 1 atm. H2O (s) H2O (l) Copyright © Houghton Mifflin Company. All rights reserved. DH = 6.01 kJ 6.3 10 | 12 Thermochemical Equations • The stoichiometric coefficients always refer to the number of moles of a substance H2O (s) • DH = 6.01 kJ If you reverse a reaction, the sign of DH changes H2O (l) • H2O (l) H2O (s) DH = -6.01 kJ If you multiply both sides of the equation by a factor n, then DH must change by the same factor n. 2H2O (s) 2H2O (l) Copyright © Houghton Mifflin Company. All rights reserved. DH = 2 x 6.01 = 12.0 kJ 10 | 13 Thermochemical Equations • The physical states of all reactants and products must be specified in thermochemical equations. H2O (s) H2O (l) DH = 6.01 kJ H2O (l) H2O (g) DH = 44.0 kJ How much heat is evolved when 266 g of white phosphorus (P4) burn in air? P4 (s) + 5O2 (g) 266 g P4 x P4O10 (s) 1 mol P4 123.9 g P4 x Copyright © Houghton Mifflin Company. All rights reserved. DH = -3013 kJ 3013 kJ = 6470 kJ 1 mol P4 10 | 14 Different enthalpies • Heat of reaction (DHr or DHrxn)- heat energy absorbed or released during a reaction. • Heat of formation (DHf)- heat energy absorbed or released during synthesis of one mole of a compound from its elements at 298 K and 1 atm pressure (STPstandard temp and pressure). • Heat of solution (DHsol)- heat energy absorbed or released when a substance dissolves in a solvent. • Heat of combustion (DHcomb)- heat energy released when a substance reacts with oxygen to form CO2 and H2O. Copyright © Houghton Mifflin Company. All rights reserved. 10 | 15 • Heat of fusion (DHfus)= Energy needed to melt one mole (solid to liquid) • Heat of vaporization (DHvap)=Energy needed to boil one mole (liquid to gas) • In a phase change graph, it is possible to calculate the total energy involved as well as the energy consumed in each step. • Note that water has different values for sp. heat depending upon its physical state. Copyright © Houghton Mifflin Company. All rights reserved. 10 | 16 Thermodynamics • The Law of Conservation of Energy is also known as The First Law of Thermodynamics. It can be stated as “the energy of the universe is constant.” • Internal Energy (E) = kinetic energy + potential energy • ΔE = q + w = change in internal energy q = heat absorbed by the system w = work done on the system Copyright © Houghton Mifflin Company. All rights reserved. 10 | 17 Units of Energy • One calorie = amount of energy needed to raise the temperature of one gram of water by 1°C – kcal = energy needed to raise the temperature of 1000 g of water 1°C • joule – 4.184 J = 1 cal • In nutrition, calories are capitalized. – 1 Cal = 1 kcal Copyright © Houghton Mifflin Company. All rights reserved. 10 | 18 Example - Converting Calories to Joules Convert 60.1 cal to joules. Copyright © Houghton Mifflin Company. All rights reserved. 10 | 19 Energy & Temperature of Matter • The amount the temperature of an object increases depends on the amount of heat added (q). – If you double the added heat energy the temperature will increase twice as much. • The amount the temperature of an object increases when heat is added depends on its mass – If you double the mass it will take twice as much heat energy to raise the temperature the same amount. Copyright © Houghton Mifflin Company. All rights reserved. 10 | 20 Specific Heat Capacity • Specific heat (s): the amount of energy required to raise the temperature of one gram of a substance by one degree Celsius Amount of Heat = Specific Heat x Mass x Temperature Change Q = s x m x DT Copyright © Houghton Mifflin Company. All rights reserved. 10 | 21 Specific Heat Capacity Copyright © Houghton Mifflin Company. All rights reserved. 10 | 22 Example #1: Calculate the amount of heat energy (in joules) needed to raise the temperature of 7.40 g of water from 29.0°C to 46.0°C. Copyright © Houghton Mifflin Company. All rights reserved. 10 | 23 Example #1 (cont.) Specific heat of water = 4.184 J g C Mass = 7.40 g Temperature change = 46.0°C – 29.0°C = 17.0°C Q = s • m • DT Copyright © Houghton Mifflin Company. All rights reserved. 10 | 24 Example #2 A 1.6 g sample of metal that appears to be gold requires 5.8 J to raise the temperature from 23°C to 41°C. Is the metal pure gold? Copyright © Houghton Mifflin Company. All rights reserved. 10 | 25 Example #2 Table 10.1 lists the specific heat of gold as 0.13 Therefore the metal cannot be pure gold. Copyright © Houghton Mifflin Company. All rights reserved. 