Talk:PlanetPhysics/First Law of Thermodynamics

Original TeX Content from PlanetPhysics Archive edit

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\begin{definition}
The amount of \htmladdnormallink{work}{http://planetphysics.us/encyclopedia/Work.html} required to change the state of an otherwise adiabatically isolated \htmladdnormallink{system}{http://planetphysics.us/encyclopedia/SimilarityAndAnalogousSystemsDynamicAdjointnessAndTopologicalEquivalence.html} depends only on the initial and final states, and not on the means by which the work is performed, or on the intermediate stages through which the system passes.
\end{definition}

\smallskip

\begin{remark}
Transformations between different \htmladdnormallink{equilibrium}{http://planetphysics.us/encyclopedia/ThermalEquilibrium.html} states can be achieved by applying work or \htmladdnormallink{heat}{http://planetphysics.us/encyclopedia/Heat.html} to the system. The first law states that both work and heat are forms of \htmladdnormallink{energy}{http://planetphysics.us/encyclopedia/CosmologicalConstant.html}, and that the total energy is conserved.
\end{remark}

\smallskip

\textbf{References}

This is a derivative work from [1] a \htmladdnormallink{Creative Commons Attribution-Noncommercial-Share Alike 3.0 work}{http://creativecommons.org/licenses/by-nc-sa/3.0/us/}

[1] MIT OpenCourseWare, 8.333 \htmladdnormallink{Statistical Mechanics I}{http://ocw.mit.edu/OcwWeb/Physics/8-333Fall-2007/LectureNotes/index.htm}: \htmladdnormallink{statistical mechanics}{http://planetphysics.us/encyclopedia/ThermodynamicLaws.html} of \htmladdnormallink{particles}{http://planetphysics.us/encyclopedia/Particle.html}, Fall 2007

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