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Henrik Lund is a Professor at Aalborg University in the Department of Sustainability and Planning under the Technical Faculty of IT and Design . He is an ISI Highly Cited researcher and Editor-in-Chief of Elsevier's journal Energy , which receives over 8000 annual submissions.
Martin Bizzarro is a Professor at the University of Copenhagen , affiliated with the Globe Institute and serving as Director of the Centre for Star and Planet Formation . He leads the STARPLAN section, focusing on cosmochemistry, astrophysics, and planetary science. Research Interests : His work centers on the earliest evolution of the Solar System through high-precision isotope ratio measurements in extraterrestrial materials. Key areas include linking meteoritic records to astrophysical models, nucleosynthetic processes in planetary formation, and volatile partitioning in rocky planets. Recent studies involve Martian mantle isotopes, asteroid Ryugu samples, and chondritic component analysis. Article Trends : His 15 most recent papers (2023–2025) cover topics like calcium/zirconium isotopes , protoplanetary disk dynamics , asteroid composition , and planetary differentiation , with methods including LA-MC-ICP-MS and U-Pb dating. Collaborations : He works with international teams on projects involving asteroid Ryugu , Mars meteorites , and chondrite analysis .
Anja C. Andersen is a Professor of Public Understanding of Science at the Niels Bohr Institute , University of Copenhagen, and leads research in astrophysics of dust. She supervises bachelor, master, and PhD students and has taught courses like Stars and Planets (Astro2) and Extragalactic Astrophysics (Astro4) . Education: Ph.D. in Astrophysics (1999), University of Copenhagen M.Sc. in Physics and Astronomy (1995), University of Copenhagen Diploma in Higher Education Teaching (2003) Leadership Training (2011) Research Interests revolve around cosmic dust in astrophysical environments, including its role in star/planet formation, interstellar medium dynamics, and galactic evolution. She combines observational studies, theoretical modeling, and laboratory experiments to explore dust properties and nucleosynthesis. Articles Trends show expertise in dust lifecycle ( HELGA studies), r-process elements in neutron star mergers (Nature 2019), and interstellar dust growth. Her work bridges astrophysics, cosmochemistry, and observational techniques. Scientific Awards include 21 honors, such as the 2022 Hørups Debatpris , 2014 Direktør N. Bang Scholarship , and 2004 National Danish Award for Public Outreach . Teaching & Supervision spans institutions like Uppsala University, with mentorship in the University of Copenhagen's network for young female scientists. She has supervised 4 PhD, 7 M.Sc., and 27 B.Sc. students.
Uffe Gråe Jørgensen is an Associate Professor at the Niels Bohr Institute , University of Copenhagen , specializing in Astrophysics and Planetary Research . His work bridges theoretical modeling with observational astrophysics, focusing on exoplanetary systems, sub-stellar atmospheres, and Galactic globular clusters. Current Affiliation: Niels Bohr Institute, University of Copenhagen Research Focus: Exoplanet dynamics, binary star systems, and atmospheric modeling Research Interests include: Exoplanet detection and orbital decay Self-consistent sub-stellar atmosphere models Cloud formation in extreme extraterrestrial environments Stellar evolution in binary systems Photometric analysis of dense stellar clusters Interplay of magnetic fields in solar-type stars Publication Trends show a strong emphasis on exoplanetary science, sub-stellar atmospheres, and Galactic structure studies, with methodological innovations in photometric and computational techniques. Contact Details: Email: uffegj@nbi.ku.dk Phone: +45 3532 5998 Location: Jagtvej 155A, Copenhagen N
Martin Elias Pessah is a Professor of Theoretical Astrophysics and the leader of the Theoretical Astrophysics Group at the Niels Bohr International Academy in the Niels Bohr Institute at the University of Copenhagen. He holds positions in both the Niels Bohr Institute and the Astrophysics and Planetary Research division. His academic journey began at the Facultad de Ciencias Astronomicas y Geofisicas at the Universidad Nacional de La Plata, continued with a PhD from the University of Arizona's Astronomy and Physics Departments, and included a membership at the Institute for Advanced Study in Princeton. Professor Pessah's research focuses on theoretical astrophysics with specific interests in accretion physics, magnetohydrodynamics, galaxy clusters, and black hole dynamics. His work bridges theoretical modeling with observational constraints, particularly in understanding the complex dynamics of astrophysical fluids and gravitational systems. His recent publications demonstrate a strong research trajectory in multiple areas of astrophysics, with notable contributions to understanding magnetic field amplification in accretion disks, gravitational-wave mergers in active galactic nuclei, and planet formation dynamics. The 2022 Nature publication on AGN as factories for eccentric black hole mergers represents a particularly significant contribution with 139 citations and coverage by 132 news outlets. Scientific Recognition: Published in Nature (2022) with 139 citations Research picked up by 132 news outlets Professor Pessah leads the Theoretical Astrophysics Group at the Niels Bohr International Academy, supervising research projects related to astrophysical fluid dynamics, black hole physics, and planetary formation. His research has attracted significant attention in the scientific community and broader media, indicating the importance and impact of his work in contemporary astrophysics. His laboratory and research environment at the Niels Bohr Institute provides a collaborative space for theoretical investigations into fundamental astrophysical processes, with connections to observational astronomy and computational physics.
