10.1.1: The Idea of Dynamic Chemical Equilibrium

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    10.1.1: The Idea of Dynamic Chemical Equilibrium

    Chapter 1
    1. Chapter 1: The Chemical World
    2. 1.1: The Scope of Chemistry
    3. 1.2: Chemicals Compose Ordinary Things
    4. 1.3: Hypothesis, Theories, and Laws
    5. 1.4: The Scientific Method: How Chemists Think
    6. 1.5: A Beginning Chemist: How to Succeed
    7. 1.E: Exercises
     •  Chapter 2
    1. Chapter 2: Measurement and Problem Solving
    2. 2.1: Taking Measurements
    3. 2.2: Scientific Notation: Writing Large and Small Numbers
    4. 2.3: Significant Figures: Writing Numbers to Reflect Precision
    5. 2.4: Significant Figures in Calculations
    6. 2.5: The Basic Units of Measurement
    7. 2.6: Problem Solving and Unit Conversions
    8. 2.7: Solving Multistep Conversion Problems
    9. 2.8: Units Raised to a Power
    10. 2.9: Density
    11. 2.10: Numerical Problem-Solving Strategies and the Solution Map
    12. 2.E: Measurement and Problem Solving (Exercises)
     •  Chapter 3
    1. Chapter 3: Matter and Energy
    2. 3.1: In Your Room
    3. 3.2: What is Matter?
    4. 3.3: Classifying Matter According to Its State: Solid, Liquid, and Gas
    5. 3.4: Classifying Matter According to Its Composition
    6. 3.5: Differences in Matter: Physical and Chemical Properties
    7. 3.6: Changes in Matter: Physical and Chemical Changes
    8. 3.7: Conservation of Mass: There is No New Matter
    9. 3.8: Energy
    10. 3.9: Energy and Chemical and Physical Change
    11. 3.10: Temperature: Random Motion of Molecules and Atoms
    12. 3.11: Temperature Changes: Heat Capacity
    13. 3.12: Energy and Heat Capacity Calculations
    14. 3.E: Exercises
     •  Chapter 4
    1. Chapter 4: Atoms and Elements
    2. 4.1: Experiencing Atoms at Tiburon
    3. 4.2: Indivisible: The Atomic Theory
    4. 4.3: The Nuclear Atom
    5. 4.4: The Properties of Protons, Neutrons, and Electrons
    6. 4.5: Elements: Defined by Their Number of Protons
    7. 4.6: Looking for Patterns: The Periodic Table
    8. 4.7: Ions: Losing and Gaining Electrons
    9. 4.8: Isotopes: When the Number of Neutrons Varies
    10. 4.9: Atomic Mass: The Average Mass of an Element’s Atoms
      •  Chapter 5
    1. Chapter 5: Molecules and Compounds
    2. 5.1: Sugar and Salt
    3. 5.2: Compounds Display Constant Composition
    4. 5.3: Chemical Formulas: How to Represent Compounds
    5. 5.4: A Molecular View of Elements and Compounds
    6. 5.5: Writing Formulas for Ionic Compounds
    7. 5.6: Nomenclature: Naming Compounds
    8. 5.7: Naming Ionic Compounds
    9. 5.8: Naming Molecular Compounds
    10. 5.9: Naming Acids
    11. 5.10: Nomenclature Summary
    12. 5.11: Formula Mass: The Mass of a Molecule or Formula Unit
      •  Chapter 6
    1. 6: Chemical Composition
    2. 6.1: How Much Sodium?
    3. 6.2: Counting Nails by the Pound
    4. 6.3: Counting Atoms by the Gram
    5. 6.4: Counting Molecules by the Gram
    6. 6.5: Chemical Formulas as Conversion Factors
    7. 6.6: Mass Percent Composition of Compounds
    8. 6.7: Mass Percent Composition from a Chemical Formula
    9. 6.8: Calculating Empirical Formulas for Compounds
    10. 6.9: Calculating Molecular Formulas for Compounds
      •  Chapter 7
