Iris van Zelst

ORCID: 0000-0003-4698-9910
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About
Contact & Profiles
Research Areas
  • earthquake and tectonic studies
  • Planetary Science and Exploration
  • High-pressure geophysics and materials
  • Geological and Geochemical Analysis
  • Astro and Planetary Science
  • Seismology and Earthquake Studies
  • Seismic Imaging and Inversion Techniques
  • Geological and Geophysical Studies
  • Geological Studies and Exploration
  • Geology and Paleoclimatology Research
  • Methane Hydrates and Related Phenomena
  • Space Exploration and Technology
  • Scientific Computing and Data Management
  • Hydrocarbon exploration and reservoir analysis
  • Geological Modeling and Analysis
  • Earthquake Detection and Analysis
  • Space Science and Extraterrestrial Life
  • Marine animal studies overview
  • Geotechnical and Geomechanical Engineering
  • CO2 Sequestration and Geologic Interactions
  • Computational Physics and Python Applications
  • Geological formations and processes
  • Phase Equilibria and Thermodynamics
  • Data Visualization and Analytics
  • Earthquake and Tsunami Effects

Deutsches Zentrum für Luft- und Raumfahrt e. V. (DLR)
2019-2025

Technische Universität Berlin
2023-2024

University of Leeds
2017-2023

ETH Zurich
2019-2022

Czech Academy of Sciences, Institute of Geophysics
2021

California Institute of Technology
2021

Utrecht University
2021

Centre for the Observation and Modelling of Earthquakes, Volcanoes and Tectonics
2020

Jet Propulsion Laboratory
2019

The September 2018, $$M_w$$ 7.5 Sulawesi earthquake occurring on the Palu-Koro strike-slip fault system was followed by an unexpected localized tsunami. We show that direct earthquake-induced uplift and subsidence could have sourced observed tsunami within Palu Bay. To this end, we use a physics-based, coupled earthquake–tsunami modeling framework tightly constrained observations. model combines rupture dynamics, seismic wave propagation, propagation inundation. scenario, featuring sustained...

10.1007/s00024-019-02290-5 article EN cc-by Pure and Applied Geophysics 2019-08-22

Abstract Taking the full complexity of subduction zones into account is important for realistic modeling and hazard assessment zone seismicity associated tsunamis. Studying requires numerical methods that span a large range spatial temporal scales. We present first coupled framework resolves dynamics over millions years earthquake down to fractions second. Using two‐dimensional geodynamic seismic cycle (SC) model, we model 4 million followed by cycles spontaneous megathrust events. At...

10.1029/2019jb017539 article EN cc-by Journal of Geophysical Research Solid Earth 2019-09-02

Abstract It has long been recognized that sediments subducting along the megathrust influence occurrence of giant ( M w ≥ 8.5 ) earthquakes. However, limited observation span and concurrent multiple parameters on behavior prevent us from understanding how affect earthquake size frequency. Here, we address these limitations by using two‐dimensional, visco‐elasto‐plastic, seismo‐thermo‐mechanical numerical models to isolate sediment thickness affects subduction geometry seismicity. Our results...

10.1029/2019jb018964 article EN Journal of Geophysical Research Solid Earth 2020-06-15

Abstract. Geodynamic modelling provides a powerful tool to investigate processes in the Earth's crust, mantle, and core that are not directly observable. However, numerical models inherently subject assumptions simplifications on which they based. In order use review studies appropriately, one needs be aware of limitations geodynamic as well its advantages. Here, we present comprehensive yet concise overview process applied solid Earth from choice governing equations methods, model setup,...

10.5194/se-13-583-2022 article EN cc-by Solid Earth 2022-03-17

Abstract Intermediate‐depth earthquakes (focal depths 70–300 km) are enigmatic with respect to their nucleation and rupture mechanism the properties controlling spatial distribution. Several recent studies have shown a link between intermediate‐depth thermal‐petrological path of subducting slabs in relation stability field hydrous minerals. Here we investigate whether structural characteristics incoming plates can be correlated seismicity rate. We quantify 17 by estimating maximum fault...

10.1029/2018gl081585 article EN Geophysical Research Letters 2019-03-22

SUMMARY How does megathrust earthquake rupture govern tsunami behaviour? Recent modelling advances permit evaluation of the influence 3-D dynamics on genesis, propagation, and coastal inundation. Here, we present explore a virtual laboratory in which source arises from coseismic seafloor displacements generated by dynamic model. This is achieved linking open-source computational models that follow discontinuous Galerkin schemes are facilitated highly optimized parallel algorithms software....

