Chemistry

Enthalpy for Phase Changes

Enthalpy for phase changes refers to the heat energy absorbed or released when a substance changes from one phase to another, such as from solid to liquid or liquid to gas. This energy is known as the heat of fusion or vaporization and is represented by the enthalpy change (∆H) for the specific phase transition. It is a key concept in understanding the thermodynamics of phase changes.

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12 Key excerpts on "Enthalpy for Phase Changes"

  • Book cover image for: Survival Guide to General Chemistry
    • Patrick E. McMahon, Rosemary McMahon, Bohdan Khomtchouk(Authors)
    • 2019(Publication Date)
    • CRC Press
      (Publisher)
    p .
    ΔE = qp − PΔV
    ΔE = ΔH − PΔV; or solving for ΔH: ΔH = ΔE + PΔV
    Enthalpy is the change in potential energy (ΔPE) of a chemical process measured as heat transfer under conditions of constant pressure; work energy change (expansion or contraction of volume) is not included. Enthalpy, however, is a useful measure of energy change for a wide variety of chemical processes and is often a close approximation of total energy change. For many chemical reactions, such as solubility reactions, reactions in solution, or reactions involving only solids and liquids, volume expansion at constant pressure is very small (ΔV ≅ 0). In these cases, enthalpy and total energy change are approximately equal: ΔE ≅ ΔH.
    Volume expansion or contraction can be significant whenever gases are formed or consumed in a reaction; the number of moles of gas then changes from reactants to products. Even in many of these cases, however, the total energy contribution from the work term (−PΔV) can often be small as compared to the enthalpy term (ΔH).
    Example:
    C 2
    H 8
    N 2
    ( I )
    + 2
    N 2
    O
    4 ( g )
    3
    N
    2
    ( g )
    + 2 C
    O
    2
    ( g )
    + 4
    H 2
    O
    ( g )
    2  moles of gas   9  moles of gas
    At constant pressure, the work of gas expansion (w = −PΔV) equals −22 kJ/mole. (Properties of gases and energy are described in Chapter 20
  • Book cover image for: Thermochemistry
    eBook - PDF
    • Rose Marie O. Mendoza(Author)
    • 2020(Publication Date)
    • Arcler Press
      (Publisher)
    The energy to affect a transition phase has been evaluated for a number of substances. The enthalpy or heat of fusion (Hf) of a substance is the required energy to melt one mole or one gram of that substance while the enthalpy (heat) of vaporization or heat of vaporization (Hv) is the required energy to vaporize one mole or one gram of that substance. 2.2. HESS’S LAW There are basically two methods to assess the amount of heat involved in a chemical change: measure it through experiments or estimate it from other experimentally determined enthalpy changes. There are some reactions which are difficult to do, if not impossible, to examine and make exact experimental measurements. . The estimation of the total enthalpy changes of a certain chemical system lies in obtaining some basic thermodynamic properties of the substances and a knowledge of its formation process. As stated in the Hess Law: “ If a process can be written as the summation of numerous stepwise processes, the enthalpy changes of the total process is equivalent with the sum of the enthalpy changes of the various steps. ” Hess’s law is emphasizes that because enthalpy is a state function, enthalpy changes basically depend on the preliminary stage of a chemical process, but not on the path it takes from start to finish. Example 1: One can take into consideration the reaction of carbon with oxygen in order to create CO2 as by a two-step process that must end up with an overall process: C(s) + O2(g) ⟶ CO2(g) ΔH298° = −394 kJ (2.3) Principles of Thermochemistry 37 As proof of concept for Hess Law, consider the formation of carbon dioxide from the combustion of solid carbon with corresponding ΔH298°C = -394 kJ. In the two-step process, first there is formation of carbon monoxide using equation (2.3.1) then the formation of carbon dioxide from carbon monoxide using equation (2.3.2). Add up the two equations and cancel all terms that can be seen both is the reactant and product side.
  • Book cover image for: Introduction to the Physical Chemistry of Foods
    • Christos Ritzoulis(Author)
    • 2013(Publication Date)
    • CRC Press
      (Publisher)
    dV = 0), then Equation (2.4) can be written as
    Δ U =
    q v
    (2.5)
    where qV is the heat under constant volume.
  • If the transformation is under constant pressure,
    P d V
    = P
    V final 
    V initial 
    = P Δ V
    then Equation (2.4) can be written as
    Δ U =
    q p
    P Δ V
    (2.6)
    where qP is the change in heat under constant pressure. Let us call this heat qP “enthalpy” and represent it with the symbol H for ease of reference. The enthalpy of a system under constant pressure can thus be defined by a transformation of Equation (2.6):
    Δ H =
    q p
    = Δ U + P Δ V
    (2.7)
    and by extension
  • H = U + P V
    (2.8)
    The enthalpy here encompasses the internal energy U, namely the energy that is bound in the system, plus a parameter PV that is related to the pressure and the volume of the system.
    For systems in which the initial and final pressures are the same, enthalpy is usually preferred as it includes within it any change in volume. Thus, in the description of a hypothetical explosion that involves the instantaneous generation of n new molecules of ideal gas that expand by volume ΔV (until the final pressure becomes equal to the initial), we have from the ideal gas equation that
    P Δ V = Δ n  (R T )
    (2.9)
    and from Equation (2.8)
    Δ H = Δ U + Δ n  (R T )
    (2.10)
    On the contrary, for reactions where the change in volume of the products is negligible in comparison to the volume of the solvent in which the reaction occurs (a typical scenario in food and pharmaceutical sciences), we have Δn = 0 and Equation (2.10) becomes
    Δ H = Δ U
    (2.11)

