Dr. Peter L. Olson is a Research Professor at Johns Hopkins University's Department of Earth and Planetary Sciences. His research examines Earth's deep interior dynamics including core-mantle interactions, geomagnetic field generation, and planetary evolution processes. Research Focus: Combines theoretical models, numerical simulations, and laboratory experiments to study core dynamics, geodynamo processes, and mantle convection. Current investigations include the slow carbon cycle and polar ice shelf dynamics through interdisciplinary collaborations. Publications: Recent work explores geomagnetic reversal mechanisms, core-mantle boundary interactions, and planetary dynamo diversity using advanced computational models and fluid dynamics experiments. Education: Ph.D. from University of California, Berkeley
Amy Bonsor is an Official Fellow and Director of Studies in Natural Sciences (Physical) at Queens' College, University of Cambridge. Her academic work focuses on the intersection of astronomy and planetary science, particularly examining the composition and evolution of planetary systems through the lens of white dwarf pollution. Dr. Bonsor's research primarily centers on understanding the composition of exoplanetary material by studying polluted white dwarfs. Her work combines observational astronomy with theoretical modeling to investigate planetary debris disks, tidal interactions, and the geochemical signatures of accreted planetary material. She has made significant contributions to understanding how white dwarfs can serve as cosmic laboratories for studying the bulk composition of exoplanetesimals, including their differentiation processes and volatile content. Her recent publications reveal a strong emphasis on the chemical analysis of planetary material through white dwarf spectroscopy, with particular attention to mineralogy, elemental abundances, and the implications for planetary formation and evolution. She has pioneered approaches combining machine learning with traditional astronomical techniques to categorize and interpret white dwarf spectral data at scale. As Director of Studies in Natural Sciences at Queens' College, Dr. Bonsor plays a key role in undergraduate education within the Physical Sciences track of Cambridge's renowned Natural Sciences Tripos. Her leadership position indicates her standing within the Cambridge academic community and her commitment to nurturing the next generation of scientists.
Julian Lowman is a Professor at the University of Toronto Scarborough (UTSC), specializing in planetary interiors, mantle convection, and computational fluid dynamics. His research focuses on understanding the thermal and structural evolution of planetary mantles, core-mantle interactions, and high-performance numerical modeling techniques. He holds a Ph.D. from York University (1996) and contributes to advancing geodynamic simulations for terrestrial planets and moons. Key research interests include the mechanics of mantle convection, the role of viscosity and compositional variations, and the application of high-performance computing to model planetary processes. He has explored topics such as stagnant-lid convection, plate tectonic dynamics, and the thermal evolution of planetary cores and mantles. His work bridges computational methods with geophysical observations to address questions in Earth science and planetary science. Lowman’s publications span over three decades, addressing topics from Mercury’s mantle dynamics to exoplanet tectonics. His methodologies include advanced numerical models that simulate 2D and 3D convection patterns, fluid dynamics under Arrhenius viscosity regimes, and the influence of curvature on planetary interiors. He collaborates on projects involving mantle plumes, supercontinent cycles, and the interplay between surface tectonics and deep mantle structure. Despite his extensive contributions, no specific scientific awards or grants are explicitly listed in the provided texts. He advises no named students in the available data but likely contributes to graduate training at UTSC. His research aligns with interdisciplinary themes in computational geosciences and planetary evolution.
