Constraints on Formation History of Large Scale Lunar Topography from Observed Admittance: Viscous Relaxation with Lunar Thermal History

Details Constraints on Formation History of Large Scale Lunar Topography from Observed Admittance: Viscous Relaxation with Lunar Thermal History Constraints on Formation History of Large Scale Lunar Topography from Observed Admittance: Viscous Relaxation with Lunar Thermal History

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1322o&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1322

Physics

Scientific paper

The scale- and age-dependence of topographic relaxation of a cooling
viscoelastic sphere indicates that the 5000- km-scale (dichotomy scale)
topography of the Moon should be external origin and formed later than
100 m.y. from the lunar formation.

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