Abstract

The intent of this thesis is to explore the pressure-sinkage relationship for simulated lunar regolith (simulant). The simulants used in this experiment emulate the lunar highlands (LHS-1) and the lunar mare (LMS-1). The ultimate ability of a terrain or regolith to support a load without shear failure is vital to the planning and construction of permanent infrastructure. This relationship can be measured by applying a normal load to the regolith until shear failure, from which allowable and ultimate bearing capacity can be deduced. An understanding of the pressure-sinkage of lighter loads on the higher ‘fluffy' layer of regolith is of great importance to low mass projects. The experimental hardware consisted of a test bed filled with simulated lunar regolith. The focus was to create a mechanism to apply a known load to a simulant surface normal to a square box filled with a regolith simulant. A known mass of each simulant was placed into the bearing capacity box and gently agitated to encourage natural settling and the density was measured. The simulant was only packed as much as was caused by gravity and settling. Normal loads of increasing weight were put into the box, putting pressure on the simulant. It was determined that widely accepted models for pressure-sinkage reasonably anticipate sinkage in both LHS-1 and LMS-1, though this study recommends improvements to the experimental design.

Thesis Completion

2023

Semester

Spring

Thesis Chair/Advisor

Britt, Daniel

Degree

Bachelor of Science (B.S.)

College

College of Sciences

Department

Physics

Degree Program

Physics

Language

English

Access Status

Open Access

Release Date

5-15-2023

Included in

Physics Commons

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