Late Cretaceous to Early Paleocene Climate and Sea-Level £Uctuations: the Tunisian Record

Late Cretaceous to Early Paleocene Climate and Sea-Level £Uctuations: the Tunisian Record

Published in Palaeogeography, Palaeoclimatology, Palaeoecology 2754 : 1-32, 2002, 1 which should be used for any reference to this work Late Cretaceous to early Paleocene climate and sea-level £uctuations: the Tunisian record Thierry Adatte a;*, Gerta Keller b, Wolfgang Stinnesbeck c a Institut de Ge¨ologie, 11 Rue Emile Argand, 2007 Neuchatel, Switzerland b Department of Geosciences, Princeton University, Princeton, NJ 08544, USA c Geologisches Institut, Universitat Karlsruhe, 76128 Karlsruhe, Germany Abstract Climate and sea-level fluctuations across the Cretaceous^Tertiary (K^T) transition in Tunisia were examined based on bulk rock and clay mineralogies, biostratigraphy and lithology in five sections (El Melah, El Kef, Elles, Ain Settara and Seldja) spanning from open marine to shallow inner neritic environments. Late Campanian to early Danian trends examined at El Kef and Elles indicate an increasingly more humid climate associated with sea-level fluctuations and increased detrital influx that culminates at the K^T transition. This long-term trend in increasing humidity and runoff in the Tethys region is associated with middle and high latitude cooling. Results of short-term changes across the K^T transition indicate a sea-level lowstand in the latest Maastrichtian about 25^100 ka below the K^T boundary with the regression marked by increased detrital influx at El Kef and Elles and a short hiatus at Ain Settara. A rising sea-level at the end of the Maastrichtian is expressed at Elles and El Kef by deposition of a foraminiferal packstone. A flooding surface and condensed sedimentation mark the K^T boundary clay which is rich in terrestrial organic matter. The P0^ P1a transition is marked by a sea-level lowstand corresponding to a short hiatus at Ain Settara where most of P0 is missing and a period of non-deposition and erosion in the lower part of P1a (64.95 Ma). At Seldja, P0 and possibly the topmost part of CF1 are missing. These sea-level fluctuations are associated with maximum humidity. These data suggest that in Tunisia, long-term environmental stresses during the last 500 ka before the K^T boundary and continuing into the early Danian are primarily related to climate and sea-level fluctuations. Within this long-term climatic trend the pronounced warm and humid event within the latest Maastrichtian Zone CF1 may be linked to greenhouse conditions induced by Deccan volcanism. The absence of any significant clay mineral variations at or near the K^T boundary and Ir anomaly suggests that the bolide impact had a relatively incidental short-term effect on climate in the Tethys region. Keywords: sea-level; climate £uctuations; K^T boundary; Upper Campanian; Maastrichtian; Tunisia; bulk; clay minerals; organic matter; geochemistry 1. Introduction There are relatively few studies that detail long- * Corresponding author. Tel.: +41-32-718-26-18; Fax: +41- 32-718-26-01. term climate and sea-level changes during the late E-mail address: [email protected] (T. Adatte). Cretaceous which was generally assumed to have 2 been equally warm. Recent stable isotope studies, addition, climatic changes inferred from clay min- however, have revealed that the Maastrichtian eral contents correlate with sea-level changes. global climate was signi¢cantly cooler than during Warm or humid climates accompany high sea-lev- the earlier Cretaceous. Strong climate and temper- els and cooler or arid climates generally accom- ature £uctuations mark the late Campanian and pany low sea-level (Li et al., 2000). Maastrichtian, as indicated from stable isotope The global sea-level £uctuations are linked to records from the equatorial Paci¢c (Site 463, Kel- climatic changes (Li et al., 1999) and inversely ler and Li, in press) and middle and high latitude correlate with species diversity in planktic fora- South Atlantic (Sites 525, 689 and 690, Barrera minifera (e.g. diversity maximum follows maxi- and Huber, 1990; Barrera, 1994; Barrera et al., mum cooling at 70.7^70.3 Ma; diversity decline 1997; Li and Keller, 1998a,b). The ¢rst major follows warming at 65.4^65.2 Ma, Li and Keller, global cooling occurred between 71 and 73 Ma 1998a,c). But precisely how climate changed and decreased intermediate water temperatures across the K^T boundary mass extinction and by 5^6³C and surface temperatures by 4^5³C in during the subsequent evolution of early Tertiary middle and high latitudes. Between 68.5 and 70 faunas is still an enigma largely because diagenetic Ma, intermediate waters warmed by 2³C. Global alteration of carbonates obscures the oxygen iso- cooling resumed between 68.5 and 65.5 Ma when tope records (see Stueben et al., this volume). intermediate water temperatures decreased by 3^ A number of studies have attempted to recon- 