Terrain Intelligence for Planetary Exploration

Integrating remote sensing, analog field studies, and terrain modeling across planetary environments.

Current Research

My research is grounded in planetary surface-process science, investigating how volcanic, fluvial, and aeolian processes shape planetary surfaces and how those processes can be quantified through field studies, geological mapping, quantitative morphometry, and geospatial interpretation. I combine orbital remote sensing, high-resolution terrain modeling, terrestrial analog field campaigns, and computational systems to analyze surface evolution on Mars, the Moon, and Earth at mission-relevant scales. As robotic and human exploration accelerates, this science supports collaborative mission teams to support operational safety and maximize scientific return.

Orbital Surface Analysis using Image and Digital Terrain Models

terrain analysis
Science-quality digital terrain models and quantitative analysis of Mars and the Moon at mission-relevant scales. Pictured: DTM showing a lava flow margin on the flank of Alba Mons, Mars.

Surface-Process Field Studies using Low Altitude Remote Sensing

Terrestrial volcanic and sedimentary process laboratories linking field measurements with orbital surface interpretation. Pictured: Litli-Hrútur eruption site, Iceland, seen from UAS.

Surface Intelligence using Real and Synthetic Terrain Systems

Geologically constrained synthetic landscapes and computational pipelines supporting surface analysis and interpretation, hazard assessment, and mission simulation. Pictured: Rim of Shackleton Crater, the Moon.

→ Go to Scientific Research

Affiliations

Contact

Email: scheidt [at] umd.edu
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