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Early to Late Maastrichtian environmental changes in the Indian Ocean compared with Tethys and South Atlantic

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dc.contributor.author Mateo, Paula en_US
dc.contributor.author Keller, Gerta en_US
dc.contributor.author PUNEKAR, JAHNAVI en_US
dc.contributor.author Spangenberg, Jorge E. en_US
dc.date.accessioned 2019-07-01T05:37:14Z
dc.date.available 2019-07-01T05:37:14Z
dc.date.issued 2017-07 en_US
dc.identifier.citation Palaeogeography, Palaeoclimatology, Palaeoecology, 478, 121-138. en_US
dc.identifier.issn 0031-0182 en_US
dc.identifier.uri http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/3330
dc.identifier.uri https://doi.org/10.1016/j.palaeo.2017.01.027 en_US
dc.description.abstract Planktic foraminiferal analysis, including species populations, diversity trends, high-stress indices and stable isotopes of the latest Campanian through Maastrichtian in the South Atlantic, Tethys and Indian oceans reveal four major climate and faunal events that ended with the Cretaceous-Paleogene (K/Pg), formerly Cretaceous-Tertiary (K/T), mass extinction. The prelude to these events is the late Campanian cooling that reached minimum temperatures in the earliest Maastrichtian (base C31r) correlative with low primary productivity and species diversity. Event-1 begins during the persistent cool climate of the early Maastrichtian (lower C31r) when primary productivity rapidly increased accompanied by rapid species originations, attributed to increased nutrient influx from increased upwelling, erosion during the sea-level fall ~ 70.6 Ma, and Ninety East Ridge volcanism. During Event-2 (upper C31r to lower C30n), climate rapidly warmed by 2–3 °C in deep waters and peaked at 22 °C on land, primary productivity remained high and diversification reached maximum for the entire Cretaceous. We attribute this climate warming to intense Ninety East Ridge volcanic activity beginning ~ 69.5 Ma, accompanied by rapid reorganization of intermediate oceanic circulation. Enhanced greenhouse conditions due to the eruption of Deccan Phase-1 in India resulted in detrimental conditions for planktic foraminifera marking the end of diversification. Global cooling resumed in Event-3 (C30n), species diversity declined gradually accompanied by dwarfing, decreased large specialized species, increased small ecologically tolerant taxa, and ocean acidification. Event-3 is mainly the result of enhanced weathering and volcanogenic CO2 adsorption by the oceans during the preceding warm Event-2 that led to cooling and lower pH in the surface ocean. Event-4 marks the last 250 kyr of the Maastrichtian (C29r), which began with the largest Deccan eruptions (Phase-2) that caused rapid climate warming of 4 °C in deep waters and 8 °C on land, acid rain and ocean acidification leading to a major carbonate crisis preceding the K/T mass extinction. en_US
dc.language.iso en en_US
dc.publisher Elsevier B.V. en_US
dc.subject Late Maastrichtian en_US
dc.subject Indian Ocean compared en_US
dc.subject Tethys and South Atlantic en_US
dc.subject Ninety East en_US
dc.subject Ridge Volcanism en_US
dc.subject Deccan volcanism en_US
dc.subject |Mid-Maastrichtian event en_US
dc.subject TurnoversClimate change en_US
dc.subject 2017 en_US
dc.title Early to Late Maastrichtian environmental changes in the Indian Ocean compared with Tethys and South Atlantic en_US
dc.type Article en_US
dc.contributor.department Dept. of Earth and Climate Science en_US
dc.identifier.sourcetitle Palaeogeography en_US
dc.publication.originofpublisher Foreign en_US


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