    2.2 Thermochemistry

    Thermochemistry is the application of the First Law of Thermodynamics for the purpose of studying and quantifying the energy changes that take place during chemical reactions. Chemical reactions are divided into endothermic and exothermic reactions. If the temperature increases during a chemical reaction, heat will be transferred to the environment in order to restore the initial temperature of the system. This heat transfer is negative from the point of view of the system (i.e., heat is lost from the system to the environment), and such a reaction is termed exothermic. If the temperature decreases during the reaction, heat is transferred from the environment into the system. This is a positive heat transfer and the reaction is termed endothermic.
  • Book cover image for: Phase Transformations in Metals and Alloys
    • David A. Porter, Kenneth E. Easterling, Mohamed Y. Sherif(Authors)
    • 2021(Publication Date)
    • CRC Press
      (Publisher)
    ) .
    The Gibbs free energy of a system is defined by the equation
    G = H T S
    (1.1)
    where H is the enthalpy, T is the absolute temperature and S is the entropy of the system. Enthalpy is a measure of the heat content of the system and is given by
    H = E + P V
    (1.2)
    where E is the internal energy of the system, P is the pressure and V is the volume. The internal energy arises from the total kinetic and potential energies of the atoms within the system. Kinetic energy can arise from atomic vibration in solids or liquids and from translational and rotational energies for the atoms and molecules within a liquid or gas; whereas potential energy arises from the interactions, or bonds, between the atoms within the system. If a transformation or reaction occurs, the heat that is absorbed or evolved will depend on the change in the internal energy of the system. However, it will also depend on changes in the volume of the system and the term PV takes this into account, so that at constant pressure the heat absorbed or evolved is given by the change in H. When dealing with condensed phases, i.e., solids and liquids, the PV term is usually very small in comparison to E , that is, H E. This approximation will be made frequently in the treatments given in this book. The other function that appears in the expression for G is entropy
    ( S )
  • Book cover image for: General Chemistry I as a Second Language
    eBook - PDF

    General Chemistry I as a Second Language

    Mastering the Fundamental Skills

    • David R. Klein(Author)
    • 2015(Publication Date)
    • Wiley
      (Publisher)
    But there are also a couple of special processes (not reactions) that also get special names. Here are the two common names that you will see in this course: 1. When one mole of a substance turns from a solid into a liquid (so the solid is melting), there is a change in enthalpy associated with the melting process. This H is called the heat of fusion, and it is shown like this: H fus . 2. When one mole of a substance turns from a liquid into a gas (so the liquid is said to vaporize), there is a change in enthalpy associated with the vaporiza- 5.4 WHAT IS ENTHALPY? 147 148 CHAPTER 5 ENERGY AND ENTHALPY tion process. This H is called the heat of vaporization, and it is shown like this: H vap . These two processes both represent phase changes. These are the only two values of H that you will need to describe any phase change. This is shown in the fol- lowing diagram: Gas Solid Liquid H fus H vap H fus H vap We have now seen several situations that get their own special terms: H fus , H vap , H comb , and H f . But all of these terms represent the same concept: enthalpy. There is one more thing we should mention about the way we report enthalpy. The value of H depends on the temperature and pressure at which the process takes place. So, if I say that the enthalpy change for a process is 34 Joules per mole, you should say, “At what temperature and pressure did you do the process?” If you did the process at a different temperature or pressure, the value of H would be dif- ferent. In order to take this into account, we have created a term called the Stan- dard State Enthalpy (H°). This means that we are specifically talking about 25° C and 1 atmosphere of pressure. To denote the standard state enthalpy change, we use the degree symbol: H°. You can think of it as reminding you what tempera- ture (and pressure) we are talking about. 5.5 HESS’S LAW When it comes to calculating enthalpies, there are two common types of problems that you need to know how to do.
  • Book cover image for: Foundations of Chemistry
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    Foundations of Chemistry