Maria Schönbächler is a Full Professor and Deputy Head of the Institute of Geochemistry and Petrology at ETH Zürich. Her research focuses on the formation of the Solar System and planets, with expertise in cosmochemistry, isotopic analysis, and meteorite studies. She leads projects on nucleosynthetic isotope anomalies, volatile element distribution, and planetary accretion processes. Her recent publications highlight isotopic studies of asteroid Ryugu samples, titanium and zirconium isotope heterogeneity, and volatile depletion in carbonaceous chondrites. Key themes include early solar system water circulation, presolar grain dynamics, and Hadean mantle evolution. Collaborations span planetary science, analytical chemistry, and astrophysics. Notable trends in publications: Isotopic constraints on planetary formation (Ryugu, Vesta, Earth's mantle) Volatile element mobility in meteorites and planetary bodies Protoplanetary disk heterogeneity and nucleosynthetic processes Advanced mass spectrometry techniques (MC-ICPMS, TIMS) Implications for solar system accretion and core formation
Scott King is a Professor of Geophysics at Virginia Tech's Department of Geosciences within the College of Science. His research focuses on planetary interiors, mantle convection, and tectonic processes, with emphasis on Mars, Venus, Mercury, and Ceres. He has contributed to NASA's InSight mission and the Dawn mission to Ceres. Key roles include advancing numerical methods for geodynamic modeling and studying mantle dynamics through seismic and computational approaches. Education: PhD in Geophysics from Caltech (1990), and dual B.A. degrees in Geophysical Sciences and Applied Mathematics from the University of Chicago (1985). Research Interests: King explores plate tectonics, planetary thermal evolution, and mantle flow using numerical simulations. His work includes analyzing seismic data from Mars (via InSight), Venusian coronae formation, and Mercury's thermal evolution. He also develops computational tools for 3D convection modeling. Recent Article Themes: Articles focus on Mars' core-mantle boundary, mantle plumes on Venus, and Earth's North American plate dynamics. Methodological advancements include comparing convection codes (ASPECT vs. CitcomS) and optimizing fault implementation in numerical models. Awards: Fellow of the Geological Society of America (2018) Alexander von Humboldt Research Award (2009) University Faculty Scholar, Purdue University (2004–2007) Advising & Grants: Mentors students studying Venus resurfacing, Mars volcanism, and Mercury's thermal evolution. His computational methods have been supported by grants and fellowships, including Argonne National Laboratory and Scripps Institution collaborations. Labs/Teams: Research group specializes in planetary geodynamics, with active projects on mantle convection, seismic analysis, and mission-related data interpretation (e.g., InSight).
Michael Thorne is an Associate Professor in the Department of Geology & Geophysics at the University of Utah, where he has been faculty since July 2014. His research focuses on using seismology to investigate Earth's structure, with specialization in mapping seismic structure of the deep mantle and developing numerical techniques for seismic wave propagation modeling. He teaches courses in geophysics, the dynamic Earth, and seismology. Dr. Thorne's educational background includes: B.S. in Physics from Indiana University Bloomington (1991-1996) Ph.D. in Geological Sciences from Arizona State University (2000-2005) His primary research interests span global seismic wave propagation, Earth's deep interior structure, and the dynamics of the core-mantle boundary region. Dr. Thorne specializes in studying ultra-low velocity zones (ULVZs), D" discontinuity structure, and seismic array processing techniques. His work combines advanced waveform modeling with seismic observations to understand Earth's deep structure and dynamics, including connections between deep mantle features and surface geology. Dr. Thorne's recent publications demonstrate a consistent focus on ultra-low velocity zones at the core-mantle boundary, with increasing sophistication in modeling techniques. His work has evolved from basic detection of ULVZs to detailed characterization of their morphology, elastic properties, and potential origins. Recent papers incorporate advanced Bayesian inversion methods and multidimensional modeling to better understand these enigmatic features and their implications for Earth's thermal and chemical evolution. Dr. Thorne actively mentors graduate students through thesis research courses and has secured numerous research grants to support his work. His current projects include: "Mapping the Lateral Variability of Groundwater Input into the Great Salt Lake Using Electrical Methods" (2024-2025) "NSFGEO-NERC: Advancing Capabilities to Model Ultra-Low Velocity Zone Properties Through Full Waveform Bayesian Inversion" (2024-2027) "The Future of Glaciers Using a Novel, Interdisciplinary Approach" (2024-2026) "Global Search for D Discontinuity Structure" (2022-2026) His research group utilizes advanced computational methods and collaborates with institutions worldwide to investigate Earth's deep interior structure using seismic observations and modeling.
Dr. Yanhao Lin is a Visiting Research Fellow at the Department of Geology and Geochemistry, Faculty of Science, Vrije Universiteit Amsterdam. His research focuses on experimental geochemistry and mineral physics, particularly magma dynamics, oxygen fugacity effects, and hydrogen transport in Earth's interior. He collaborates with institutions globally, contributing to understanding planetary evolution and mantle processes. Research Interests: Magma ocean dynamics and early Earth differentiation Hydrogen partitioning in magmatic systems Oxygen fugacity control mechanisms Subduction zone water transport Lunar basalt formation processes Recent work highlights experimental studies on lunar mare basalts (2025), magma ocean melting (2024), and core-mantle boundary hydration (2022). His studies integrate high-pressure experiments with computational modeling to address fundamental geodynamic questions. No scientific awards explicitly listed. Supervised 1 PhD thesis but no student names provided. Collaborations include researchers from institutions like Carnegie Institution (Mao), University of Tokyo (Katsura), and ETH Zurich (Walter).