    1. Chapter 7: Chemical Reactions
    2. 7.1: Grade School Volcanoes, Automobiles, and Laundry Detergents
    3. 7.2: Evidence of a Chemical Reaction
    4. 7.3: Chemical Equations
    5. 7.4: How to Write Balanced Chemical Equations
    6. 7.5: Aqueous Solutions and Solubility: Compounds Dissolved in Water
    7. 7.6: Precipitation Reactions
    8. 7.7: Writing Chemical Equations for Reactions in Solution: Molecular, Complete Ionic, and Net Ionic Equations
    9. 7.8: Acid–Base and Gas Evolution Reactions
    10. 7.9: Oxidation–Reduction Reactions
    11. 7.10: Classifying Chemical Reactions
    12. 7.11: The Activity Series: Predicting Spontaneous Redox Reactions
     •  Chapter 8
    1. Chapter 8: Quantities in Chemical Reactions
    2. 8.1: Climate Change: Too Much Carbon Dioxide
    3. 8.2: Stoichiometry
    4. 8.3: Mole-to-Mole Conversions
    5. 8.4: Making Molecules: Mole to Mass (or vice versa) and Mass-to-Mass Conversions
    6. 8.5: Limiting Reactant and Theoretical Yield
    7. 8.6: Limiting Reactant, Theoretical Yield, and Percent Yield from Initial Masses of Reactants
    8. 8.7: Enthalpy Change is a Measure of the Heat Evolved or Absorbed
     •  Chapter 9
    1. Chapter 9: Electrons in Atoms and the Periodic Table
    2. 9.1: Blimps, Balloons, and Models of the Atom
    3. 9.2: Light is Visible Electromagnetic Radiation
    4. 9.3: The Electromagnetic Spectrum
    5. 9.4: The Bohr Model: Atoms with Orbits
    6. 9.5: The Quantum-Mechanical Model: Atoms with Orbitals
    7. 9.6: Quantum-Mechanical Orbitals and Electron Configurations
    8. 9.7: Electron Configurations and the Periodic Table
    9. 9.8: The Explanatory Power of the Quantum-Mechanical Model
    10. 9.9: Periodic Trends: Atomic Size, Ionization Energy, and Metallic Character
    11. 9.E: Electrons in Atoms and the Periodic Table (Exercises)
    Chapter 10
    1. Chapter 10: Chemical Bonding
    2. 10.1: Bonding Models and AIDS Drugs
    3. 10.2: Representing Valence Electrons with Dots
    4. 10.3: Lewis Structures of Ionic Compounds: Electrons Transferred
    5. 10.4: Covalent Lewis Structures: Electrons Shared
    6. 10.5: Writing Lewis Structures for Covalent Compounds
    7. 10.6: Resonance: Equivalent Lewis Structures for the Same Molecule
    8. 10.7: Predicting the Shapes of Molecules
    9. 10.8: Electronegativity and Polarity: Why Oil and Water Don’t Mix
     •  Chapter 11
    1. Chapter 11: Gases
    2. 11.1: Extra-Long Straws
    3. 11.2: Kinetic Molecular Theory: A Model for Gases
    4. 11.3: Pressure: The Result of Constant Molecular Collisions
    5. 11.4: Boyle’s Law: Pressure and Volume
    6. 11.5: Charles’s Law: Volume and Temperature
    7. 11.5A: Gay-Lussac's Law: Temperature and Pressure
    8. 11.6: The Combined Gas Law: Pressure, Volume, and Temperature
    9. 11.7: Avogadro’s Law: Volume and Moles
    10. 11.8: The Ideal Gas Law: Pressure, Volume, Temperature, and Moles
    11. 11.9: Mixtures of Gases: Why Deep-Sea Divers Breathe a Mixture of Helium and Oxygen
    12. 11.10: Gases in Chemical Reactions
     •  Chapter 12
    1. Chapter 12: Liquids, Solids, and Intermolecular Forces
    2. 12.1: Interactions between Molecules
    3. 12.2: Properties of Liquids and Solids
    4. 12.3: Surface Tension and Viscosity
    5. 12.4: Evaporation and Condensation
