Research Interests
I use planetary geomorphological mapping paired with geodynamic computer modeling of icy worlds to better understand how the thermal and mechanical characteristics of ice shells affect topographic support and the mechanisms of transport within ice shells over geologic timescales.
Modeling Icy Moon Geodynamics 💻 Topographic Support ⛰️ Creep Mechanisms in Ice 🧊 Clathrates 🌋 Cryovolcanism 🪐 Geomorphological Mapping of Moons
Scroll down for examples and links!
Grants and Fellowships
2025 – 2028 NASA ROSES Precursor Science Investigations for Europa Grant: “Chaos Theory: Formation and Evolution of Chaos Terrain, and Prospects for Probing Interior Activity” PI: Fagents; Co-I: Schurmeier, L. $1.9 M
2024 – 2027 NASA ROSES Cassini Data Analysis Program: “Explaining Titan’s Topography: Modeling the Influence of Crustal Clathrates and Organics” PI: L. Schurmeier: $563,000
2024 – 2027 NASA ROSES Cassini Data Analysis Program: “Effects of Methane Clathrate on the Depth of Titan’s Craters” PI: Soderblom; Co-I: L. Schurmeier
2021 – 2024 NASA ROSES Cassini Data Analysis Program “The Influence of Clathrates on Titan’s Ice Shell” Science PI: L., Schurmeier: $247,000
2020 – 2023 NASA Astrobiology Institute Grant: “Habitability of Hydrocarbon Worlds: Titan and Beyond” PI: Lopes, R. Postdoc & Collaborator: Schurmeier, L.
2016 Illinois Space Grant Consortium Graduate Fellowship: $10,000
2015 Illinois Space Grant Consortium Graduate Fellowship: $10,000
2013 Illinois Space Grant Consortium Graduate Fellowship: $10,000
2017 Earth Educators Rendezvous Travel Grant: $400
2017 UIC Liberal Arts and Sciences Travel Grant: $250
Research Experience
2025 – present Assistant Researcher (HIGP, University of Hawai’i at Mānoa)
Modeling the lithosphere and topography of chaos terrain on Europa
Modeling the topographic relaxation of craters on Titan with clathrates
Explaining Titan's global topography: modeling topographic support mechanisms
2022 – 2025 Research Associate, Affiliate Faculty (HIGP, University of Hawai’i at Mānoa)
The Influence of Clathrates on Titan’s Thermo-Physical Behavior
Modeling the topographic relaxation of craters on Titan with clathrates
2020 - 2022 Postdoctoral Fellow (Advisor: Sarah Fagents, HIGP, University of Hawai’i at Mānoa)
NASA (NAI) Habitability of Hydrocarbon Worlds: Titan and Beyond Collaborator
Calculating Titan's brittle-ductile transition. Modeling transport mechanisms and limitations of cryovolcanism. Mapped potential expressions of cyrovolcanism.
Modeling the Formation of Gas-Driven Explosion Craters
Modeling the explosive release of methane trapped in destabilizing methane clathrates on Earth (Siberia) and Titan.
2012 - 2018 PhD Dissertation (Advisor: Andrew Dombard, University of Illinois at Chicago)
Mapped Titan’s radial labyrinth terrains and explored possible uplift mechanisms
Modeled the evolution and stability of titan’s large topographic loads
Modeled the viscoeastic relaxation of impact craters on Titan
2011 - 2014 Mars Icebreaker Landing Site Selection (J. Heldmann, C. McKay - NASA Ames)
2010 – 2012 Titan Tholin Experiments (B. Khare, C. McKay - NASA Ames)
2010 – 2011 Undergraduate Senior Thesis on Exoplanets (G. Laughlin - UC Santa Cruz)
Publications
Schurmeier, L. and Fagents, S., 2025. “Titan's Lithospheric Strength Envelope and Brittle-Ductile Transition: The Importance of Crustal Pore Fluids, Organics, and Clathrates” JGR Planets, 130(9), https://doi.org/10.1029/2025JE009118.
*Brouwer, G., Schurmeier, L., Fagents, S., Bray, V., Neish, C., Costello, E., 2025. “Topographic Relaxation of Complex Impact Craters in a Clathrate Crust on Titan” The Planetary Science Journal, 6(9), 217.
Schurmeier, L., Brouwer, G., Fagents, S., 2024. “Rapid Impact Crater Relaxation Caused by An Insulating Methane Clathrate Crust on Titan” The Planetary Science Journal, 5 (201), doi: 10.3847/PSJ/ad7018.