Steven Jacobsen is a Professor of Earth and Planetary Sciences at Northwestern University’s Weinberg College of Arts & Sciences. He holds a Ph.D. in Geophysics, M.S. in Geology, and B.A. in Geology from the University of Colorado. His research focuses on high-pressure mineral physics, exploring the properties of materials under extreme conditions to understand Earth’s interior and develop novel energy and construction materials. Jacobsen leads studies on water cycling in the mantle, hydrous minerals, and planetary materials science, utilizing advanced facilities like the Advanced Photon Source and Sandia National Laboratories’ Z machine. He serves as Director of Graduate Recruitment, shaping the department’s graduate program. Research interests include mineral elasticity, phase transitions, and applications in geophysical and planetary contexts. Notable projects involve electrodeposition for marine construction and NASA collaborations for off-world regolith utilization. Jacobsen’s work bridges fundamental science and practical innovation, addressing low-carbon technologies and planetary exploration. His recent publications highlight advancements in ferropericlase inclusions, superdeep diamonds, and tunable materials. Collaborations with industry and space agencies underscore his interdisciplinary impact.
Jie Li is the Rodney C. Ewing Collegiate Professor of Earth and Planetary Sciences and Professor of Earth and Environmental Sciences at the University of Michigan. She holds a Ph.D. in Earth and Planetary Sciences (Harvard University, 1998) and an M.A. in Geophysics (Harvard University, 1997). Her research focuses on Earth and planetary materials under extreme conditions, leveraging high-pressure techniques like diamond-anvil cells and synchrotron facilities. Key interests include terrestrial planet evolution, core composition, and dynamics of planetary interiors. Recent studies explore light elements in Earth’s core, Mercury’s magnetic field origin, and early Earth crust formation. Her work bridges experimental geochemistry, mineral physics, and computational modeling to understand planetary interiors. Notable contributions include pioneering studies on iron spin states in the lower mantle and the role of metallic melts in mantle dynamics. She collaborates globally, advancing methodologies for high-pressure experiments. Her research has been featured in outlets like Mashable India , highlighting her insights on Earth’s core dynamics and planetary science. Li’s lab emphasizes interdisciplinary approaches to unraveling the origins of planetary materials and their evolution over geological time.
Dr. Khuliso Masindi serves as a Lecturer at the School of Geosciences, University of the Witwatersrand, contributing to academic instruction and research within South Africa's premier geoscience education framework. His educational foundation was entirely cultivated at the University of the Witwatersrand through sequential attainment of a BSc, BSc (Hons), MSc, and PhD degrees, establishing deep institutional expertise. Research interests span core geoscience disciplines with emphasis on: Geology: Earth's structural composition and historical evolution Earth Sciences: Integrated planetary systems analysis Environmental Geoscience: Human-geosphere interactions Hydrogeology: Subsurface water dynamics and contamination Mineralogy: Crystallographic properties and mineral classification Petrology: Rock formation processes across geological timescales No scientific awards, student supervision records, research grants, or laboratory affiliations were documented in the available profile, though his academic trajectory indicates active engagement in geoscience scholarship.
Dr. Zhaoxia Pu is a Professor in the Department of Atmospheric Sciences at the University of Utah and an Adjunct Professor at the School of Computing . Recognized as a Fellow of both the American Meteorological Society and the Royal Meteorological Society, she serves on the NOAA Science Advisory Board and has led 38 federally funded projects from agencies including NOAA, NASA, NSF, DOE, and ONR. Specializes in numerical weather prediction , data assimilation , and AI/machine learning for high-impact weather systems Developed advanced methods integrating satellite/radar data (GOES-R, CYGNSS, TROPICS) with Earth system models (UFS, E3SM, WRF) Recipient of the 2024 Excellence in Research Award and 2023 Provost's Banner Project recognition Research Trends : Her recent publications focus on: Machine learning approaches for precipitation retrieval using GOES-R data Cold fog microphysics and visibility parameterization in complex terrain Tropical cyclone dynamics through radar and lidar data assimilation Boundary layer turbulence in landfalling storms Drought mechanisms linked to synoptic-scale circulation New particle formation in mountainous regions Scientific Leadership : Lead scientist for CFACT NSF field campaign (2021–2025) Editorial board member of leading journals Active reviewer for NSF, DOE, NOAA, and NASA Teaching & Mentorship : Teaches Numerical Weather Prediction , Atmospheric Dynamics , and Introduction to Atmospheric Sciences courses. Has supervised 28 graduate students to completion.
