Tidal-Rotational Dynamics of Solar System Worlds, From the Moon to Pluto

The spins of planetary bodies are not stagnant; they evolve in response to both external and internal forces. One way a planet's spin can change is through true polar wander. True polar wander is the reorientation of a planetary body with respect to its angular momentum vector, and occurs when...

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Bibliographic Details
Main Author: Keane, James Tuttle
Other Authors: Matsuyama, Isamu, Malhotra, Renu, Hubbard, William B., Byrne, Shane, Richardson, Randall M.
Format: Doctoral or Postdoctoral Thesis
Language:English
Published: The University of Arizona. 2017
Subjects:
Online Access:http://hdl.handle.net/10150/625474