    6. 12.5: Melting, Freezing, and Sublimation
    7. 12.6: Types of Intermolecular Forces: Dispersion, Dipole–Dipole, Hydrogen Bonding, and Ion-Dipole
    8. 12.7: Types of Crystalline Solids
    9. 12.8: Water: A Remarkable Molecule
     •  Chapter 13
    1. Chapter 13: Solutions
    2. 13.1: Prelude - Tragedy in Cameroon
    3. 13.2: Solutions: Homogeneous Mixtures
    4. 13.3: Solutions of Solids Dissolved in Water: How to Make Rock Candy
    5. 13.4: Solutions of Gases in Water
    6. 13.5: Solution Concentration: Mass Percent
    7. 13.6: Solution Concentration: Molarity
    8. 13.7: Solution Dilution
    9. 13.8: Solution Stoichiometry
    10. 13.9: Freezing Point Depression and Boiling Point Elevation
    11. 13.10: Osmosis
      •  Chapter 14
    1. Chapter 14: Acids and Bases
    2. 14.1: Sour Patch Kids and International Spy Movies
    3. 14.2: Acids: Properties and Examples
    4. 14.3: Bases: Properties and Examples
    5. 14.4: Molecular Definitions of Acids and Bases
    6. 14.5: Reactions of Acids and Bases
    7. 14.6: Acid–Base Titration
    8. 14.7: Strong and Weak Acids and Bases
    9. 14.8: Water: Acid and Base in One
    10. 14.9: The pH and pOH Scales: Ways to Express Acidity and Basicity
    11. 14.10: Buffers: Solutions That Resist pH Change
     •  Chapter 15
    1. Chapter 15: Chemical Equilibrium
    2. 15.1: Life is Controlled Disequilibrium
    3. 15.2: The Rate of a Chemical Reaction
    4. 15.3: The Idea of Dynamic Chemical Equilibrium
    5. 15.4: The Equilibrium Constant: A Measure of How Far a Reaction Goes
    6. 15.5: Heterogeneous Equilibria: The Equilibrium Expression for Reactions Involving a Solid or a Liquid
    7. 15.6: Calculating and Using Equilibrium Constants
    8. 15.7: Disturbing a Reaction at Equilibrium: Le Châtelier’s Principle
    9. 15.8: The Effect of a Concentration Change on Equilibrium
    10. 15.9: The Effect of a Volume Change on Equilibrium
    11. 15.10: The Effect of Temperature Changes on Equilibrium
    12. 15.11: The Solubility-Product Constant
    13. 15.12: The Path of a Reaction and the Effect of a Catalyst
      •  Chapter 16
    1. Chapter 16: Oxidation and Reduction
    2. 16.1: The End of the Internal Combustion Engine?
    3. 16.2: Oxidation and Reduction: Some Definitions
    4. 16.3: Oxidation States: Electron Bookkeeping
    5. 16.4: Balancing Redox Equations
    6. 16.5: The Activity Series: Predicting Spontaneous Redox Reactions
    7. 16.6: Batteries: Using Chemistry to Generate Electricity
    8. 16.7: Electrolysis: Using Electricity to Do Chemistry
    9. 16.8: Corrosion: Undesirable Redox Reactions
      •  Chapter 17
    1. Chapter 17: Radioactivity and Nuclear Chemistry
    2. 17.1: Diagnosing Appendicitis
    3. 17.2: The Discovery of Radioactivity
    4. 17.3: Types of Radioactivity: Alpha, Beta, and Gamma Decay
    5. 17.4: Detecting Radioactivity
    6. 17.5: Natural Radioactivity and Half-Life
    7. 17.6: Radiocarbon Dating: Using Radioactivity to Measure the Age of Fossils and Other Artifacts
    8. 17.7: The Discovery of Fission and the Atomic Bomb
    9. 17.8: Nuclear Power: Using Fission to Generate Electricity
    10. 17.9: Nuclear Fusion: The Power of the Sun
    11. 17.10: The Effects of Radiation on Life
    12. 17.11: Radioactivity in Medicine

