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Keywords

planets and satellites: dynamical evolution and stability
planet-star interactions

How to Cite

Creep Tides. A New Model to study the Tidal Evolution of Close-in Satellites and Exoplanets. (2014). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 44(1), 7-7. https://astronomia.unam.mx/journals/rmxac/article/view/2014rmxac..44....7f
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Abstract

New theory of the bodily tide problem based on only one physical law: the Newtonian creep. It shows that rocky and gaseous bodies do not respond to tidal stresses in the same way. Almost all results of the theory result from the creeping first-order differential equation.