Development of a combined capacity of numerical and experimental simulation of cosmic impacts with special focus on effects of marine targets
Cosmic impact craters marine targets
Share on facebook
Share on twitter
Share on linkedin

Spanish Research Council (CSIC) support for international cooperation: I-LINK project LINKA20203.

Total funding: 23.001,24 Eur

Período: 01/01/2020 until 31/12/2021

Investigador principal (CSIC): Dr. Jens Ormö

Otros investigadores: Dr. M. Isabel Herreros

Investigadores principales extranjeros: Dr. Vinamra Agrawal (Auburn University, USA) y Dr. Erik Sturkell (Gothenburg University, Sweden)

We aim to establish a stable and long-lasting collaboration between the Centro de Astrobiología (CAB INTA-CSIC) team and the international teams at Auburn University (AU) and University of Gothenburg (GU), being both of them of highest relevance to the subject of the project. Cosmic impact craters are useful tools to assess target properties, paleo-environments and related hazards to humanity. The laboratory for experimental impact cratering at the CAB INTA-CSIC is unique in its design for the analysis of marine impacts. Likewise, the three teams from CAB INTA-CSIC, AU, and GU hold extensive knowledge on the geology of such craters. When linked with the new capacity of advanced numerical simulation of impact processes at AU and CAB INTA-CSIC, the team will have the the capacity for combined experimental and numerical analysis of the cratering process, especially for marine targets. Such targets represent >70% of Earth’s surface as well as having mechanical properties of great importance in the development of numerical codes. Likewise, the special features of the resulting marine-target crater provide further information on the target (paleo)environment (e.g. volatile content), which can guide future Mars missions to sites where water in combination with fracturing and long-lived impact-induced heat may have generated life habitats. On the other hand, it is well known that marine impacts may generate hazardous tsunamis, and such have recently been suggested to be the cause of certain landforms even on Mars. Knowledge of the effects of target properties (e.g. layering) is also of great importance for the mitigation of Earth-threatening asteroids by means of projectile impacts. The CSIC-led team’s combination of observational data and simulation capacity is exceptional in the world in analyzing these effects from marine (i.e. layered target) impacts.

Cosmic impact craters marine targets
The EPIC target tank in preparation for aquatic quarter-space experiments (i.e., shots along the glass window of the “camera tank”). The large diameter of the funnel-shaped target tank is to reduce the effect of reflected waves on the crater modification processes (e.g. water resurge). The “wings” of the camera tank are to minimize disturbances of the tsunami wave propagation.
Cosmic impact craters marine targets
The EPIC projectile launcher. It shoots projectiles of any material and up to 20mm in diameter at angles between 20 and 90 degrees over the horizontal.

Abstracts presented at the EPSC 2020:

– King Jr., D. T., Ormo, J., Petruny, L. W., De Marchi, L., and Agrawal, V.: Crater-filling materials, Wetumpka impact structure, Alabama.

– De Marchi, L., King, D., Ormö, J., and Agrawal, V.: Numerical and experimental analysis of the Wetumpka (Alabama USA) impact crater.

– Sturkell, E. and Ormö, J.: The Lockne – Målingen doublet: effects of a rubble-pile impact in a marine environment (layered target).

– Ormö, J., Gulick, S. S. P., Whalen, M. T., King Jr., D. T., Sturkell, E., and Morgan, J.: A method to assess event magnitude and target water depth for marine-target impacts. Part 1: Granulometry of resurge deposits.

– Herreros, I. and Ormö, J.: A method to assess event magnitude and target water depth for marine-target impacts. Part 2: The physics behind the observations.

– Ormö, J., Raducan, S. D., Luther, R., Herreros, M. I., Collins, G. S., Losiak, A., and Wünnemann, K.: Effects of target heterogeneity on impact cratering processes in the light of the Hera mission: combined experimental and numerical approach.

– De Marchi, L., King, D., Ormö, J., Sturkell, E., and Agrawal, V.: Numerical simulations of Lockne impact crater formation using iSALE-2D.

Submitted manuscripts for research articles:

– Ormö et al. “Assessing event magnitude and target water depth for marine-target impacts: Ocean resurge deposits in the Chicxulub M0077A drill core compared”. Submitted to Earth and Planetary Science Letters.

– De Marchi et al. “Numerical simulation of the formation of the critical, ocean-facing, southern sector of the Wetumpka impact structure constrained by field and drill-core data”. Submitted to Meteoritics and Planetary Science.

Noticias relacionadas

Publicaciones relacionadas

Rigid body motion in viscous flows using the finite element method


Departamento de Planetología y Habitabilidad
Teléfono: + 34 9152 01226
Departamento de Planetología y Habitabilidad
Teléfono: +34 91 5201662

This website uses cookies to ensure you get the best experience on our website.