Imperial College London

Dr Gareth Collins

Faculty of EngineeringDepartment of Earth Science & Engineering

Reader in Planetary Science



+44 (0)20 7594 1518g.collins Website




4.83Royal School of MinesSouth Kensington Campus





My research explores the many consequences of impacts in the solar system through the development and application of numerical impact models.


Impacts and Astromaterials Research Centre 

Environmental consequences of impacts on Earth

iSALE: A shock physics code for simulating impact phenomena

The major themes of my research are described below.

Chicxulub impact

Chicxulub impact

The 65.5 Ma, K-Pg mass extinction event was triggered by a large impact that formed the Chicxulub crater, Mexico. My numerical simulations have aided geophysical interpretation of the Chicxulub crater [1,2,3,4], Mexico, and constrained the impact energy of this major event in Earth history, which wiped out more than 70% of species [5].

Cratering on the Moon

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I am interested in how large asteroid impacts shaped the Moon’s crust during its early evolution. My recent work [6,7,8,9,10] has provided new insight into the relationship between observed crater diameter and asteroid size, and helped to constrain the mass flux of asteroids in the inner solar system, which has implications for accurate dating of planetary surfaces, delivery of volatiles to the Earth-Moon system since its formation, and the severity of early bombardment in the inner solar system.

Impacts in the Early Solar System


My research aims to quantify the thermal consequences of impacts on asteroids, the parent bodies of most meteorites. Meteorites are a window into the early solar system as they contain a physical record of the processes that occurred during its inception. In the past, impacts were not regarded as important in the thermal evolution of asteroids. My recent research has shown that, on the contrary, impacts on porous asteroids cause more localised heating than previously thought [11] and that this localised heat is retained for tens of thousands of years, consistent with heating and cooling rates inferred from meteoritic evidence [12]. This has prompted a re-evaluation of the importance of collisions in the thermal evolution of the early solar system [13].

Oblique impact

Oblique impactNumerical investigations of impact crater formation have traditionally been limited to 2D vertical impacts, which are rare in nature, because of the computational expense of more realistic oblique impacts. I have co-developed a new, efficient 3D numerical impact simulator, and used it to quantify the effect of impact angle on crater size and shape [14,15,16]. The results have been used to derive the first estimates of the size-frequency distribution of elliptical craters on the terrestrial planets [17].

Cratering in complex targets

A focus of my research is to understand the role target heterogeneity plays in the formation of the multiple concentric-rings that characterize large terrestrial impact craters. Without a quantitative model of how these rings form it is impossible to associate a ring feature with the energy of the impact, and hence identify its true “scale.” Quantifying the relationship between impactor properties and final crater shape is critical for understanding the immediate environmental consequences of an impact, and for accurately assessing the hazard posed by impacts. My numerical modelling work suggests that strength variations in layered targets can change substantially the size and shape of the crater formed during an impact, and lead to multiple-ringed impact structures. This is exemplified by my research on the Chesapeake Bay crater, the largest impact structure in the USA, which showed that during the formation of the crater the upper target layers behaved in a fluid-like manner, leading to a broad outer crater in the sediments and a smaller inner crater in the basement rocks. This work overturned the previous interpretation of the crater as a typical extra-terrestrial peak-ring crater, and revised the impact energy down from much larger prior estimates. The work helped select the location of a recent successful USGS drill hole into the crater.

Material models for impact simulations

iSALEIn my research I develop, manage and employ numerical models for the simulation of impact events and other violent, dynamic geologic processes. The impact software I develop, iSALE, is used by >50 scientists world-wide at >12 institutions. iSALE includes advanced physics-based material strength and porosity compaction models specifically designed for impact simulations.

Environmental consequences of impacts

I have developed a simple-to-use interactive web program to estimate the consequences of asteroid and comet impacts on Earth.

The site allows users to calculate consequences ranging from the size of the crater and the probability of such an event occurring, to the speed of the winds from the blast wave and Chicxulub ejectathermal radiation from the hot vapour plume. Results from the calculator have also been used for scientific research: the science behind the calculator was published as a journal article, and resulted in a new discovery about Barringer crater, Arizona.

Extreme geologic processes

Tephra settling

3D multiphase Fluidity simulation of particle settling in water

I also investigate the hazard of other important, closely related, large, energetic surface processes, such as long-runout rock avalanches and large tsunamis generated by earthquakes and landslides.


Dr Joanna Morgan, Earth Science and Engineering, Impact cratering

Dr M.D. Piggott, Earth Science and Engineering, Computational Physics, 2004

Research Staff



Research Student Supervision

Smith,RC, Submarine Landslide Tsunami Hazard to the UK

Jacobs,CT, Modelling of Multiphase Flows on Adaptive Unstructured Meshes with Applications to the Dynamics of Volcanic Ash Plumes

Potter,RWK, Numerical Modelling of Basin-Scale Impact Crater Formation

Davison,T, Numerical Modelling of Heat Generation in Porous Planetesimal Collisions

Wilson,C, Modelling of multiple-material flows on adaptive unstructured meshes

Bray,V, Impact Crater Formation on the Icy Galilean Satellites