Rotational Stability of Dynamic Planets with Lithospheres

Details Rotational Stability of Dynamic Planets with Lithospheres Rotational Stability of Dynamic Planets with Lithospheres

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.2230m&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.2230

Physics

Scientific paper

We investigate the long term rotational stability of terrestrial planets
subject to surface mass and internal (convectively driven) loading. The
stability theory extends work by Willemann [1984] and is illustrated
with several case studies.

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