    An Introductory Course for Science Students

    • Philippa B. Cranwell, Elizabeth M. Page(Authors)
    • 2021(Publication Date)
    • Wiley
      (Publisher)
    150 Energy, enthalpy, and entropy enthalpy change are kJ mol − 1 . The actual value of the enthalpy change for a spe-cific reaction depends upon three variables: the amount of substance, the temper-ature, and the pressure at which the reaction is carried out. The standard enthalpy change is the enthalpy change that occurs when the reaction is carried out under standard conditions. This means at a pressure of 1 bar (1.00 × 10 5 Pa) with the reactants in their standard states. Values for enthalpy changes are usually quoted at a temperature of 298 K (25 C). When referring to a standard enthalpy change, we use the symbol Δ H ϴ . We say this as ‘ delta H plimsoll ’ . 6.1.2 Exothermic and endothermic reactions In many chemical reactions, heat energy is released to the surroundings. This type of reaction is called an exothermic reaction . We can detect the heat energy released because the reaction mixture gets hot, and this heat energy flows to the surroundings. The surroundings include any material around the reaction mix-ture – this can be the air in the room, the apparatus, and any solvent or insulation material. In some reactions, such as the combustion of magnesium wire or petrol, it is obvious that heat is given out as we can observe the material burning and measure a temperature increase. However, in some reactions, the enthalpy change is small and not as easy to detect or measure. Some reactions absorb heat energy from the surroundings when they take place. The reaction mixture gets cooler and so heat energy flows from the sur-roundings to equilibrate the temperatures. These are known as endothermic reactions . The direction of heat flow in exothermic and endothermic reactions is shown in Figure 6.2. Several ammonium salts dissolve in water endothermically, so the tempera-ture of the solution decreases.
  • Book cover image for: Chemistry
    eBook - PDF

