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The Chicxulub impact and its environmental consequences
The extinction of the dinosaurs and around three-quarters of all living species was almost
certainly caused by a large asteroid impact 66 million years ago. Seismic data acquired …
certainly caused by a large asteroid impact 66 million years ago. Seismic data acquired …
Geophysical characterization of the Chicxulub impact crater
Geophysical data indicate that the 65.5 million years ago Chicxulub impact structure is a
multi‐ring basin, with three sets of semicontinuous, arcuate ring faults and a topographic …
multi‐ring basin, with three sets of semicontinuous, arcuate ring faults and a topographic …
The formation of peak rings in large impact craters
Large impacts provide a mechanism for resurfacing planets through mixing near-surface
rocks with deeper material. Central peaks are formed from the dynamic uplift of rocks during …
rocks with deeper material. Central peaks are formed from the dynamic uplift of rocks during …
The first day of the Cenozoic
Highly expanded Cretaceous–Paleogene (K-Pg) boundary section from the Chicxulub peak
ring, recovered by International Ocean Discovery Program (IODP)–International Continental …
ring, recovered by International Ocean Discovery Program (IODP)–International Continental …
A steeply-inclined trajectory for the Chicxulub impact
The environmental severity of large impacts on Earth is influenced by their impact trajectory.
Impact direction and angle to the target plane affect the volume and depth of origin of …
Impact direction and angle to the target plane affect the volume and depth of origin of …
Scaling of oblique impacts in frictional targets: Implications for crater size and formation mechanisms
D Elbeshausen, K Wünnemann, GS Collins - Icarus, 2009 - Elsevier
Almost every meteorite impact occurs at an oblique angle of incidence, yet the effect of
impact angle on crater size or formation mechanism is only poorly understood. This is, in …
impact angle on crater size or formation mechanism is only poorly understood. This is, in …
Constraining the size of the South Pole-Aitken basin impact
The South Pole-Aitken (SPA) basin is the largest and oldest definitive impact structure on the
Moon. To understand how this immense basin formed, we conducted a suite of SPA-scale …
Moon. To understand how this immense basin formed, we conducted a suite of SPA-scale …
Numerical simulations of impact crater formation with dilatancy
GS Collins - Journal of Geophysical Research: Planets, 2014 - Wiley Online Library
Impact‐induced fracturing creates porosity that is responsible for many aspects of the
geophysical signature of an impact crater. This paper describes a simple model of dilatancy …
geophysical signature of an impact crater. This paper describes a simple model of dilatancy …
Asymmetric distribution of lunar impact basins caused by variations in target properties
Maps of crustal thickness derived from NASA's Gravity Recovery and Interior Laboratory
(GRAIL) mission revealed more large impact basins on the nearside hemisphere of the …
(GRAIL) mission revealed more large impact basins on the nearside hemisphere of the …
Rock fluidization during peak-ring formation of large impact structures
Large meteorite impact structures on the terrestrial bodies of the Solar System contain
pronounced topographic rings, which emerged from uplifted target (crustal) rocks within …
pronounced topographic rings, which emerged from uplifted target (crustal) rocks within …