目录

  • 1 Nomenclature
    • 1.1 Nomenclature
    • 1.2 Inorganic compounds
    • 1.3 Organic compounds
  • 2 Atom
    • 2.1 Basic Atomic Theory
    • 2.2 Evolution of Atomic Theory
    • 2.3 Atomic Structure and Symbolism
    • 2.4 Isotopes
    • 2.5 Early development of the periodic table of elements
    • 2.6 Organization of the elements
  • 3 Atoms: the quantum world
    • 3.1 Wave Nature of Light
    • 3.2 Quantized Energy and Photons
    • 3.3 the Bohr Model
    • 3.4 Wave Character of Matter
    • 3.5 Atomic Orbitals
    • 3.6 3D Representation of Orbitals
    • 3.7 Electron Spin
    • 3.8 Electron Configurations
  • 4 Molecular Shape and Structure
    • 4.1 VSEPR theory
    • 4.2 Hybridization
    • 4.3 sp3 hybridization
    • 4.4 sp2 hybridization
    • 4.5 sp hybridization
    • 4.6 Other hybridization
    • 4.7 Multiple Bonds
    • 4.8 Molecular Orbitals
    • 4.9 Second-Row Diatomic Molecules
  • 5 Fundamentals of Thermochemistry
    • 5.1 Systems, States and Processes
    • 5.2 Heat as a Mechanism to Transfer Energy
    • 5.3 Work as a Mechanism to Transfer Energy
    • 5.4 Heat Capacity and Calorimetry
    • 5.5 The First Law of Thermodynamics
    • 5.6 Heats of Reactions - ΔU and ΔH
    • 5.7 Indirect Determination of ΔH - Hess's Law
    • 5.8 Standard Enthalpies of Formation
  • 6 Principles of Thermodynamics
    • 6.1 The Nature of Spontaneous Processes
    • 6.2 Entropy and Spontaneity - A Molecular Statistical Interpretation
    • 6.3 Entropy Changes and Spontaneity
    • 6.4 Entropy Changes in Reversible Processes
    • 6.5 Quantum States, Microstates, and Energy Spreading
    • 6.6 The Third Law of Thermodynamics
    • 6.7 Gibbs Energy
  • 7 Chemical equilibrium
    • 7.1 Equilibrium
    • 7.2 Reversible and irreversible reaction
    • 7.3 Chemical equilirbium
    • 7.4 Chemical equilibrium constant, Kc
    • 7.5 Le Chatelier's principle
    • 7.6 RICE table
    • 7.7 Haber process
  • 8 Acid–Base Equilibria
    • 8.1 Classifications of Acids and Bases
    • 8.2 The Brønsted-Lowry Scheme
    • 8.3 Acid and Base Strength
    • 8.4 Buffer Solutions
    • 8.5 Acid-Base Titration Curves
    • 8.6 Polyprotic Acids
    • 8.7 Exact Treatment of Acid-Base Equilibria
    • 8.8 Organic Acids and Bases
  • 9 Kinetics
    • 9.1 Prelude to Kinetics
    • 9.2 Chemical Reaction Rates
    • 9.3 Factors Affecting Reaction Rates
    • 9.4 Rate Laws
    • 9.5 Integrated Rate Laws
    • 9.6 Collision Theory
    • 9.7 Reaction Mechanisms
    • 9.8 Catalysis
Heat Capacity and Calorimetry

Heat Capacity

We now introduce two concepts useful in describing heat flow and temperature change. The heat capacity () of a body of matter is the quantity of heat () it absorbs or releases when it experiences a temperature change () of 1 degree Celsius (or equivalently, 1 kelvin)



Heat capacity is determined by both the type and amount of substance that absorbs or releases heat. It is therefore an extensive property—its value is proportional to the amount of the substance.

For example, consider the heat capacities of two cast iron frying pans. The heat capacity of the large pan is five times greater than that of the small pan because, although both are made of the same material, the mass of the large pan is five times greater than the mass of the small pan. More mass means more atoms are present in the larger pan, so it takes more energy to make all of those atoms vibrate faster. The heat capacity of the small cast iron frying pan is found by observing that it takes 18,140 J of energy to raise the temperature of the pan by 50.0 °C


The larger cast iron frying pan, while made of the same substance, requires 90,700 J of energy to raise its temperature by 50.0 °C. The larger pan has a (proportionally) larger heat capacity because the larger amount of material requires a (proportionally) larger amount of energy to yield the same temperature change:


The specific heat capacity () of a substance, commonly called its specific heat, is the quantity of heat required to raise the temperature of 1 gram of a substance by 1 degree Celsius (or 1 kelvin):



Specific heat capacity depends only on the kind of substance absorbing or releasing heat. It is an intensive property—the type, but not the amount, of the substance is all that matters. For example, the small cast iron frying pan has a mass of 808 g. The specific heat of iron (the material used to make the pan) is therefore:



The large frying pan has a mass of 4040 g. Using the data for this pan, we can also calculate the specific heat of iron:



Although the large pan is more massive than the small pan, since both are made of the same material, they both yield the same value for specific heat (for the material of construction, iron). Note that specific heat is measured in units of energy per temperature per mass and is an intensive property, being derived from a ratio of two extensive properties (heat and mass). The molar heat capacity, also an intensive property, is the heat capacity per mole of a particular substance and has units of J/mol °C (Figure 1).


