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3      Thermodynamics and



                        Geothermal Systems






            Effective use of geothermal energy requires the ability to move heat efficiently. In some instances,
            heat is used to do work, as in the generation of electricity. In other cases, heat is either concentrated
            or dissipated. Regardless of the application, an understanding of the behavior of fluids and materials
            when heated or cooled, and the implications for energy balances, is the foundation for achieving an
            economically successful outcome for any geothermal application. This chapter provides an intro-
            duction to the elements of thermodynamics that are important for such considerations.


            The FIrsT law oF ThermodynamIcs: The eqUIValence oF
            heaT and work and The conserVaTIon oF enerGy

            conservaTion of enerGy
            By the second half of the 1700s, the engineering community had become intrigued by the repeat-
            edly observed fact that doing work on some materials generated heat. It was noted by Benjamin
            Thompson in 1798 that, in the process of making cannons, boring into metal resulted in the metal
            becoming very hot. A series of experiments he conducted (followed shortly by experiments by
            Humphrey Davy in 1799) demonstrated that mechanical work and heat were directly related. They
            and others eventually demonstrated that a given amount of mechanical work would result in the
            generation of a predictable amount of heat.
              However, it wasn’t until Julius Mayer published a seminal paper in 1842 that the concept of
              conservation of energy, as embodied in the equivalence of heat and mechanical work, was articu-
            lated. Although Mayer’s paper was the first to present the concept directly, it lacked sufficient
            experimental  grounding  and  mathematical  rigor  to  be  considered  an  adequate  demonstration
            of the equivalence of work and heat. In 1847 Hermann von Helmholtz developed a mathemati-
            cal basis for the concept. Then, in 1849 the thorough experimental and observational work of
            James Prescott Joule was presented to the Royal Society, in a paper entitled “On the Mechanical
            Equivalent of Heat.” These achievements established the concept that mechanical work and heat
            are equivalent and that, invariably, energy is conserved. This principle became the First Law of
            Thermodynamics.
              Simple statements of the First Law of Thermodynamics have been numerous, two of which are:

              Energy can neither be created nor destroyed
              All forms of energy are equivalent

            Internal energy
            The most rigorous description relies on the concept of internal energy, E. The E is a characteristic
            of a specific, defined system. A system can be a cylinder of gas, a bottle of water, a bar of steel, a
            rock—anything that can be physically described by parameters of state (such as temperature, T;
            pressure, P; volume, V; etc.). If a system is completely isolated from its surroundings (that is, it is
            a closed system, meaning no mass can move into or out of it) then at any given set of conditions
            (T, P), the internal energy E of the defined system is fixed and only depends on the properties of the
            materials of which the system is composed. The internal energy, E, will solely change in response to


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