Pits, Uplifts and Small Chaos Features on Europa: Morphologic and Morphometric Evidence for Intrusive Upwelling and Lower Limits to Ice Shell Thickness
Kelsi N. Singer, William B. McKinnon, Paul M. Schenk

TL;DR
This study analyzes Europa's surface features to estimate the ice shell thickness, suggesting a lower limit of 3-8 km based on geomorphological evidence of pits, uplifts, and chaos features.
Contribution
It provides new morphological and morphometric evidence supporting intrusive upwelling models and constrains Europa's ice shell thickness using detailed feature analysis.
Findings
Largest features are around 5-6 km in diameter
No pits smaller than 3.3 km in high-resolution images
Supports intracrustal sill models over melt-through models
Abstract
One of the clearest but unresolved questions for Europa is the thickness of its icy shell. Europa's surface is resplendent with geological features that bear on this question, and ultimately on its interior, geological history, and astrobiological potential. We characterize the size and topographic expression of circular and subcircular features created by endogenic thermal and tectonic disturbances on Europa: pits, uplifts, and small, subcircular chaos. We utilize the medium-resolution Galileo regional maps (RegMaps), as well as high-resolution regions, digital elevation models derived from albedo-controlled photoclinometry, and in some cases stereo-controlled photoclinometry. While limited in extent, the high-resolution images are extremely valuable for detecting smaller features and for overall geomorphological analysis. A peak in the size-distribution for all features is found at…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