4³C and sea surface temperatures decreased by struct the sea-level history across the K^T transi- 5³C in middle latitudes. About 450^200 ka before tion in Tunisia based on benthic and planktic for- the Cretaceous^Tertiary (K^T) boundary rapid aminifera, dino£agellates or palyno£oras (e.g. global warming increased intermediate and sea Brinkhuis and Zachariasse, 1988; Keller, 1988b, surface temperatures by 3^4³C, though sea sur- 1992; MacLeod and Keller, 199la,b; Schmitz et face temperatures changed little in low latitudes al., 1992; Speijer, 1994; Keller and Stinnesbeck, (Li and Keller, 1998b). Beginning about 200 ka 1996; Brinkhuis and Visscher, 1994; Brinkhuis et before the end of the Maastrichtian, climate al., 1998; Galeotti and Coccioni, 2002). The over- cooled rapidly by 2^3³C in both surface and in- all sea-level trends in these studies are in general termediate waters and warmed again during the agreement, though may vary in the details and the last 50^100 ka of the Maastrichtian (Li and Kel- timing of sea-level lowstands. A major problem ler, 1998b; Stueben et al., this volume). has been the absence of oxygen isotope-inferred These global climatic changes were associated climate data to support sea-level £uctuations in- with major sea-level £uctuations as expressed in ferred from faunal and £oral proxies. Oxygen iso- a variety of sea-level proxies, including bulk rock tope data are frequently not reliable temperature and clay mineral compositions, stable isotopes, indicators across the K^T transition because of total organic carbon (TOC), Sr/Ca ratios and diagenetic alteration of carbonate and recrystalli- macro- and microfaunal associations. Based on zation of foraminiferal tests (Oberhaensli et al., these sea-level and climate proxies, Li et al. 1998; Stueben et al., this volume). Alternate tem- (1999, 2000) have identi¢ed seven major sea-level perature proxies based on the coiling direction of regressions during the last 10 myr of the Creta- the benthic foraminifera Cibicidoides pseudoacutus ceous at El Kef and Elles (Tunisia): late Campa- (Galeotti and Coccioni, 2002) and the ratio of nian (V74.2 Ma, 73.4^72.5 Ma and 72.2^71.7 warm/cool dinocysts (Brinkhuis et al., 1998) Ma), early Maastrichtian (70.7^70.3 Ma, 69.6^ have been proposed, but these have yet to be in- 69.3 Ma and 68.9^68.3 Ma), and late Maastrich- dependently con¢rmed. tian (65.45^65.50 Ma). Low sea-levels are gener- This study evaluates climate and sea-level ally associated with increased terrigenous in£ux, changes across the K^T transition based on litho- low kaolinite/chlorite+illite ratios, high TOC and logical characteristics, bulk rock and clay mineral high Sr/Ca ratios, whereas high sea-levels are gen- data from several Tunisian sections that span erally associated with the reverse conditions. In from upper slope (El Melah) to outer neritic (El 3 Fig. 1. Paleoenvironmental settings of ¢ve Tunisian K^T sections spanning from the restricted shallow Gafsa Basin (Seldja sec- tion) at the edge of the Sahara to the middle and outer shelf depths of the El Kef, Elles and Ain Settara sections to the north of the Kasserine Island, and to the upper bathyal El Melah section to the north (modi¢ed after Burollet, 1956; Burollet and Oudin, 1980). Isopach lines are given in meter for the Maastrichtian interval. Kef, Elles), middle neritic (Ain Settara) and inner trichtian of Elles and El Kef sections. Biostrati- neritic (Seldja) environments (Fig. 1). The time graphic data for each section are based on pub- interval analyzed spans from the uppermost lished studies: Elles I and El Melah from Karoui- Maastrichtian Zone CF1 to the early Danian Yakoub et al. (2002), Elles II K^T transition from Zone Plb or Plc. In addition, we examine long- Keller et al. (2002) and upper Maastrichtian from term trends based on bulk rock and clay mineral Abramovich and Keller (2002), Ain Settara from data from the late Campanian through Maas- Luciana (2002) and Seldja from Keller et al. trichtian of the Elles and El Kef sections. (1998). Sediment accumulation rates were calcu- lated based on the time scale of Cande and Kent (1995). 2. Methods Whole rock and clay mineral analyses were conducted at the Geological Institute of the Uni- In the ¢eld, sections were cleaned from surface versity of Neuchatel, Switzerland, based on XRD contamination by digging a trench to fresh bed- analyses (SCINTAG XRD 2000 Di¡ractometer). rock. Samples were then collected at 5^10 cm in- Sample processing followed the procedure out- tervals and at closer 1^2 cm intervals across the lined by Ku«bler (1987) and Adatte et al. (1996). K^T boundary clay layer. For each section, the XRD analyses of the whole rock were carried out same sample set was used for faunal, geochemical for all the samples at the Geological Institute of and mineralogical studies to insure direct compar- the University of Neuchatel.

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