    Template:HideTOC

    Learning Objectives
    • Describe the three possibilities that exist when reactants come together.
    • Describe what is occurring in a system at equilibrium.

    Think for a minute about sitting down to a table to eat dinner. There are three possibilities that could happen when you eat dinner. You could (1) finish your entire dinner, (2) you could not want any of it and leave it all on your plate, or (3) you could eat some of it and leave some of it. Reactions have the same possibilities. Reactions do not always proceed all the way from start to finish. You may have reactions that (1) go to completion so that at the end, the reaction vessel contains all products and only products. Some reactions (2) may not start at all, so at the end the reaction vessel contains all reactants and only reactants. And some reactions (3) may start but not go to completion, that is, the reaction might start but not go completely to products. In this last case, the reaction vessel would contain some reactants and some products. In this section, we are going to take a closer look at the third type of reaction.

    Reversible Reactions and Equilibrium

    Consider the hypothetical reaction:

    \[\text{A} + \text{B} \rightarrow \text{C} + \text{D}. \nonumber \]

    If we looked at this reaction using what we have learned, this reaction will keep going, forming \(\text{C}\) and \(\text{D}\) until \(\text{A}\) and \(\text{B}\) run out. This is what we call an "irreversible reaction" or a "reaction that goes to completion".

    Some reactions, however, are reversible, meaning the reaction can go backwards in which products react to form reactants, so that: \(\text{A} + \text{B} \leftarrow \text{C} + \text{D}\). The direction of the arrow shows that \(\text{C}\) and \(\text{D}\) are reacting to form \(\text{A}\) and \(\text{B}\). What if the two reactions, the forward reaction and the reverse reaction, were occurring at the same time? What would this look like? If you could peer into the reaction, you would be able to find \(\text{A}\), \(\text{B}\), \(\text{C}\), and \(\text{D}\) particles. \(\text{A}\) and \(\text{B}\) would react to form \(\text{C}\) and \(\text{D}\) at the same time that \(\text{C}\) and \(\text{D}\) are reacting to form \(\text{A}\) and \(\text{B}\).

    If the forward and reverse reactions are happening at the same rate, the reaction is said to be at equilibrium or dynamic equilibrium. At this point, the concentrations of \(\text{A}\), \(\text{B}\), \(\text{C}\), and \(\text{D}\) are not changing (or, are constant) and we would see no difference in our reaction container, but reactions are still occurring in both directions. It is important to point out that having constant amounts of reactants and products does NOT mean that the concentration of the reactants is equal to the concentration of the products. It means they are not changing. These reactions appear to have stopped before one of the reactants has run out.

    Chemists use a double-headed arrow, \(\rightleftharpoons\), to show that a reaction is at equilibrium. We would write the example reaction as:

    \[\text{A} + \text{B} \rightleftharpoons \text{C} + \text{D}. \nonumber \]

    The arrow indicates that both directions of the reaction are happening.

    Another way to think about reversible and irreversible reactions is to compare them to two types of games of tag. Reversible reactions are in many ways like a traditional game of tag: the "it" person can become "not it" and somebody who is "not it" is tagged and becomes "it". In this way, it is a reversible change. It is also like a reaction at equilibrium, because overall no change is occurring. There is always a constant number of "it" people and "not it" people in the game. Also, having constant numbers of "it" and "not it" people in our game does not mean that the number of "it" people (reactants) is equal to the number of "not it" people (products). Furthermore, this is similar to equilibrium in that this game never truly ends (unless everybody gets tired of playing). The game could go on forever. We could write this as the following reversible reaction:

    \[\text{"It"} \rightleftharpoons \text{"Not it"} \nonumber \]

    Irreversible reactions (those that only go in one direction from reactants to products and cannot reach a state of equilibrium) are more like a game of sharks and minnows. In sharks and minnows, almost everybody starts out as a minnow. Once tagged, they become a shark. However, the difference here is that once you are a shark you are always a shark; there is no way to go back to becoming a minnow. The game continues until everybody has been tagged and becomes a shark. This is similar to irreversible reactions in that the reactants turn into products, but can't change back. Furthermore, the reaction will proceed until the reactants have been used up and there are not any more left. We could write the reaction as:

    \[\text{Minnow} \rightarrow \text{Shark} \nonumber \]

    Here's another example of a reversible reaction—dissolving salt in a beaker of water, described by the following reaction:

    \[\ce{NaCl(s) \leftrightarrow NaCl(aq)} \nonumber \]

    If you keep adding more and more solid salt, eventually you'll reach the point where no more salt dissolves, and the excess sits at the bottom of the beaker. At this point we have a saturated solution. Has the dissolving reaction stopped? It would appear so, but that's not the case (wouldn't that be too easy?).