Peter Stanley Jørgensen is a Senior Researcher in the Department of Energy Conversion and Storage at the Technical University of Denmark (DTU), specializing in advanced imaging techniques for energy materials characterization. His work spans multiple areas of materials science with a focus on energy applications. Dr. Jørgensen earned his M.Sc.(eng) from IMM at DTU between 1999 and 2006, followed by a research assistant position at the university from 2006 to 2007. His research interests include: 3D image analysis and acquisition techniques Scanning electron microscopy and X-ray tomography applications Microstructure analysis of energy conversion materials Solid Oxide Fuel Cells and related electrochemical systems Materials characterization for sustainable energy solutions Dr. Jørgensen's recent publications demonstrate a strong trend toward developing and applying advanced 3D imaging methodologies to understand materials at micro and nano scales, with particular emphasis on solid oxide cells, ceramic materials, and solar technology. His work combines experimental characterization with computational analysis to address challenges in energy materials. His scientific contributions support UN Sustainable Development Goals related to affordable and clean energy. Dr. Jørgensen actively supervises PhD students across multiple projects: N. M. Leal Reyes (Physics-informed Deep Learning for Energy Materials) Y. Shang (Phase field modeling of microstructure evolution) S. Pollok (Deep Learning for optimizing magnets) E. O. Brenne (Physical model priors for tomogram segmentation) His research is supported by numerous projects including the Marie Skłodowska-Curie actions and multiple DTU-funded initiatives focused on energy materials characterization and analysis.
دانشیار
Per Morgen is a Danish Associate Professor at the University of Southern Denmark’s Department of Physics and Chemistry, with adjunct roles in SDU Chemical Engineering. He holds a Doctor of Science degree and has led major surface analysis infrastructure development since 1991. Education: Cand.scient. (1969), lic.scient. (1978), dr.scient. (1991) in Physics and Chemistry from Århus University His research spans experimental surface science, nanotechnology, and materials for energy applications. Key areas include: Semiconductor surface physics Atomic-layer thin film growth Nanostructured Al2O3 templates Nanoparticle applications in fuel cells/solar cells Synchrotron radiation surface studies Biomedical polymer surface conditioning Hydrogen storage materials Recent work focuses on iridium-based electrocatalysts for water splitting, with collaborations spanning India, Japan, and Germany. He has supervised over 50 bachelor’s and master’s projects and 10 PhD theses. Grants and infrastructure development include: Carlsberg Foundation support (1970) Public-private funding for UHV surface labs FINST innovation consortium (2007-2009) EU LEONARDO LASTED.net project (2004-2007) He co-founded NanoS ApS in 2001 and maintains visiting professor status at the Indian Institute of Science since 2003, with notable work on tribological systems and educational technology.
