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CATEGORIES:Class/Seminar
DESCRIPTION:Moons in the outer Solar System release heat as they orbit thei
 r host planets\, creating intense volcanism and subsurface water oceans. Ho
 wever\, few experimental constraints exist on the geodynamics of materials 
 under moonlike conditions\, limiting understanding of moon evolution and su
 bsurface deformation. This talk discusses the importance of understanding m
 oons from the microscale up\, using case studies about Io's volcanoes\, Enc
 eladus' core\, and brine infiltration into Europa's crust to show that geod
 ynamic modeling based on laboratory data is essential for interpreting resu
 lts from missions to the outer Solar System\, and also for using moons as a
  comparative laboratory for fundamental Earth processes.\n \n\nSpeaker-reco
 mmended reading: Seltzer\, C.\, Peč\, M.\, Zimmerman\, M. E.\, & Kohlstedt\
 , D. L. (2023). Melt network reorientation and crystallographic preferred o
 rientation development in sheared partially molten rocks. Geochemistry\, Ge
 ophysics\, Geosystems\, 24\, e2023GC010927. https://doi.org/10.1029/2023GC0
 10927
DTEND:20260122T210000Z
DTSTAMP:20260314T202948Z
DTSTART:20260122T200000Z
GEO:37.426402;-122.172635
LOCATION:Mitchell Earth Sciences\, 350/372
SEQUENCE:0
SUMMARY:Geophysics Seminar - Cassandra Seltzer\, "Micromechanisms of moon d
 eformation"
UID:tag:localist.com\,2008:EventInstance_51774920629052
URL:https://events.stanford.edu/event/geophysics-seminar-cassandra-seltzer-
 micromechanisms-of-moon-deformation
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