*Brouwer, G., Schurmeier, L., Fagents, S., 2024. An Endogenic Origin for Titan's Rampart Craters: Assessment of Explosion Mechanisms” JGR Planets, 129, doi: 10.1029/2024JE008459
Schurmeier, L., Dombard, 2024 “Unrelaxed Craters Muddy the Waters of the Dwarf Planet Ceres” Nature Astronomy News and Views, 8, 1352–1353, doi: 10.1038/s41550-024-02316-6
Schurmeier, L., Brouwer, G., Fagents, S., 2024 “Formation of the Siberian Yamal Gas Emission Crater via Accumulation and Explosive Release of Gas Within Permafrost” Permafrost and Periglacial Processes, 35(1), doi: 10.1002/ppp.2211.
Schurmeier, L., Dombard, A., Malaska, M., Fagents, S., Radebaugh, J., Lalich, D., 2023. “An Intrusive Cryomagmatic Origin for Northern Radial Labyrinth Terrains on Titan and Implications for the Presence of Crustal Clathrates ” Icarus, 404. doi: 10.1016/j.icarus.2023.115664
Schurmeier L. and Dombard, A. 2018 “Crater Relaxation Aided by Low Thermal Conductivity Sand on Titan” Icarus, 305, 314 – 323. doi: 10.1016/j.icarus.2017.10.034
Lalich, D., Poggiali, V., Hayes, A., Mastrogiuseppe, M., Malaska, M., Schurmeier, L., 2022. “Diverse Evolution of Mountains on Titan as Observed by the Cassini Radar Altimeter” Icarus, 347. doi: 10.1016/j.icarus.2021.114775
Malaska, M., Radebaugh, J., … Schurmeier, L., et al. 2020 “Labyrinth Terrain on Titan” Icarus. 344. doi: 10.1016/j.icarus.2020.113764
Jarmak, S., Leonard, E., … L. Schurmeier et al. 2020 "QUEST: A New Frontiers Uranus Orbiter Mission Concept Study" Acta Astronautica, 140, 6-26. doi: 10.1016/j.actaastro.2020.01.030
Heldmann, J., Schurmeier, L., Stoker, C., McKay, C., Davila, A. Marinova, M., Wilhelm, M. B. 2014 “Midlatitude ice-rich ground on Mars as a target in the search for evidence of life and for in situ resource utilization on human missions” Astrobiology, 14 (2), 102 -118. doi: 10.1089/ast.2013.1103
Our Science in the News
See a full list here
Comments on other science in the news:
Abstracts and Presentations
Schurmeier, L., and Brouwer G. Wakita, S., Soderblom J., Neish C., and Johnson, B. (2025) “Titan’s Methane Clathrate Crust Constrained by Combined Crater Impact and Relaxation Modeling” LPSC.
*Brouwer, G., Schurmeier, L., Fagents, S. (2025) “Topographic Relaxation of Complex Craters in Titan’s Clathrate Crust” LPSC.
Wakita, S., Johnson, B., Soderblom J., Neish C., Schurmeier, L., and Brouwer G. (2025) “A Methane Clathrate Layer Yields Shallow Craters on Titan” LPSC.
Soderblom, J., Wakita, S., Schurmeier, L., Brouwer, G, Johnson, B., Neish, C., Steckloff, J. K. (2024) “Effects of Methane Clathrate on the Depth of Titan’s Craters” AGU.
Neish, C., Wakita, S., Schurmeier, L., Brouwer, G, Johnson, B., Soderblom, J. (2024) “Effects of Methane Clathrate on the Depth of Titan’s Craters” DPS 56th.
*Brouwer, G., Schurmeier, L., Fagents, S., (2024) “Modeling Explosive Origins: Assessing Terrestrial Analogues for Titan’s Rampart Craters” Milos Planetary Analogues Workshop.
Schurmeier, L., Fagents, S., (2024) “Titan’s Lithospheric Strength Envelope and Brittle-Ductile Transition Depths” LPSC Abstract #2231.
Schurmeier, L., Brouwer, G., Fagents, S., Kay, J. P. (2023) "Titan’s Craters are Shallower than Ganymede’s: Is a Clathrate Crust the Culprit?" AGU.
Schurmeier, L., Brouwer, G., Fagents, S., (2023) "Formation of the Siberian Yamal Gas Emission Crater via Accumulation and Explosive Release of Gas Within Permafrost" AGU.
Schurmeier, L., Brouwer, G., Fagents, S., Kay, J. P., Marusiak, A., Vance S., (2023) “Crater Relaxation & Removal Caused by an Insulating Methane Clathrate Crust on Titan" LPSC (Talk).
*Brouwer, G., Schurmeier, L., Fagents, S., (2022) “Modeling Terrestrial Gas Emission Craters as Analogs for Titan’s Raised-Rim Depressions” LPSC.
Schurmeier, L., Brouwer, G., Fagents, S., (2021) “Explosive Gas Emission Craters on Earth: Possible Analog For Raised Rim Lakes On Titan” LPSC (Talk).