10 | 26 Enthalpy • Change in enthalpy (ΔHp = qp): the amount of heat exchanged when heat exchange occurs under conditions of constant pressure • Enthalpy is a state function • ΔH is independent of the path taken Copyright © Houghton Mifflin Company. All rights reserved. 10 | 27 Hess’s Law • Hess’s Law: in going from a set of reactants to a set of 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. All rights reserved. 10 | 28 Hess’ Law (cont.) • ΔHreaction= ∑Δhsteps • If the direction of a reaction is reversed, the sign of ΔH is reversed. • ΔHforward = -Δhreverse • Magnitude of ΔH α quantities of reactants and products Copyright © Houghton Mifflin Company. All rights reserved. 10 | 29 Hess’s Law (cont.) • Overall reaction: N2 + 2O2 2NO2 ΔH = 68 kJ • This reaction can be carried out in 2 steps: N2 + O2 2NO ΔH = 180 kJ 2NO + O2 2NO2 ΔH = -112 kJ -------------------------------------------------------N2 + 2O2 2NO2 ΔH = 68 Kj Note: the sum of the two reactions gives the overall reaction and the same is true for the sum of the enthalpy change values. Copyright © Houghton Mifflin Company. All rights reserved. 10 | 30 Calorimetry • The amount of heat flow transferred during a reaction is determined from temperature measurements made in a calorimeter. • Heat loss is minimized by having insulation. A simple calorimeter can be made in the lab by stacking 2 styrofoam cups. A calorimeter minimizes heat exchange between the system and the surroundings. • Amount of heat produced is calculated by measuring the temp change in the surrounding water. • DH=D t (H20) X mH2O XCpH2O Copyright © Houghton Mifflin Company. All rights reserved. 10 | 31 Calorimetry (cont.) Copyright © Houghton Mifflin Company. All rights reserved. 10 | 32 Energy Quality & Quantity • While the total amount or quantity of energy in the universe is constant (1st Law) the quality of energy is degraded as it is used. Burning of petroleum: High grade concentrated energy energy (heat) Copyright © Houghton Mifflin Company. All rights reserved. Low grade 10 | 33 Fuels • Petroleum – A fossil fuel composed mainly of hydrocarbons • Natural gas – Consists largely of methane – Also contains ethane, propane, and butane Copyright © Houghton Mifflin Company. All rights reserved. 10 | 34 Fuels (cont.) Copyright © Houghton Mifflin Company. All rights reserved. 10 | 35 Fuels (cont.) Copyright © Houghton Mifflin Company. All rights reserved. 10 | 36 Fuels (cont.) • Coal – Matures geologically through stages Copyright © Houghton Mifflin Company. All rights reserved. 10 | 37 Global Warming Copyright © Houghton Mifflin Company. All rights reserved. 10 | 38 Global Warming (cont.) Copyright © Houghton Mifflin Company. All rights reserved. 10 | 39 Energy Use and Sources Copyright © Houghton Mifflin Company. All rights reserved. 10 | 40 Energy as a Driving Force • Most processes that occur spontaneously involve an “energy spread.” – Heat flows from high to low temperature and “spreads” …or a “matter spread” – Salt dissolves or “spreads” in water Copyright © Houghton Mifflin Company. All rights reserved. 10 | 41 Entropy • Entropy (S) is a measure of disorder or randomness. – As a system becomes more disordered, ΔS >0 • Second Law of Thermodynamics: the entropy of the universe is always increasing. • Tendency in nature is to increase disorder (unless external forces counteract). Ex—messy room, throwing a puzzle • -Entropy in solids< liquids<gases Copyright © Houghton Mifflin Company. All rights reserved. 10 | 42 • Entropy=S (absolute Entropy for a substance=Entropy at absolute zero temp -273K). Units J/K.mol • - change in Entropy= DS • DS=Sproducts-Sreactants – - Entropy can be the driving force behind reactions. Ex- reactions leading to the formation of gases (from solids) are favored. – - Higher temp=higher Entropy (due to more KE of particles) – - Lower temp=lower Entropy (less KE) – - Ideal conditions for a spontaneous reaction • Increase Entropy (disorder) • Decrease enthalpy of products Copyright © Houghton Mifflin Company. All rights reserved. 10 | 43 •- Reactions can thus occur even if not entropically favored. Ex• 2H2 (g)+O2 (g) 2H2O (g) • 3 molecules2 molecules (decrease in entropysame physical state) • But reaction is highly exothermic (ie. Much lower enthalpy of products) Copyright © Houghton Mifflin Company. All rights reserved. 10 | 44