Planetary Orbital Evolution due to Tides
Orbital evolution of two objects experiencing tides
ExponentialDecayDiffRotBody.h File Reference

Declares a DissipatingBody with exponentially decaying differential rotation coupling. More...

#include "../Core/SharedLibraryExportMacros.h"
#include "../Evolve/DissipatingBody.h"
#include "../Evolve/ZoneOrientation.h"
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Classes

class  Star::ExponentialDecayDiffRotBody
 A body with differential rotation torque between two zones given by: \(\dot{L}_1=\frac{I_1 L_2 - I_2 L_1}{\tau_c(I_1+I_2)}\). More...
 

Detailed Description

Declares a DissipatingBody with exponentially decaying differential rotation coupling.

Definition in file ExponentialDecayDiffRotBody.h.