Lalich, D., Poggiali, V., Hayes, A., Schurmeier, L., Malaska, M. (2021) “Invisible Mounds: Observing The Earliest Stages Of Labyrinth Evolution On Titan With The Cassini Radar” LPSC.
*Brouwer, G., Fagents, S., Schurmeier, L. (2020) “Pressure-Driven Eruption of Liquid Reservoirs in Titan’s Ice Lithosphere” Fall AGU.
Lalich, D., Poggiali, V., Hayes, A., Schurmeier, L., Malaska, M. (2020) “New Observations Show the Earliest Stages of Titan’s Radial Labyrinth Terrain Evolution” Fall AGU.
Malaska, M., Schurmeier, L., Lopes, R., Schoenfeld, A., Solomonidou, A., Le Gall, A., Radebaugh, (2019) “Titan’s Radial Labyrinths” EPSC-DPS.
Jarmak, S., Leonard, E., Schurmeier, L., et al. (2018) “QUEST: A New Frontiers Uranus Orbiter Concept Study from the 30th Annual NASA/JPL Planetary Science Summer Seminar” OPAG.
Schurmeier, L. (2018) “Domed Labyrinth Terrains: What can they tell us about Titan’s ice shell?” Lunar and Planetary Institute (Invited Seminar).
Schurmeier, L., Dombard, A., Radebaugh, J., Malaska, M., (2018) “Intrusive and Extrusive Cryovolcanism and the Composition of Titan’s Icy Crust” LPSC Abstract # 2934 (Talk).
*Tremblay, S., Dombard, A., Schurmeier, L., (2018) “Global Lacunarity of Planetary Datasets: Methodology” LPSC Abstract #2460.
*Castillo, J., Dombard, A., Schurmeier, L., (2018) “Ceres’ Largest Craters: Age Analysis of Kerwan and Yalode” LPSC Abstract #2476.
Schurmeier, L., Dombard, A., Malaska, M., Radebaugh, J., (2017). “Are Titan’s radial Labyrinth terrains surface expressions of large laccoliths?” Fall AGU Abstract # 227212.
Malaska, M., Lopes-Gautier, R., Solomonido, A., Mitchel, K., Radebaugh, J., Schurmeier, L., Le Gall, A., (2017). “Is there a Laccolith Origin for Titan's Radial Labyrinths?” AOGS Abstract.
Schurmeier, L., Dombard, A., Radebaugh, J. (2016) “Titan’s Isolated Mountain Plateaus: Investigating Possible Support Mechanisms and Cryovolcanic Origins” LPSC # 2197 (Talk).
Schurmeier, L. and Dombard, A. (2015). “The Effects of Low Thermal Conductivity Sand on the Relaxation of Titan’s Impact Craters” LPSC Abstract # 2913.
Schurmeier, L. and Dombard, A. (2014). “Crater Relaxation Aided by Aeolian Infill on Titan” Titan Through Time Workshop (Talk).
Schurmeier, L., Heldmann, J., et al. (2013). “Midlatitude Ice-Rich Ground on Mars as a Target in the Search for Evidence of Life and for in situ Resource Utilization on Human Missions” Fall AGU Abstract # P23F-1856.
*Student researcher that I helped advise.
2020 – pres. Gwendolyn Brouwer, University of Hawai’i at Manoa (MS/ PhD) "Crater Relaxation on Titan," and "Modeling an Endogenic Origin for Raised Rim Depressions on Titan"
2017 - 2018 Sheri Trembley, University of Illinois at Chicago (undergraduate) “Lacunarity spatial analysis on global planetary scales: applied to Venus and the Moon”
2017 - 2018 John Castillo, University of Illinois at Chicago (undergraduate) “Crater counting to establish the ages of large impact basins on dwarf planet Ceres”
The thermal and compositional structure of a planetary interiors controls the brittle and ductile transport regimes within ice shells.
This is important for the search for signs of life (astrobiology) and cryovolcanism, and mission planning.
1. Organic-rich sand that collects within craters can act as a strong insulator and cause topographic relaxation.
2. Methane clathrate insulates Titan's ice and results in topographic relaxation that can reproduce the unexpectedly shallow depths of Titan's craters.
1. Setup for a model where insulating sand results in an increase in the effective surface temperature inside a crater bowl.
Axisymmetric finite element modeling. 1/2 of the crater is shown.
2. Results: Evolution crater topography for a 100 km diameter crater in a 10 km methane clathrate crust over 1 billion years. Arrows indicate current crater depths.
We found that gas pressure alone can reproduce the morphology of gas emission craters (GEC) in Siberia. Sudden warming periods can weaken permafrost and allow explosive release of gas trapped in the ice. We predict more GEC to form as our planet warms.
My student G. Brouwer also uses this as analog for similar raised-rim depressions on Titan.
Brouwer, G., Schurmeier, L., Fagents, S.