10.1093/gji/ggaa484 article EN cc-by Geophysical Journal International 2020-10-08

Abstract Detailed imaging of accretionary wedges reveals splay fault networks that could pose a significant tsunami hazard. However, the dynamics multiple activation during megathrust earthquakes and consequent effects on generation are not well understood. We use 2‐D dynamic rupture model with complex topo‐bathymetry six curved geometries constrained from realistic tectonic loading modeled by geodynamic seismic cycle consistent initial stress strength conditions. find all faults...

10.1029/2022jb024300 article EN cc-by Journal of Geophysical Research Solid Earth 2022-07-14

STEM fields in Europe and across the globe are not balanced terms of gender, ethnic racial groups, sexual orientation other aspects diversity (e.g. Fry et al. 2021, Freeman 2018). For example, 2018, women made up over 40% European academic staff, but 2019 only 26.2% full professors were women, less than 25% heads institutes, 31.1% board members (EC She figures 2021). This under-representation has caused institutions to implement new hiring practices, unconscious bias training, intervention...

10.5194/egusphere-egu25-5760 preprint EN 2025-03-14

In 2024, we published QUARTETnary - the card game about geological time scale with help of almost 400 Kickstarter backers. QUARTETnary, players collect sets four cards belonging to a certain unit aim obtaining most complete line win game. Consisting 60 beautifully illustrated and colourful cards, has explore all important events in Earth’s history: from dinosaurs humans formation Alps Himalayas.As January 2025, backers have received their games, meaning that people around world are...

10.5194/egusphere-egu25-11714 preprint EN 2025-03-14

Science Sisters is a YouTube video and seminar series hosted by Dr. Iris van Zelst. Lighthearted in tone, it explores different career paths, academic life, science communication the planetary geosciences. The guests on show represent range of role models to celebrate diversity people working STEM. They are interviewed their personal experiences topics. Past seasons have included topics like ethical fieldwork, switching careers, communication, postdoc leadership, women science, job...

10.5194/egusphere-egu25-6963 preprint EN 2025-03-14

Venus is often called Earth’s sister planet due to its similar size and mass. Apart from that, however, the two planets are wildly different, with surface temperatures on that easily melt lead a Venusian pressure almost hundred times larger than of Earth. Additionally, completely covered in clouds; obscuring shrouding entire mystery. How did observed topographic features form? Is there still some form tectonics ongoing? Are earthquakes - or indeed:...

10.5194/egusphere-egu25-6949 preprint EN 2025-03-14

The deployment of surface seismometers on the Moon and Mars has demonstrated their ability to recover both internal structure seismicity these planetary bodies.However, planets with dense atmospheres extreme conditions like Venus, deployed at face significant challenges, including short measurement durations due high temperature limitations electronics elevated background noise ground deformations generated by atmospheric dynamics. However, relatively unconstrained Venus is an important...

10.5194/egusphere-egu25-6634 preprint EN 2025-03-14

Warm rocky exoplanets within the habitable zone of Sun-like stars are favoured targets for current and future missions. Theory indicates these planets could be wet at formation remain long enough life to develop. However, it is unclear what extent an early ocean on such worlds influence response potential biosignatures. In this work we test climate-chemistry response, maintenance, detectability biosignatures in warm, water-rich atmospheres with Earth biomass fluxes framework planned LIFE...

10.5194/egusphere-egu25-16449 preprint EN 2025-03-15

The past decade has seen the consolidation of open access practices in scientific publishing, with funding bodies, international agencies and academic institutions requiring free to not only papers but also other output such as datasets computer codes. transition led multiple publishers offer Gold Open Access (GOA) schemes, under which are free-to-read. Compared traditional publication models, GOA comes at a much higher cost for authors. These have had documented negative impact on...

10.5194/egusphere-egu25-16049 preprint EN 2025-03-15

The September 2018, Mw 7.5 Sulawesi earthquake occurring on the Palu-Koro strike-slip fault system was followed by an unexpected localized tsunami. We show that direct earthquake-induced uplift and subsidence could have sourced observed tsunami within Palu Bay. To this end, we use a physics-based, coupled earthquake-tsunami modeling framework tightly constrained observations. model combines rupture dynamics, seismic wave propagation, propagation inundation. scenario, featuring sustained...