    What happens in our saturated solution, which has reached the point of equilibrium, is that both the forward

    \[\ce{NaCl(s) \rightarrow NaCl(aq)} \nonumber \]

    and reverse

    \[\ce{NaCl(aq) \rightarrow NaCl(s)} \nonumber \]

    reactions are still going on, but at the same rate. This in effect cancels out any observable, or measurable, changes in our system. At the same rate that solid NaCl produces aqueous NaCl (dissolved salt), the dissolved salt is re-crystallizing to form more solid NaCl.

    • Equilibrium is the state at which the rate of the forward reaction equals the rate of the reverse reaction.
    • At the point of equilibrium, no more measurable or observable changes in the system can be noted.

    It is important for you to understand that equilibrium means the rates of the forward and reverse reactions are equal; it does not mean that there are equal amounts of reactants and products present at equilibrium.

    For example, the following reaction was allowed to come to the point of equilibrium, and concentrations of all reaction participants were measured at that time:

    \(\ce{H_2(g) + I_2(g) \leftrightarrow 2HI(g)}\)

    At equilibrium:

    \(\mathrm{[H_2]=0.022\: M}\)

    \(\mathrm{[I_2]=0.022\: M}\)

    \(\mathrm{[HI]=0.156\: M}\)

    For this particular reversible reaction, there is more HI at equilibrium (0.156 M) than there is of H2 and I2 (both at 0.022M). We say that the product side of the reaction is favored.

    Equilibrium does not mean equal amounts at equilibrium!

    Here is an example to help you understand how equilibrium works: imagine yourself on a escalator that is going down. You start at the top (reactants) and end up at the bottom (products). But when you are partway down, you start walking up the escalator as it continues going down. If you match your rate of walking up to the same rate that the escalator is going down, you make no progress and appear to be at a standstill. To an observer it would look as if you and the escalator had come to a stop, when actually both upward and downward movements continue.

    Equilibrium is dynamic—both forward and reverse reactions continue, even though the reaction appears to have stopped. And this equilibrium does not need to occur right in the middle of two floors—you could be near the bottom, near the top, or anywhere in between when you carry out your reverse process.

    In order for a reversible reaction to reach the point of equilibrium, the reaction must be carried out in a closed system—no additional reactants can be added or products removed. If, in our last example, the product HI was removed as it formed, the reaction would never reach the point of equilibrium; instead, H2 and I2 would continue to react to produce HI until one or both of the reactants was used up.

    If reactants are constantly being added, and products removed as they form, the system would appear to be at equilibrium because to an outside observer it would appear that the reaction has stopped—but that would not be the case. This situation—with new material constantly being added as products are removed—is called a steady state system. A factory with an assembly line is a steady state system—new raw materials are constantly being added; finished products are removed. A campfire with wood being added to the fire is another steady state system. Be careful not to confuse steady state with equilibrium.

    How do the rates of the forward and reverse reactions change as the reaction heads towards equilibrium (before it reaches equilibrium)?

    If we start our above reaction with H2 and I2, and with no HI, the two gases will react at a certain rate. But remember that the rate of a reaction slows down over time, as the reactants get used up (and lower their concentrations). Eventually, however, the amount of the product HI increases, and it will begin producing H2 and I2. Thus the rate of the reverse reaction starts out slowly (there is no HI present), but will speed up as the concentration of HI increases. Eventually both rates will level off (not always to the same level as shown by this example, however):

    Graph showing a curve that decreases from 3.8 to 1.0 over time, labeled with "Rate (mL/min)" on the vertical axis and "Time (seconds)" on the horizontal axis.

    Chemists have found that there is a mathematical relationship that exists between the concentration of the reactants and products, once equilibrium has been reached, that is independent of the initial concentration of the participants. For any general reaction,

    \[\ce{aA + bB \rightleftharpoons cD + dD} \label{2.1.1} \]

    an equilibrium constant expression can be written as:

    \[\mathrm{K_{eq}=\dfrac{[C]^c \times [D]^d}{[A]^a \times [B]^b}} \label{2.1.2} \]

    This mathematical relationship exists for all equilibrium systems, and produces a constant ratio called the equilibrium constant, Keq .

    Law of Mass-Action

    Equation \ref{2.1.2} is sometimes called the Law of Mass-Action.

    This relationship will be very important to us for the next few units, so it is important that you understand how to set this relationship up and what it tells us about an equilibrium system.

