William M. White - Geochemistry

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Geochemistry: краткое содержание, описание и аннотация

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A Comprehensive Introduction to the “Geochemist Toolbox” – the Basic Principles of Modern Geochemistry In the new edition of William M. White’s
, undergraduate and graduate students will find each of the core principles of geochemistry covered. From defining key principles and methods to examining Earth’s core composition and exploring organic chemistry and fossil fuels, this definitive edition encompasses all the information needed for a solid foundation in the earth sciences for beginners and beyond. 
For researchers and applied scientists, this book will act as a useful reference on fundamental theories of geochemistry, applications, and environmental sciences. The new edition includes new chapters on the geochemistry of the Earth’s surface (the “critical zone”), marine geochemistry, and applied geochemistry as it relates to environmental applications and geochemical exploration.
● A review of the fundamentals of geochemical thermodynamics and kinetics, trace element and organic geochemistry
● An introduction to radiogenic and stable isotope geochemistry and applications such as geologic time, ancient climates, and diets of prehistoric people
● Formation of the Earth and composition and origins of the core, the mantle, and the crust
● New chapters that cover soils and streams, the oceans, and geochemistry applied to the environment and mineral exploration
In this foundational look at geochemistry, new learners and professionals will find the answer to the essential principles and techniques of the science behind the Earth and its environs.

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where S 0is the entropy at 0 K (the configurational, or third law entropy) and ΔS φ is the entropy change associated with any phase change. Compilations for S 298are available for many minerals. Table 2.2lists some heat capacity constants for the power series formula as well as other thermodynamic data for a few geologically important minerals. Example 2.6illustrates how entropy and enthalpy changes are calculated.

Example 2.6Calculating enthalpy and entropy changes

If the heat capacity of steam can be represented by a three-term power series:

with constants and - фото 247

with constants and and the enthalpy of vaporization at 100C is 406 kJmol c - фото 248, and and the enthalpy of vaporization at 100C is 406 kJmol calculate the - фото 249, and and the enthalpy of vaporization at 100C is 406 kJmol calculate the S and - фото 250, and the enthalpy of vaporization at 100°C is 40.6 kJ/mol, calculate the S and H changes when 1 mol of liquid water at 100°C and 1 atm is converted to steam and brought to 200°C and 3 atm. Assume that with respect to volume, steam behaves as an ideal gas (which, in reality, it is certainly not).

Answer : We need to calculate entropy and enthalpy associated with three changes: the conversion of water to steam, raising the steam from 100°C to 200°C, and increasing the pressure from 1 atm to 3 atm. Since both S and H are state variables, we can treat these three processes separately; our answer will be the sum of the result for each of these processes and will be independent of the order in which we do these calculations.

1 Conversion of water to steam. This process will result in ΔH of 40.6 kJ. For entropy, . We converted centigrade to Kelvin, or absolute, temperature.

2 Raising the steam from 100°C to 200°C (from 373 K to 473 K) isobarically. Since heat capacity is a function of temperature, we will have to integrate eqn. 2.112over the temperature interval:Evaluating this, we find that . The entropy change is given by:Evaluating this, we find that .

3 Increasing pressure from 1 atm to 3 atm (0.1 MPa to 0.3 MPa) isothermally. We can use eqn. 2.114to determine the enthalpy change associated with the pressure change. On the assumption of ideal gas behavior, we can substitute 1/T for α. Doing so, we find the equation goes to 0; thus, there is no enthalpy change associated with a pressure change for an ideal gas. This is in accord with assumptions about an ideal gas: namely, that there are no forces between molecules, hence no energy is stored as potential energy of attraction between molecules.

The isothermal pressure dependence of entropy is given by eqn. 2.106. We substitute 1/ T for α and R T/P for V and integrate from P 1to P 2:

The whole enthalpy and entropy changes are the sum of the changes in these - фото 251

The whole enthalpy and entropy changes are the sum of the changes in these three steps:

211 FREE ENERGY We can now introduce two free energy functions the Helmholtz - фото 252

2.11 FREE ENERGY

We can now introduce two free energy functions, the Helmholtz free energy and Gibbs free energy. Gibbs free energy is one of the most useful functions in thermodynamics.

2.11.1 Helmholtz free energy

We can rearrange eqn. 2.58to read d UT d S = − P d V . The − P d V term is the work term and the T d S term is the heat function. T d S is the energy unavailable for work. Therefore, d UT d S is the amount of internal energy available for work , or the free energy . We define it as A , the Helmholtz free energy:

(2.119) Geochemistry - изображение 253

As usual, we are interested in the differential form (since we are more interested in changes than in absolutes):

(2.120) or substituting eqn 258into 2120 2121 2112 Gibbs free energy - фото 254

or substituting eqn. 2.58into 2.120:

(2.121) 2112 Gibbs free energy 21121 Derivation The Gibbs free energy is - фото 255

2.11.2 Gibbs free energy

2.11.2.1 Derivation

The Gibbs free energy is perhaps misnamed. By analogy to the Helmholtz free energy, it should be called the free enthalpy (but enthalpy is an energy), because it is derived as follows:

(2.122) Geochemistry - изображение 256

and

(2.123) or which reduces to 2124 Notice the - фото 257

or

which reduces to 2124 Notice the similarity to the Helmholtz free energy - фото 258

which reduces to:

(2.124) Notice the similarity to the Helmholtz free energy in that case we subtracted - фото 259

Notice the similarity to the Helmholtz free energy; in that case we subtracted the TS term from the internal energy; in this case we subtracted the TS term from the enthalpy. The Gibbs free energy is the energy available for nonPV work (such as chemical work) . It has two other important properties: its independent variables are T and P , generally the ones in which we are most interested in geochemistry, and it contains the entropy term (as does the Helmholtz free energy), and hence can be used as an indication of the direction in which spontaneous reactions will occur.

2.11.2.2 Gibbs free energy change in reactions

For a finite change at constant temperature, the Gibbs free energy change is:

(2.125) The free energy change of formation is related to the enthalpy and entropy - фото 260

The free energy change of formation, is related to the enthalpy and entropy change of reaction 2126 Like - фото 261, is related to the enthalpy and entropy change of reaction:

(2.126) Like other properties of state the Gibbs free energy is additive Therefore - фото 262

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