GSA Connects 2023 Meeting in Pittsburgh, Pennsylvania

Paper No. 112-22
Presentation Time: 8:00 AM-5:30 PM

THE RAIN OF FIRE THAT ENDED THE MESOZOIC: MOLTEN ROCK DROPLETS DURING THE DINOSAUR APOCALYPSE


BERMUDEZ, Hermann1, BOLIVAR, Liliana2, GLASS, Billy P.3, MORGAN, Joanna V.4, GILABERT, Vicente5, ARZ, José Antonio5, ARENILLAS, Ignacio5, PHILLIPS, George E.6, BERMUDEZ, Daniela7, GOMEZ, Clemencia8, DE PALMA, Maurizia9 and CUI, Ying10, (1)Department of Earth and Environmental Studies, Montclair State University, 1 Normal Ave, Montclair, NJ 07043; Grupo de Investigacion Paleoexplorer, 400 Lincoln st, Dupont, PA 18641; Departamento de Geociencias, Universidad Nacional de Colombia, Bogota, D.C. 11001, Colombia, (2)Grupo de Investigacion Paleoexplorer, 400 Lincoln st, Dupont, PA 18641, (3)Geological Sciences, University of Delaware, 255 Academy St, Newark, DE 19716, (4)Department of Earth Science and Engineering, Imperial College London, Prince Consort Road, South Kensington, London, SW7 2BP, United Kingdom, (5)Departamento de Ciencias de la Tierra, Instituto Universitario de Investigación en Ciencias Ambientales de Aragón, University of Zaragoza, C/Pedro Cerbuna, 12, Zaragoza, 50009, Spain, (6)Paleontology, Mississippi Museum of Natural Science, 2148 Riverside Drive, Jackson, MS 39202-1353, (7)Pittston Area High School, Yatesville, PA 18640, (8)Departamento de Geociencias, Universidad Nacional de Colombia, Bogota, D.C. 11001, Colombia, (9)Department of Earth and Environmental Studies, Montclair State University, 1 Normal Ave, Montclair, NJ 07043, (10)Department of Earth and Environmental Studies, Montclair State University, 1 Normal Avenue, Montclair, NJ 07043

The Chicxulub asteroid impact (~66 Ma) coincided with the Cretaceous-Paleogene (K-Pg) boundary and was the probable trigger for the last mass extinction in Earth's history. The events unleashed by the collision led to the demise of three-quarters of the species, including the iconic non-avian dinosaurs. During the crater formation, millions of tons of molten and vaporized rock, dust, and gases were expelled into the atmosphere. These materials spread across the globe and fell as a scorching rain that lasted for hours. The soot resulting from the global fires, the dust, and the settling of the finer fraction persisted for weeks or months after impact. Tiny glass droplets (impact spherules) represent a significant volume of the ejecta. Our hypothesis suggests that the morphology, size, and distribution of the impact spherules within the K-Pg bed are related to their origin and transport mechanisms. To test this, thousands of spherules from Wahalak Creek (Mississippi), Gorgonilla Island (Colombia), and Zumaia (Spain) were described, analyzed, and illustrated. Our observations suggest that three fractions within the K-Pg bed are related to three different transport mechanisms: 1) the coarser fraction (lower layer when it has not been reworked) records the accumulation of rotational molten rock droplets, which arrived early at very temperature to locations close to the impact site following ballistic trajectories. 2) the intermediate fraction (middle layer) represents tiny molten rock droplets transported by the rapid expansion of a high-temperature cloud. 3) the finer fraction (upper layer, commonly called the fireball layer) is globally distributed and represents the accumulation of tiny droplets condensed from a vapor cloud. Our results show that Chicxulub's ejecta were distributed through different processes, each leaving a distinctive signature. This information provides valuable insights into ejecta distribution during massive asteroid impacts and enhances our understanding of the Chicxulub event and its aftermath.