The picture shows two black metal frying pans sitting on a flat surface. The left pan is about half the size of the right pan.
Figure 1: Due to its larger mass, a large frying pan has a larger heat capacity than a small frying pan. Because they are made of the same material, both frying pans have the same specific heat. (CC BY; Mark Blaser via OpenStax).


The heat capacity of an object depends on both its mass and its composition. For example, doubling the mass of an object doubles its heat capacity. Consequently, the amount of substance must be indicated when the heat capacity of the substance is reported. The molar heat capacity (Cp) is the amount of energy needed to increase the temperature of 1 mol of a substance by 1°C; the units of Cp are thus J/(mol•°C).The subscript p indicates that the value was measured at constant pressure. The specific heat (cs) is the amount of energy needed to increase the temperature of 1 g of a substance by 1°C; its units are thus J/(g•°C).

We can relate the quantity of a substance, the amount of heat transferred, its heat capacity, and the temperature change either via moles  or mass:


where

  •  is the number of moles of substance and

  •  is the molar heat capacity (i.e., heat capacity per mole of substance), and

  •  is the temperature change.



where

  •  is the mass of substance in grams,

  •  is the specific heat (i.e., heat capacity per gram of substance), and

Both Equations are under constant pressure (which matters) and both show that we know the amount of a substance and its specific heat (for mass) or molar heat capcity (for moles), we can determine the amount of heat, , entering or leaving the substance by measuring the temperature change before and after the heat is gained or lost.

The specific heats of some common substances are given in Table 1. Note that the specific heat values of most solids are less than 1 J/(g•°C), whereas those of most liquids are about 2 J/(g•°C). Water in its solid and liquid states is an exception. The heat capacity of ice is twice as high as that of most solids; the heat capacity of liquid water, 4.184 J/(g•°C), is one of the highest known. The specific heat of a substance varies somewhat with temperature. However, this variation is usually small enough that we will treat specific heat as constant over the range of temperatures that will be considered in this chapter. Specific heats of some common substances are listed in Table 1.

Table 1: Specific Heats of Common Substances at 25 °C and 1 bar
SubstanceSymbol (state)Specific Heat (J/g °C)
heliumHe(g)5.193
waterH2O(l)4.184
ethanolC2H6O(l)2.376
iceH2O(s)2.093 (at −10 °C)
water vaporH2O(g)1.864
nitrogenN2(g)1.040
airmixture1.007
oxygenO2(g)0.918
aluminumAl(s)0.897
carbon dioxideCO2(g)0.853
argonAr(g)0.522
ironFe(s)0.449
copperCu(s)0.385
leadPb(s)0.130
goldAu(s)0.129
siliconSi(s)0.712
quartzSiO2(s)0.730

The value of  is intrinsically a positive number, but  and  can be either positive or negative, and they both must have the same sign. If  and  are positive, then heat flows from the surroundings into an object. If and  are negative, then heat flows from an object into its surroundings.

If a substance gains thermal energy, its temperature increases, its final temperature is higher than its initial temperature, then and  is positive. If a substance loses thermal energy, its temperature decreases, the final temperature is lower than the initial temperature, so  and  is negative.

Note that the relationship between heat, specific heat, mass, and temperature change can be used to determine any of these quantities (not just heat) if the other three are known or can be deduced.



Heat "Flow" to Thermal Equilibrium

When two objects at different temperatures are placed in contact, heat flows from the warmer object to the cooler one until the temperature of both objects is the same. The law of conservation of energy says that the total energy cannot change during this process:



The equation implies that the amount of heat that flows from a warmer object is the same as the amount of heat that flows into a cooler object. Because the direction of heat flow is opposite for the two objects, the sign of the heat flow values must be opposite:


Thus heat is conserved in any such process, consistent with the law of conservation of energy.

The amount of heat lost by a warmer object equals the amount of heat gained by a cooler object.

Substituting for  from Equation  gives




which can be rearranged to give


When two objects initially at different temperatures are placed in contact, we can use Equation to calculate the final temperature if we know the chemical composition and mass of the objects.