I am a geologist interested in the evolution of planetary surfaces. I use a combination of remote sensing observations, numerical modeling, and field work at analogue sites to study extraterrestrial landscapes, with the goal of advancing our understanding of how these landscapes came to be. My interest in planetary geomorphology is driven by two motivations. The three planets in or near the Solar System’s “Goldilocks zone” - Venus, Earth, and Mars – may have shared similar conditions early in Solar System history. The geologic record of Venus has been completely covered by volcanism and Earth’s has been erased or modified by billions of years of tectonism, volcanism, and erosion. Mars still retains a record from its early history, dating back to around the time that life first arose on Earth. This means that by studying ancient terrains on Mars we are in a way studying the environment of early Earth that gave rise to life. More broadly, the diverse settings of planetary surfaces across the Solar System provides an opportunity to use these as natural laboratories, allowing us to better understand the mechanisms behind landscape change. There is a synergy between terrestrial and planetary geoscience - studies of terrestrial analogue environments are necessary to better interpret planetary surface processes, and processes observed on extraterrestrial surfaces provide tests for geomorphic models developed for landforms on Earth.
Some highlights of projects I have worked on or am working on are listed below.
Mars
- Martian valley networks
- Demonstration that ~25% of valley network erosion was due to lake outlet floods
- Timescales of valley formation using crater counts and reconstruction of pre-valley surface
- Manuscript in preparation, see Morgan (2021) AGU Fall Meeting
- Global investigations of valley morphology using a semi-automated approach
- Evidence for multiple episodes of erosional activity in the Gale crater region
- Manuscript in preparation, see Law & Morgan (2020) AGU Fall Meeting
- Martian alluvial fans
- Global distribution of alluvial fans and putative deltas
- Detailed geomorphic and sedimentologic study of the alluvial fans in Saheki crater
- Landform evolution modeling of fine grained alluvial fan sedimentation
- Work in progress, see Morgan et al. (2017) LPSC)
- Estimating paleoflow discharge from remote sensing data
Earth
- Atacama Desert
- Studies of fine-grained alluvial fans as a Mars analogue
- Work in progress, see Morgan et al. (2021) Planetary Analogues Workshop
- Geomorphic response to a hundred year storm in the absolute desert
- Studies of fine-grained alluvial fans as a Mars analogue
- Hawaii
- Investigations of the provenance of basaltic sand dunes
- Manusript in preparation, see Craddock et al. (2019) LPSC
- Sieve lobe dominance of Hawaiian alluvial fans
- Investigations of the provenance of basaltic sand dunes
- Hawaii and Iceland
- Reconstructing basaltic sediment transport on Mars. Recently funded, field work is planned for 2022 and 2023.
- Simpson Desert, Australia
- Manuscript in preparation, see Craddock et al. (2021) Planetary Analogues Workshop
- Work in progress, see Kling et al. (2019) LPSC
- Northern Canada
- Manuscript in preparation, see Palucis et al. (2021) LPSC