    Chemistry

    Principles and Reactions

    187 8 ▼ Thermochemistry Chapter Outline 8-1 Principles of Heat Flow 8-2 Measurement of Heat Flow; Calorimetry 8-3 Enthalpy 8-4 Thermochemical Equations 8-5 Enthalpies of Formation 8-6 Bond Enthalpy 8-7 The First Law of Thermodynamics ▼ T his chapter deals with energy and heat, two terms used widely by both the gen-eral public and scientists. Energy, in the vernacular, is equated with pep and vitality. Heat conjures images of blast furnaces and sweltering summer days. Scientifically, these terms have quite different meanings. Energy can be defined as the capacity to do work. Heat is a particular form of energy that is transferred from a body at a high temperature to one at a lower temperature when they are brought into contact with each other. Two centuries ago, heat was believed to be a material fluid (caloric); we still use the phrase “heat flow” to refer to heat transfer or to heat effects in general. Thermochemistry refers to the study of the heat flow that accompanies chemical reactions. Our discussion of this subject will focus on ■ the basic principles of heat flow (Section 8-1). ■ the experimental measurement of the magnitude and direction of heat flow, known as calorimetry (Section 8-2). ■ the concept of enthalpy, H (heat content) and enthalpy change , D H (Section 8-3). ■ the calculation of D H for reactions, using thermochemical equations (Section 8-4) and enthalpies of formation (Section 8-5). ■ heat effects in the breaking and formation of covalent bonds (Section 8-6). ■ the relation between heat and other forms of energy, as expressed by the first law of thermodynamics (Section 8-7). Scala/Art Resource, NY The candle flame gives off heat, melting the candle wax. Wax melting is a phase change from solid to liquid and an endothermic reaction. Some say the world will end in fire, Some say in ice. From what I’ve tasted of desire I hold with those who favor fire. —ROBERT FROST Fire and Ice Copyright 2016 Cengage Learning.
  • Book cover image for: General Chemistry: Atoms First
    • Young, William Vining, Roberta Day, Beatrice Botch(Authors)
    • 2017(Publication Date)
    Vasilyev/Shutterstock.com Thermochemistry Unit Outline 10.1 Energy 10.2 Enthalpy 10.3 Energy, Temperature Changes, and Changes of State 10.4 Enthalpy Changes and Chemical Reactions 10.5 Hess’s Law 10.6 Standard Heats of Reaction In This Unit… This unit begins an exploration of thermochemistry, the study of the role that energy in the form of heat plays in chemical processes. We inves-tigate the energy changes that take place during phase changes and the chemical reactions you have studied previously and learn why some chemical reactions occur while others do not. In Electromagnetic Radiation and the Electronic Structure of the Atom (Unit 3), you stud-ied energy changes at the molecular level and the consequences those energy changes have on the properties of atoms and elements. 10 Copyright 2018 Cengage Learning. All Rights Reserved. May not be copied, scanned, or duplicated, in whole or in part. WCN 02-300 Unit 10 Thermochemistry 272 10.1 Energy 10.1a Energy and Energy Units Chemical reactions involve reactants undergoing chemical change to form new substances, products. reactants S products What is not apparent in the preceding equation is the role of energy in a reaction. For many reactions, energy, often in the form of heat, is absorbed—that is, it acts somewhat like a reactant. You might write an equation for those reactions that looks like this: energy 1 reactants S products In other reactions, energy is produced—that is, it acts like a product: reactants S products 1 energy In Chemistry, Matter on the Atomic Scale (Unit 1), we defined energy (the ability to do work) and work (the force involved in moving an object some distance). From a chemist’s point of view, energy is best viewed as the ability to cause change, and thermochemistry is the study of how energy in the form of heat is involved in chemical change.
  • Book cover image for: The Basics of Physics
    • Richard L. Myers(Author)
    • 2005(Publication Date)
    • Greenwood
      (Publisher)
    Heat transfer may cause a phase change, and no temperature change occurs as long as two phases are present. In this situation, heat is referred to as latent heat. The relationship between heat and phase changes will be examined in the next section. The relationship between heat trans- fer, Q, and the change in temperature of a substance depend s on the specific heat 86 Heat capacity of the substance. The specific heat capacity of a substance is a measure of the amount of heat necessary to raise the tem- perature of 1 g of the substance by 1°C. The specific heats of several common substances are listed in Table 6.1. Table 6.1 demon- strates that the specific heat of a substance depends on its phase. The specific heat of liquid water is approximately twice that of ice and steam. Water has one of the highest specific heats compared to other liquids. The high specific heat capacity of liquid water is directly related to its chemical structure and the presence of hydrogen bonds. The high specific heat of water explains why coastal environments have more moderate weather than areas at similar latitudes located inland. Water's high specific heat capacity means coastal regions will not experience drastic temperature changes as compared to inland regions. The relationship between heat, specific heat capacity, and temperature change of a substance is given by the equation Q = mcAT. In this equation, Q is the amount of thermal Table 6.1 Specific Heat Capacity of Some Common Substances Substance Steel Wood Ice Liquid water Steam Air Alcohol Specific Heat J/g=°C 0.45 1.7 2.1 4.2 2.0 1.0 2.5 energy (often Q is referred to simply as heat) transferred in joules, m is the mass in grams, c is the specific heat capacity of the sub- stance, and AT is the change in temperature. The temperature change is equal to the final temperature minus the initial temperature. As an application of this equation, consider what happens when heating a pot of water on the stove.
  • Book cover image for: Physical Chemistry
    eBook - PDF