Andre Izidoro is an Assistant Professor in the Department of Earth, Environmental and Planetary Sciences at Rice University. His research focuses on planetary dynamics, solar system formation, and exoplanetary systems. He investigates topics such as terrestrial planet accretion, giant planet instabilities, and the evolution of asteroid belts. His work integrates numerical simulations with observational data to understand planetary system architectures and formation mechanisms. Key research interests include the role of dynamical instabilities in shaping planetary systems, the accretion processes of giant planets like Uranus and Neptune, and the formation of super-Earths and mini-Neptunes. He also explores the delivery of volatiles to terrestrial planets and the effects of planetary migration on system evolution. His publications highlight contributions to understanding the asteroid belt's primordial mass, the implications of Jupiter's migration for inner solar system dynamics, and the formation mechanisms of planetary systems via pebble accretion and resonant chain disruption. Recent work addresses exoplanet radius valley formation, wide-orbit planet origins, and the survival of planetary satellite systems under dynamical perturbations. Dr. Izidoro's research has been published in leading astrophysics journals and presented at international conferences. His work is supported by computational modeling and collaboration with observational astronomers.
James Owen is a Reader in Astrophysics at the Department of Physics within the Faculty of Natural Sciences at Imperial College London. He holds a Senior Royal Society University Research Fellowship and previously served as a Hubble Fellow at the Institute for Advanced Study in Princeton and a CITA Fellow in Toronto. His research focuses on planet formation, extrasolar planets, and accretion disc physics, with particular emphasis on atmospheric escape mechanisms and protoplanetary disc structures. He is affiliated with the Astrophysics Group and the Physics Permanent Researchers at Imperial College. His key research interests include understanding how close-in super-Earths and mini-Neptunes form and evolve under intense stellar irradiation, driving atmospheric evaporation. He also investigates structures in protoplanetary discs observed via high-resolution imaging, linking these to planet formation processes. His work combines analytic theory and simulations to study hydrodynamic instabilities and disc dynamics. Notable awards include the Hubble Fellowship and CITA Fellowship. His recent work highlights the role of disc photoevaporation on giant planet migration and the observational signatures of embedded planets. He actively contributes to missions like JWST and UV-SCOPE for exoplanet characterization. Key affiliations: Astrophysics Group, Physics Permanent Researchers, Physics of Universe Labs: Blackett Laboratory at South Kensington Campus Future research directions include analyzing the growing dataset of protoplanetary discs and advancing models of exoplanet atmospheric evolution through neural network emulations.
David A. Neufeld is a Professor in the William H. Miller III Department of Physics & Astronomy at Johns Hopkins University (JHU), part of the Krieger School of Arts & Sciences. He holds a PhD from Harvard University and specializes in theoretical astrophysics, molecular astrophysics, and interstellar medium (ISM) studies. His research utilizes advanced observatories like the Herschel Space Observatory and SOFIA (Stratospheric Observatory for Infrared Astronomy), focusing on molecular line emission, cosmic ray ionization rates, and hydride molecules in diffuse clouds. Key projects include leading the HyGAL SOFIA Legacy Program to study hydrides in the Galactic ISM and participating in Herschel’s HEXOS, PRISMAS, and WISH Guaranteed Time programs. Neufeld has developed experimental methods to constrain sexaquark dark matter and contributed to the discovery of the helium hydride ion (HeH+) in planetary nebulae. He is also involved in GUSTO, a terahertz spectroscopic mission mapping [CII] and [NII] emissions. His research integrates observational astronomy with theoretical models, exploring topics like protostellar outflows, water ice chemistry, and shock dynamics. He has published extensively on infrared/submillimeter spectroscopy, molecular ion abundances, and the role of cosmic rays in interstellar chemistry. Neufeld’s work bridges laboratory experiments (e.g., dissociative recombination studies) with astrophysical observations, advancing understanding of the ISM and star formation processes.
Dr. Alex J. Evans is the Thomas J. and Alice M. Tisch Assistant Professor of Earth, Environmental, and Planetary Sciences at Brown University . His research focuses on planetary dynamics, lunar and rocky planet evolution, and the integration of geophysical data with mission insights. He holds a BS from the University of Michigan (2006), and a MS/PhD from MIT (2013). Affiliations: LunaSCOPE , NASA SSERVI Teaching: Courses on planetary surface processes, gravitational fields, and comparative solar system geology Expertise: Impact cratering, core dynamo evolution, and mission data analysis (e.g., GRAIL, MESSENGER) His research interests span lunar compositional asymmetry, Mercury’s geologic history, and the dynamics of metallic worlds like Psyche. Articles emphasize GRAIL mission findings, Mercury’s volcanic evolution, and comparative analyses of inner solar system bodies. His work bridges field observations, computational models, and space mission data to address fundamental questions about planetary formation and evolution. Grants and partnerships include over $10M in NASA-funded research leadership. He advises on lunar innovation strategies and public engagement in space science. Labs/Teams: Active collaboration with NASA mission teams and planetary science consortia.