10.31223/osf.io/3bwqa preprint EN EarthArXiv (California Digital Library) 2019-02-16

Physics-based dynamic rupture models capture the variability of earthquake slip in space and time can account for structural complexity inherent to subduction zones. Here we link tsunami generation, propagation, coastal inundation with 3D (DR) initialized using a 2D seismo-thermo-mechanical geodynamic (SC) model simulating both dynamics seismic cycles. We analyze total 15 subduction-initialized rupture-tsunami scenarios which source arises from time-dependent co-seismic seafloor...

10.3389/feart.2021.626844 article EN cc-by Frontiers in Earth Science 2021-06-24

Abstract Venus is a terrestrial planet with dimensions similar to the Earth, but vastly different geodynamic evolution, recent studies debating occurrence and extent of tectonic‐like processes happening on planet. The precious direct data that we have for very little, there are only few numerical modeling concerning lithospheric‐scale processes. However, use models has proven crucial our understanding large‐scale Earth. Therefore, here adapt 2D thermomechanical rifting Earth study how...

10.1029/2022je007588 article EN Journal of Geophysical Research Planets 2023-03-01

Abstract. Geodynamic modelling provides a powerful tool to investigate processes in the Earth's crust, mantle, and core that are not directly observable. However, numerical models inherently subject assumptions simplifications on which they based. In order use review studies appropriately, one needs be aware of limitations geodynamic as well its advantages. Here, we present comprehensive, yet concise overview process applied solid Earth, from choice governing equations methods, model setup,...

10.5194/se-2021-14 article EN cc-by 2021-02-18

Abstract Byrne and Krishnamoorthy (2022), https://doi.org/10.1029/2021je007040 estimated the frequency of volcanic eruptions on Venus by scaling eruption obtained from a database containing Earth data. In reproducing their study, I found that number new ongoing in given year is approximately 42, instead previously reported 120 eruptions. This updated estimate (2022) based assumption data can be scaled to an important step toward quantifying volcanism Venus. However, it note this estimate,...

10.1029/2022je007448 article EN Journal of Geophysical Research Planets 2022-11-23

There is a growing consensus that Venus seismically active, although its level of seismicity could be very different from Earth due to the lack plate tectonics. Here, we estimate upper and lower bounds on expected annual by scaling Earth. We consider factors for tectonic settings account seismogenic zone thickness Venus. find 95 - 296 venusquakes equal or bigger than moment magnitude (Mw) 4 per year are an inactive Venus, where global rate assumed similar continental intraplate For active...

10.31223/x5dq0c preprint EN cc-by EarthArXiv (California Digital Library) 2023-03-31

The relatively unconstrained internal structure of Venus is a missing piece in our understanding the Solar System formation and evolution. To determine seismic Venus’ interior, detection waves generated by venusquakes crucial, as recently shown new geodetic constraints on Mars’ interior obtained InSight mission. In next decades multiple missions will fly to explore its tectonic volcanic activity, but they not be able conclusively report seismicity or detect actual waves.Looking towards fleet...

10.22541/essoar.171286367.76819789/v1 preprint EN Authorea (Authorea) 2024-04-11

Abstract There is a growing consensus that Venus seismically active, although its level of seismicity could be very different from Earth due to the lack plate tectonics. Here, we estimate upper and lower bounds on expected annual by scaling Earth. We consider factors for tectonic settings account seismogenic thickness Venus. find 95–296 venusquakes equal or bigger than moment magnitude ( M w ) 4 per year are an inactive Venus, where global rate assumed similar continental intraplate For...

10.1029/2023je008048 article EN cc-by Journal of Geophysical Research Planets 2024-07-01

Abstract Subducted sediments are thought to lubricate the subduction interface and promote faster plate speeds. However, global observations not clear‐cut on relationship between amount of motion. Sediments also influence slab dip, but variations in geometry depend multiple factors. Here we use 2D thermomechanical models explore how can dynamics geometry. We find that thick lead slower due an increase megathrust shear stress as accretionary wedge gets wider, a decrease pull buoyant...

10.1029/2021gl096266 article EN Geophysical Research Letters 2021-10-15

Abstract. To a large extent, the thermal structure of subduction zone determines where seismicity occurs through controls on transition from brittle to ductile deformation and depth dehydration reactions. Thermal models zones can help understand distribution by accurately modelling zone. Here, we assess common simplification in zones, i.e. constant values for parameters. We use temperature-dependent parameterisations, constrained lab data, conductivity, heat capacity, density systematically...

10.5194/se-14-683-2023 article EN cc-by Solid Earth 2023-07-11
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