دانشیار
Karen Pantleon is an Associate Professor in the Department of Civil and Mechanical Engineering at the Technical University of Denmark (DTU), specializing in Materials and Surface Engineering. Her work contributes to UN Sustainable Development Goals through advanced materials research for energy and industrial applications. Her research spans materials science with emphasis on surface engineering, corrosion mechanisms, microstructure evolution, and high-temperature processes. She employs X-ray diffraction and electrodeposition techniques to investigate phase transformations in Ti-Nb-Zr alloys and thermal stability of tungsten composites for nuclear fusion environments, alongside corrosion resistance in steel for solid oxide cell systems. Recent publications (2024-2025) demonstrate strong focus on energy materials, including photovoltaic efficiency enhancement through novel interfacial layers and long-term corrosion behavior in industrial alloys. Key trends involve microstructural restoration in embrittled tungsten composites and sustainable metallurgical processes. Scientific Awards: SOFT2024 PhD Poster Prize Winner (2024) Dr. Pantleon actively supervises four PhD students across major projects including "Martensitic Transformations in Ti-Nb-Zr alloys" and "Thermal Stability of Tungsten Fiber-reinforced Composites". Her research is funded by the Independent Research Fund Denmark and the "Green Steel UG" project for sustainable iron exploitation in Uganda, addressing critical challenges in fusion energy and green steel production. She leads key initiatives within DTU's Materials and Surface Engineering group, collaborating internationally on plasma-facing materials for fusion reactors and sustainable metallurgy solutions aligned with global decarbonization goals.
Austin Jarl Boyd is a Researcher at the Section for Geobiology within the Globe Institute, Faculty of Health and Medical Sciences, University of Copenhagen. His work centers on geochemical analysis of Earth's earliest geological formations, particularly the 3.7-billion-year-old Isua Supracrustal Belt in Greenland. His research expertise spans: Early Earth geochemical dynamics Isotope systematics of ancient rocks Plate tectonics onset in the Eoarchean Preservation of organic matter in primordial environments Geobiological signatures of early life Recent publications reveal groundbreaking findings: detrital sediments proving active plate tectonics 3.7 billion years ago, and amide groups preserved in ancient liquid inclusions. His work demonstrates exceptional methodological rigor in analyzing Earth's oldest geological records, with significant implications for understanding planetary evolution. His 2019 Geochimica et Cosmochimica Acta paper on tungsten isotopes has garnered 58 Scopus citations and media coverage, highlighting its impact on early Earth differentiation models. Collaborations with leading scientists like Minik Rosing and T. Hassenkam extend across international research networks. Dr. Boyd maintains active laboratory work at the Globe Institute, utilizing advanced geochemical instrumentation to investigate Earth's formative processes. His research program continues to explore the intersection of geology, chemistry, and early life signatures through ongoing fieldwork in Greenlandic Archean terrains.
Elishevah van Kooten is a Tenure Track Assistant Professor at the Centre for Star and Planet Formation within the Globe Institute at the University of Copenhagen. Her research focuses on understanding the formation and evolution of planetary systems, particularly through the study of meteorites and protoplanetary disks. Her research interests span planetary science, astrophysics, and meteoritics with particular emphasis on chondrites, isotopic analysis, and early solar system formation processes. Dr. van Kooten's work investigates the chemical and physical processes that shaped our solar system, including aqueous alteration of meteorites, nucleosynthetic heterogeneity, and the thermal processing of primordial materials. Analysis of her recent publications reveals a strong focus on cosmochemistry and meteorite analysis, with significant contributions to understanding the relationship between chondrules and matrix, metal compositions in carbonaceous chondrites, and the nucleosynthetic fingerprint in the protoplanetary disk. Her work bridges observational data with theoretical models of solar system formation. Dr. van Kooten has established collaborations with leading researchers across multiple institutions, as evidenced by her co-authorships on numerous high-impact publications in journals such as Space Science Reviews, Science Advances, and Astrophysical Journal.
Sebastian Herbert Lorek serves as an External Researcher and Academic employee at the Centre for Star and Planet Formation within the Globe Institute at the University of Copenhagen. He is a postdoctoral researcher in Anders Johansen's Planet Formation Group, focusing on computational astrophysics related to planetary system origins. His institutional base at Øster Voldgade 5-7, Copenhagen, supports his active research profile evidenced by multiple recent publications in high-impact journals. Dr. Lorek's research centers on numerical simulations of planet formation mechanisms, including gravitational collapse of pebble clouds, dynamics of planetesimal accretion, and formation pathways for Super-Earths in systems with cold giants. He investigates UV processing effects on icy pebbles in turbulent protoplanetary disks and develops computational methods for modeling planetesimal dynamics. His work bridges theoretical astrophysics and high-performance computing to address fundamental questions about planetary system evolution. Analysis of his 2020-2025 publications reveals consistent specialization in computational planet formation, with recurring themes in pebble accretion efficiency, disk-planet interactions, and turbulent disk dynamics. His research demonstrates methodological innovation in N-body simulations and hydrodynamical modeling, contributing to understanding diverse planetary architectures from early solar system evolution to exoplanet systems. No scientific awards were mentioned in the available information. Details regarding student advising or research grants were not provided in the source material. Dr. Lorek is an integral member of the Planet Formation Group at the Centre for Star and Planet Formation, collaborating with researchers including Anders Johansen, Michiel Lambrechts, and international co-authors. His work leverages advanced computational infrastructure to model complex astrophysical processes in protoplanetary environments.
