T15 Impact Cratering Across the Solar System

Sunday, 15 October 2023
8:00 AM - 12:00 PM
323

ANOTHER ONE BITES THE DUST: PHOTOSYNTHETIC COLLAPSE FOLLOWING CHICXULUB IMPACT TRIGGERED BY FINE SILICATE DUST

Paper number: T15-8
Program: Technical Sessions
Time: 9:35 AM – 9:50 AM

Authors

Abstract

Formation of the ± 200 km in size Chicxulub crater is considered the most probable cause of the Cretaceous-Paleogene (K-Pg) boundary mass extinction, 66 million years ago. However, the exact climatic outcome of the various debris injected into the atmosphere following the crater excavation, and consequently the killing mechanisms remain poorly constrained. Current paleoclimate scenarios confer a prominent role in sulfur components released by the vaporization of evaporite layers present in the upper part of the target rock. Sedimentological constraints obtained from an expanded terrestrial K-Pg boundary deposit in North Dakota and measured volumetric size distribution of silicate dust suggest the release into the atmosphere of fine silicate dust (~0.8-8 μm). The new general circulation model simulations of the injection of such a plume of micrometer-sized silicate dust (2x1018g) suggest a long atmospheric lifetime (±15 years) with a global-average surface temperature falling by as much as 25ºC. Simulated effects on the post-impact active solar radiation support a dust-induced photosynthetic shut-down for almost 2 years. In contrast to previous work, these new paleoclimate simulations, relying on robust sedimentological field data at the K-Pg boundary revealed that the impact-generated silicate dust plume plays a key role in driving the K-Pg climate and biotic crisis. The new scenarios show that the global darkness and prolonged loss in the planet's photosynthetic activity occur only in the silicate dust scenario, up to nearly 1.7 years after impact; a sufficiently long timescale to pose severe challenges for terrestrial and marine habitats. Biotic groups not adapted to survive the dark, cold, and food-deprived conditions for almost two years, experienced massive extinctions. In addition, this emission scenario shows that the photosynthetic recovery to the pre-impact levels first occurred in the austral summer season, ~1.7 years after impact. This would imply a possible earlier recovery of the primary productivity in the Southern Hemisphere. These new results highlight that the photosynthetic shut-down induced by the large volume of silicate dust, together with additional effects of sulfur and soot likely led to the collapse of primary productivity in land and ocean realms, steering the global mass extinction at the K-Pg boundary.

Geological Society of America Abstracts with Programs. Vol. 55, No. 6

doi: 10.1130/abs/2023AM-392374

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