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 …
InSight constraints on the global character of the Martian crust
Analyses of seismic data from the InSight mission have provided the first in situ constraints
on the thickness of the crust of Mars. These crustal thickness constraints are currently limited …
on the thickness of the crust of Mars. These crustal thickness constraints are currently limited …
Probing the hydrothermal system of the Chicxulub impact crater
The~ 180-km-diameter Chicxulub peak-ring crater and~ 240-km multiring basin, produced
by the impact that terminated the Cretaceous, is the largest remaining intact impact basin on …
by the impact that terminated the Cretaceous, is the largest remaining intact impact basin on …
Bombardment history of the Moon constrained by crustal porosity
The formation and evolution of the terrestrial planets were shaped by a bombardment of
large impactors in a cluttered early Solar System. However, various surface processes …
large impactors in a cluttered early Solar System. However, various surface processes …
End of the Cretaceous
SPS Gulick - Geological Society, London, Special Publications, 2025 - lyellcollection.org
The Cretaceous ended when the Chicxulub asteroid struck the Yucatán platform, and all
deposits and landforms generated are earliest Paleocene in age. Drill core from the …
deposits and landforms generated are earliest Paleocene in age. Drill core from the …
Experimental evidence for shear‐induced melting and generation of stishovite in granite at low (< 18 GPa) shock pressure
Abstract Knowledge of the shock behavior of planetary materials is essential to interpret
shock metamorphism documented in rocks at hypervelocity impact structures on Earth, in …
shock metamorphism documented in rocks at hypervelocity impact structures on Earth, in …
Crustal structure constraints from the detection of the SsPp phase on Mars
The shallowest intracrustal layer (extending to 8±2 km depth) beneath the Mars InSight
Lander site exhibits low seismic wave velocity, which is likely related to a combination of …
Lander site exhibits low seismic wave velocity, which is likely related to a combination of …
A Late Paleocene age for Greenland's Hiawatha impact structure
The~ 31-km-wide Hiawatha structure, located beneath Hiawatha Glacier in northwestern
Greenland, has been proposed as an impact structure that may have formed after the …
Greenland, has been proposed as an impact structure that may have formed after the …
New insights into the formation and emplacement of impact melt rocks within the Chicxulub impact structure, following the 2016 IODP-ICDP Expedition 364
This study presents petrographic and geochemical characterization of 46 pre-impact rocks
and 32 impactites containing and/or representing impact melt rock from the peak ring of the …
and 32 impactites containing and/or representing impact melt rock from the peak ring of the …
Geochemical and mineralogical classification of four new shergottites: NWA 10441, NWA 10818, NWA 11043, and NWA 12335
Martian meteorites are rare; therefore, the discovery of new meteorites has the potential to
significantly expand our current understanding of Mars. In this study, we describe four new …
significantly expand our current understanding of Mars. In this study, we describe four new …