پژوهشگر ارشد
Linru Fang is a Postdoctoral Researcher at the Centre for Star and Planet Formation within the Globe Institute at the University of Copenhagen, specializing in planetary formation processes and geochemical analysis of extraterrestrial materials. The research center focuses on interdisciplinary investigations of star and planet formation mechanisms through cosmochemical and astrophysical approaches. Research interests center on volatile element depletion in planetary bodies, with specific expertise in lunar interior geochemistry and carbonaceous meteorite analysis. Dr. Fang employs advanced mass spectrometry and computational modeling to investigate how impact events and thermal processes shaped the chemical evolution of the Moon and early solar system bodies. Key methodologies include isotopic ratio analysis and experimental simulation of high-temperature sublimation processes. Recent publications reveal consistent patterns in volatile depletion mechanisms across different planetary materials, demonstrating how impact-induced sublimation drives compositional changes in both lunar interiors and carbonaceous meteorites. This work establishes critical links between impact dynamics and chemical fractionation during planetary accretion. The Centre for Star and Planet Formation maintains active collaborations with international space agencies and meteorite research facilities, providing Dr. Fang access to cutting-edge analytical instrumentation and rare extraterrestrial samples for ongoing investigations into solar system formation.
Georgy Makhatadze serves as a Researcher at the Centre for Star and Planet Formation within the Globe Institute, Faculty of Health and Medical Sciences, University of Copenhagen. His work bridges cosmochemistry and planetary science through advanced isotope analysis of extraterrestrial materials. His research specializes in Planetary Science , Cosmochemistry , and Isotope Geochemistry , with emphases on nucleosynthetic processes in early Solar System materials. Key investigations include isotopic heterogeneity in meteorites, protoplanetary disk dynamics, and accretion mechanisms of terrestrial planets using nickel and silicon isotope systems. Makhatadze's 2023 publications in Nature and Geochimica et Cosmochimica Acta reveal critical constraints on planetary formation through high-precision isotope measurements. These studies demonstrate significant media impact (142+ news outlets) and academic engagement (50+ Mendeley readers), highlighting their importance in understanding Solar System evolution. He operates within the Centre for Star and Planet Formation, which maintains extensive collaborations with the Natural History Museum of Denmark and international research networks focused on stellar and planetary origins.
Martin Schiller is an Associate Professor in Geochemistry at the Globe Institute, Centre for Star and Planet Formation at the University of Copenhagen. His research focuses on understanding the earliest evolution of our Solar System through high-precision isotope ratio measurements in extraterrestrial materials. Dr. Schiller's primary research interests include the application of major element isotope systematics to link the meteoritic record to astrophysical theories and models of terrestrial planet formation, the short-lived isotope chronology of early Solar System solids, and high precision isotope measurements in terrestrial samples such as magnesium and calcium isotope records in speleothems. His work bridges cosmochemistry, planetary science, and geochemistry to unravel the formation and evolution of planetary systems. His recent research has examined calcium isotope evidence for early Solar System condensates, magnesium-iron-calcium isotope signatures of impact spherules, redox evolution of planetary mantles, and presolar heritage of titanium and aluminum isotopes in the protoplanetary disk. This work demonstrates his expertise in using isotope systems as tracers of fundamental processes in planetary formation and evolution. Dr. Schiller has published extensively in top journals including Geochimica et Cosmochimica Acta, Earth and Planetary Science Letters, Science Advances, and Nature Communications. His research has garnered significant attention, with multiple publications covered by news outlets and social media platforms.
