Difference between revisions of "First Law of Thermodynamics"
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First Law of Thermodynamics
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A statement of the conservation of energy for thermodynamic
systems (not necessarily in equilibrium). The fundamental form requires that
the heat absorbed by the system serve either to raise the internal energy of
the system or to do work on the environment:
added per unit mass; du is the increment of specific internal energy;
and dw is the specific work done by the system on the environment.
Although dq and dw are not perfect differentials, their
difference, du, is always a perfect differential. Example of the
application of this equation: in an adiabatic free expansion of gas into a
vacuum, all three terms are zero.
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''For reversible processes the mechanical work is equal to the expansion
against the pressure forces, i.e.,
volume. For a perfect gas, the internal energy change is proportional to the temperature change,
at constant volume and T is the Kelvin temperature. Therefore, the form of the first law usually used in meteorological applications is
an alternative form,
heat at constant pressure.
For open systems the variation of total rather
than specific quantities is important:
internal energy; V is the volume; m is the mass of the system; and h is the
specific enthalpy.
If a system contains the possibility of nonmechanical
work, such as work done against an electric field, this work must be included
in the first law.
See second
law of thermodynamics, third
law of thermodynamics, energy
equations.
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References
This article is based on NASA's Dictionary of Technical Terms for Aerospace Use