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...
Main Author: | |
---|---|
Other Authors: | , , , , |
Format: | Doctoral or Postdoctoral Thesis |
Language: | English |
Published: |
The University of Arizona.
2017
|
Subjects: | |
Online Access: | http://hdl.handle.net/10150/625474 |