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Methods for Mapping Europa’s Bands through Time

Presentation Year
2026
Michelle
Selvans
Faculty
Geology
Sophia
Martin
Undergraduate Student
Geology
Janelle
Flores
Undergraduate Student
Geology
Cade
Napierala
Undergraduate Student
Geology
College or Department
College of Natural Resources & Sciences
Short Description of your Research or Creative Project (700 characters or less)
Of the Galilean moons circling Jupiter, Europa is the second closest and the smallest. It has attracted some interest from the scientific community, due to its subsurface ocean which is one of the most likely places to find life in our solar system, and its geologically young surface of ~100Myr. We use stratigraphic relationships as a means to understand the evolution of Europa’s ice shell surface over time. Tectonic motion drives changes in surface morphologies, divergence of the plate creates dilational features like bands and ridges, and convergence may cause subduction-like processes. We use ArcGIS to map and categorize surface features on Europa. We are able to place features in time steps and assign them morphologies that help understand spatial and temporal changes in stress state.
Permission to Publish Work
Yes
Presentation File Upload
Primary Contact: First Name
Liam
Primary Contact: Last Name
Hodgson
Primary Contact: Email
lh1721@humboldt.edu
Primary Contact: I am a
Undergraduate Student
Primary Contact: Phone Number
7076830795
Indicate File Dimensions
4'x3'