2012
DOI: 10.1016/j.epsl.2012.09.054
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Cyclostratigraphy and astronomical tuning of the Late Maastrichtian at Zumaia (Basque country, Northern Spain)

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Cited by 80 publications
(95 citation statements)
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References 60 publications
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“…In Zumaya, using the cyclostratigraphic studies of Batenburg et al (2012) and Dinarès-Turell et al (2013), our targeted interval (last 0.5 myr of the Maastrichtian) appears to correspond to the top few meters of Member IV and the entire Member V of Ward and Kennedy (1993). This is a conservative estimate as due to small differences in measured thicknesses between Ward and Kennedy (1993), Dinarès-Turell et al (2013), and Batenburg et al (2012), the exact position of the base of our 0.5 myr interval cannot be situated more precisely than 1 m. The base of Member V is approximately 15 m below the K/Pg boundary in Ward and Kennedy (1993), 12 m below the K/ Pg boundary in Batenburg et al (2012), and 10.2 m below the K/Pg boundary in Dinarès-Turell et al (2013). The base of our 0.5 myr interval thus equates to approximately 20 and 18 m below the K/Pg boundary on the Batenburg et al (2012) and the Dinarès-Turell et al (2013) logs, respectively.…”
Section: Bay Of Biscaymentioning
confidence: 99%
“…In Zumaya, using the cyclostratigraphic studies of Batenburg et al (2012) and Dinarès-Turell et al (2013), our targeted interval (last 0.5 myr of the Maastrichtian) appears to correspond to the top few meters of Member IV and the entire Member V of Ward and Kennedy (1993). This is a conservative estimate as due to small differences in measured thicknesses between Ward and Kennedy (1993), Dinarès-Turell et al (2013), and Batenburg et al (2012), the exact position of the base of our 0.5 myr interval cannot be situated more precisely than 1 m. The base of Member V is approximately 15 m below the K/Pg boundary in Ward and Kennedy (1993), 12 m below the K/ Pg boundary in Batenburg et al (2012), and 10.2 m below the K/Pg boundary in Dinarès-Turell et al (2013). The base of our 0.5 myr interval thus equates to approximately 20 and 18 m below the K/Pg boundary on the Batenburg et al (2012) and the Dinarès-Turell et al (2013) logs, respectively.…”
Section: Bay Of Biscaymentioning
confidence: 99%
“…The first proposal provides a K-Pg boundary age of 65.59 ± 0.07 Ma and the second an age of 66.00 ± 0.07 Ma. BATENBURG et al (2012) studied the upper Maastrichtian of the Zumaia section in the Basque country (northern Spain) that contains a cyclic alternation of limestones and marls deposited in a hemipelagic setting. In this section, the stacking pattern of the lithologies shows a hierarchy that reflects the combined influence of the orbital parameters of precession and eccentricity.…”
Section: ) Herbert and Collaborators Study In South Atlanticmentioning
confidence: 99%
“…Following their figure, if we fix the K-Pg boundary at an arbitrary time of 0 kyr and the duration of the cycle at 405 kyr, then the last Cretaceous minima is situated at -338 kyr and the first Paleogene minima is situated at +67 kyr. BATENBURG et al (2012) studied the upper Maastrichtian of the Zumaia section. In this work, the expression of the 405-kyr eccentricity cycle present in the section served as a primary signal for astronomical tuning, i.e., use of a constant duration of 405 kyr between eccentricity minima and linear interpolation between these points.…”
Section: ) Westerhold and Collaborators Study In South Atlantic And mentioning
confidence: 99%
“…Recently, the Maastrichtian part of the Zumaia section has been investigated in detail, using an integrated stratigraphic approach (Batenburg et al 2012;Dinarès-Turell et al 2013). The study was directed at establishing a carbon isotope stratigraphy and an astronomically tuned age model based on the 405 kyr cycle (this cycle is stable in the astronomical solution beyond 50 Ma) (see Laskar et al 2011a;Westerhold et al 2012).…”
Section: Mesozoicmentioning
confidence: 99%
“…The study was directed at establishing a carbon isotope stratigraphy and an astronomically tuned age model based on the 405 kyr cycle (this cycle is stable in the astronomical solution beyond 50 Ma) (see Laskar et al 2011a;Westerhold et al 2012). Combined with the nearby Sopelana section, the record covers almost the entire Maastrichtian in an essentially continuous succession (Batenburg et al 2012(Batenburg et al , 2013. The continuity is confirmed by the excellent agreement with the tuned age model developed independently for the Maastrichtian in Deap Sea Drilling Project (DSDP)/ODP cores (DSDP Sites 525A and 762C, and ODP Site 1267B: Husson et al 2011;Thibault et al 2012;see Figs 7 & 8 in Batenburg et al 2012).…”
Section: Mesozoicmentioning
confidence: 99%