T238 The Age of Small World Exploration: Major Results from Minor Planets and Other Small Solar System Bodies

Wednesday, 7 November 2018
8:00 AM - 12:00 PM
Room 236-237

COULD FLOOR FRACTURES IN CERES CRATERS BE EVIDENCE OF SOLID STATE FLOW?

Paper number: T238-6
Program: Technical Sessions
Time: 9:20 AM – 9:35 AM

Authors

Abstract

The solid state flow model for Ceres [Bland et al., 2018] suggests that flow of a subsurface low viscosity and low density (LV-LD) material could be driven by differential loading brought about by the sudden removal of an overlying layer due to impact cratering. Preliminary models show that an impact into the edge of a layer of LV-LD material (presumably a mixture of ice, salts, and clathrate) within the Ceres crust can result in surface deformation of the crater wall [Bland et al., 2018]. Physical modeling of analog lobate flows suggests that the fractures might form as the subsurface LV-LD material flowed into the crater.

Ezinu, a 116 km crater located at 43.2ºN, 195.7ºE on Ceres, hosts a set of floor fractures. The primary trough is arcuate in shape, curving strongly to the east; it is 22.7 km long, 2.6 km wide, and up to 200 m deep. This trough wraps around a roughly circular topographic high that rises 514 m above the crater floor. Smaller fractures splay out from the primary trough mainly to the east, across the topographic high, while a few horsetail splays extend to the south from the western side of the trough. This pattern is comparable to the fracture pattern formed in the physical analog models.

Ezinu impacted into the northwestern flank of Hanami Planum, the only large discrete topographic rise on Ceres. This might explain why the eastern floor of Ezinu is generally higher than the western floor. However, it is also possible that the general raising of the crater floor in this area is due to an injection of a LV-LD material. In fact, since one hypothesis for the formation of Hanami Planum itself has been the intrusion of a lower density material [Scully et al., 2017], it might even be the source of LV-LD material.

There is a 13.6 km diameter crater within Ezinu that has been classified as a Class 4 floor-fractured crater [Buczkowski et al., 2018]. If an intrusion of LV-LD material resulted in the Ezinu fracturing, then it would most likely also cause the uplift of the floor and creation of subtle fractures within this smaller crater. It is possible that the moat observed within this crater is due to the impact melting of the ice within the LV-LD layer, creating a cryomagmatic sill that would inflate as it refroze, causing uplift of the floor. Further physical and numerical analyses are planned to better constrain the interpretation.

Geological Society of America Abstracts with Programs. Vol. 50, No. 6

doi: 10.1130/abs/2018AM-319463

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