    The products of the reaction (C and D) are placed in the numerator, and their concentrations are raised to the power of the coefficients from the balanced equation. The reactants (A and B) are placed in the denominator, with their concentrations raised to the power of their coefficients.

    Example \(\PageIndex{1}\)

    For the reaction between hydrogen and iodine gas to produce hydrogen iodide:

    \[\ce{H_2(g) + I_2(g) \rightleftharpoons 2HI(g)} \label{2.1.3} \]

    the equilibrium constant expression will be:

    \[\mathrm{K_{eq}=\dfrac{[HI]^2}{[H_2] \times [I_2]}} \label{2.1.4} \]

    Using the example we examined in our last section, equilibrium concentrations for each substance were measured at equilibrium and found to be:

    At equilibrium:

    \(\mathrm{[H_2]=0.022\: M}\)

    \(\mathrm{[I_2]=0.022\: M}\)

    \(\mathrm{[HI]=0.156\: M}\)

    We substitute these values into our equilibrium expression and solve for Keq:

    \[\mathrm{K_{eq}=\dfrac{[HI]^2}{[H_2] \times [I_2]}=\dfrac{(0.156)^2}{(0.022)(0.022)}=50.3} \nonumber \]

    The value of Keq, which has no units, is a constant for any particular reaction, and its value does not change unless the temperature of the system is changed. It does not depend on the initial concentrations used to reach the point of equilibrium.

    For example, the following data were obtained for equilibrium concentrations of H2, I2 and HI, and the value of Keq was calculated for each trial:

    Trial
    \(\ce{[HI]}\)
    \(\ce{[ H2]}\)
    \(\ce{[ I2]}\)
    \(K_{eq}\)
    1
    0.156
    0.0220
    0.0220
    50.3
    2
    0.750
    0.106
    0.106
    50.1
    3
    1.00
    0.820
    0.0242
    50.4
    4
    1.00
    0.0242
    0.820
    50.4
    5
    1.56
    0.220
    0.220
    50.3

    Aside from accounting for slight experimental variation between trials, the value for Keq is the same despite differences in equilibrium concentrations for the individual participants.

    There is one other important point to make at this time.

    Keq relates the concentrations of products to reactants at equilibrium.

    For aqueous solutions, concentration is often measured as mol · L-1. For gases, concentration is often measured as partial pressure.

    The concentrations of both aqueous solutions and gases change during the progress of a reaction. For reactions involving a solid or a liquid, while the amounts of the solid or liquid will change during a reaction, their concentrations (much like their densities) will not change during the reaction. Instead, their values will remain constant. Because they are constant, their values are not included in the equilibrium constant expression.

    Example \(\PageIndex{2}\)

    For example, consider the reaction showing the formation of solid calcium carbonate from solid calcium oxide and carbon dioxide gas:

    \[\ce{CaO(s) + CO_2(g) \leftrightarrow CaCO_3(s)} \nonumber \]

    The equilibrium constant for this reaction is (before modification):

    \[\mathrm{K_{eq}=\dfrac{[CaCO_3]}{[CaO] \times [CO_2]}} \nonumber \]

    But we remove those participants whose state is either a solid or a liquid, which leaves us with the following equilibrium constant expression:

    \[\mathrm{K_{eq}=\dfrac{1}{[CO_2]}} \nonumber \]

    Summary

    • There are a few possible ways a reaction can go: it can go to completion (\(\text{reactants} \rightarrow \text{products}\)), and it can occur but not go to completion. Instead, it will reach chemical equilibrium (\(\text{reactants} \rightleftharpoons \text{products}\)).
    • Chemical equilibrium occurs when the number of particles becoming products is equal to the number of particles becoming reactants.
    • A dynamic equilibrium is a state where the rate of the forward reaction is equal to the rate of the reverse reaction.

    Vocabulary

    • Equilibrium - A state that occurs when the rate of the forward reaction is equal to the rate of the reverse reaction.

    This page titled 10.1.1: The Idea of Dynamic Chemical Equilibrium was last modified on Fri, 16 Aug 2024 17:22:57 GMT and is shared under a CC BY-NC-SA 4.0 license and was authored, remixed, and/or curated by Marisa Alviar-Agnew & Henry Agnew via source content that was edited to the style and standards of the LibreTexts platform.