    Physical Chemistry

    Understanding our Chemical World

    • Paul M. S. Monk(Author)
    • 2005(Publication Date)
    • Wiley
      (Publisher)
    And, as we have consistently reported, the best macroscopic indicator of a microscopic energy change is a change in temperature. Like internal energy, we can never know the enthalpy of a reagent; only the change in enthalpy during a reaction or process is knowable. Nevertheless, we can think of changes in H . Consider the preparation of ammonia: N 2(g) + 3H 2(g) −−→ 2NH 3(g) (3.26) We obtain the standard enthalpy change on reaction H O r as a sum of the molar enthalpies of each chemical participating in the reaction: H O r = products νH O m − reactants νH O m (3.27) The values of ν for the reaction in Equation (3.26) are ν (NH 3 ) = +2, ν (H 2 ) = −3 and ν (N 2 ) = −1. We obtain the standard molar enthalpy of forming ammonia after inserting values into Equation (3.27), as H O r = 2H O m (NH 3 ) − [H O m (N 2 ) + 3H O m (H 2 )] SAQ 3.8 Write out an expression for H O r for the reaction 2NO + O 2 → 2NO 2 in the style of Equation (3.27). Unfortunately, we do not know the enthalpies of any reagent. All we can know is a change in enthalpy for a reaction or process. But what is the magnitude of this energy change? As a consequence of Hess’s law (see p. 98), the overall change in enthalpy accompanying a reaction follows from the number and nature of the bonds involved. We call the overall enthalpy change during a reaction the ‘reaction enthalpy’ H r , and define it as ‘the change in energy occurring when 1 mol of reaction occurs’. In consequence, its units are J mol −1 , although chemists will usually want to express H in kJ mol −1 . In practice, we generally prefer to tighten the definition of H r above, and look at reagents in their standard states. Furthermore, we maintain the temperature T at 298 K, and the pressure p at p O . We call these conditions standard temperature and pressure, or s.t.p. for short. We need to specify the conditions because temperature and pressure can so readily change the physical conditions of the reactants and products.
  • Book cover image for: Chemistry 2e
    eBook - PDF
    • Paul Flowers, Klaus Theopold, Richard Langley, William R. Robinson(Authors)
    • 2019(Publication Date)
    • Openstax
      (Publisher)
    According to the law of conservation of matter (seen in an earlier chapter), there is no detectable change in the total amount of matter during a chemical change. When chemical reactions occur, the energy changes are relatively modest and the mass changes are too small to measure, so the laws of conservation of matter and energy hold well. However, in nuclear reactions, the energy changes are much larger (by factors of a million or so), the mass changes are measurable, and matter-energy conversions are significant. This will be examined in more detail in a later chapter on nuclear chemistry. Thermal Energy, Temperature, and Heat Thermal energy is kinetic energy associated with the random motion of atoms and molecules. Temperature is a quantitative measure of “hot” or “cold.” When the atoms and molecules in an object are moving or 5.1 • Energy Basics 213 vibrating quickly, they have a higher average kinetic energy (KE), and we say that the object is “hot.” When the atoms and molecules are moving slowly, they have lower average KE, and we say that the object is “cold” ( Figure 5.4). Assuming that no chemical reaction or phase change (such as melting or vaporizing) occurs, increasing the amount of thermal energy in a sample of matter will cause its temperature to increase. And, assuming that no chemical reaction or phase change (such as condensation or freezing) occurs, decreasing the amount of thermal energy in a sample of matter will cause its temperature to decrease. FIGURE 5.4 (a) The molecules in a sample of hot water move more rapidly than (b) those in a sample of cold water. LINK TO LEARNING Click on this interactive simulation (http://openstax.org/l/16PHETtempFX) to view the effects of temperature on molecular motion. Most substances expand as their temperature increases and contract as their temperature decreases. This property can be used to measure temperature changes, as shown in Figure 5.5.
  • Book cover image for: Chemical Thermodynamics at a Glance
    • H. Donald Brooke Jenkins(Author)
    • 2008(Publication Date)
    • Wiley-Blackwell
      (Publisher)
    fus S = fus H T m (21.5) Similarly at EF, the entropy change, vap S , for the process (l) → (g) at T b and hence the magnitude of the entropy rise at temperature brought about by the phase change (EF) can be calculated using equation (15.10) (Frame 15), suitably adapted in order to apply to the vaporisation process, and hence: vap S = vap H T b (21.6) Hence we predict, from our simple thermodynamic arguments, there is a sharp rise in the entropy at phase transitions undergone by pure substances and that: vap S > fus S (21.7) For normal substances, this is borne out experimentally. 65 22. Variation of Enthalpy Function, H with Temperature for Solid, Liquid and Gaseous Phases 22.1 Relative Values of the Enthalpy Function, H for Solid, Liquid and Gas The enthalpy function, H , was first introduced in Frame 10, equation (10.8). In Figure 18.1, Frame 18 was shown the general variation of the Gibbs energy G as a function of temperature, T and using the equation: G = H − T S (18.1) it is clear that the intercept of the curve on the G axis at T = 0 K will be equal to H , the enthalpy function. Later (Frame 21) we extended the scope of Figure 18.1 (Frame 18) by considering individual phases solid, liquid and gas and plotted G versus T curves for each of these phases on the same axes. We can therefore see that the intercepts of the solid, liquid and gaseous phase curves on the G axis at T = 0 K will correspond then to H s , H l and H g . Also we see that: H g > H l > H s > 0 (22.1) This can be accounted for qualitatively by employing a simple model which permits the prediction of H (and S and G ) for the above phases. Schematically we can think of our respective solid, liquid and gas as shown in Figure 22.1.
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