2010
DOI: 10.1016/j.epsl.2009.12.021
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Orbital chronology of Early Eocene hyperthermals from the Contessa Road section, central Italy

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Cited by 123 publications
(125 citation statements)
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“…During the PETM global temper-V. Lauretano et al: Frequency, magnitude and character of hyperthermal events ature rose by 5-8 • C, and massive amounts of carbon were released as evidenced by a significant negative carbon isotope excursion (CIE) of > 3 ‰ in the ocean/atmosphere carbon pools, and widespread dissolution of seafloor carbonate (Kennett and Stott, 1991;Dickens et al, 1995;Thomas and Shackleton, 1996;Zachos et al, 2005Zachos et al, , 2008Sluijs et al, 2007;McInerney and Wing, 2011). A series of similar events are recorded in carbonate records from marine and continental deposits from the early Paleogene, as expressed by negative excursions in δ 13 C and δ 18 O often accompanied by dissolution horizons (e.g., Cramer et al, 2003;Lourens et al, 2005;Agnini et al, 2009;Galeotti et al, 2010;Stap et al, 2010;Zachos et al, 2010;Abels et al, 2012Abels et al, , 2015Slotnick et al, 2012;Kirtland Turner et al, 2014;Littler et al, 2014). Orbitally tuned records for this geological interval provide evidence that the early Eocene hyperthermal events were paced by variations in the Earth's orbit, specifically in the long-and short-eccentricity cycles.…”
Section: Introductionmentioning
confidence: 80%
“…During the PETM global temper-V. Lauretano et al: Frequency, magnitude and character of hyperthermal events ature rose by 5-8 • C, and massive amounts of carbon were released as evidenced by a significant negative carbon isotope excursion (CIE) of > 3 ‰ in the ocean/atmosphere carbon pools, and widespread dissolution of seafloor carbonate (Kennett and Stott, 1991;Dickens et al, 1995;Thomas and Shackleton, 1996;Zachos et al, 2005Zachos et al, , 2008Sluijs et al, 2007;McInerney and Wing, 2011). A series of similar events are recorded in carbonate records from marine and continental deposits from the early Paleogene, as expressed by negative excursions in δ 13 C and δ 18 O often accompanied by dissolution horizons (e.g., Cramer et al, 2003;Lourens et al, 2005;Agnini et al, 2009;Galeotti et al, 2010;Stap et al, 2010;Zachos et al, 2010;Abels et al, 2012Abels et al, , 2015Slotnick et al, 2012;Kirtland Turner et al, 2014;Littler et al, 2014). Orbitally tuned records for this geological interval provide evidence that the early Eocene hyperthermal events were paced by variations in the Earth's orbit, specifically in the long-and short-eccentricity cycles.…”
Section: Introductionmentioning
confidence: 80%
“…This highest occurrence close to the CIE was also encountered in other Egyptian sections such as Gebel Aweina, Gebel Duwi, and Gebel Abu Had (Aubry, 1998; von Salis et al, 1998), in the Contessa section in Italy (Galeotti et al, 2010), and in the Zumaya and Alamedilla sections in Spain (Monechi et al, 2000a(Monechi et al, , 2000b. The HO of Fasciculithus alanii coincides with the NP9a/NP9b subzonal boundary in the Gebel Matulla section.…”
Section: Gebel Matulla Section (mentioning
confidence: 85%
“…This carbon isotope excursion of >1.0 ‰ is confirmed by measurements on C. decoratus, A. acutus and A. zitteli. It is most likely related to one of the early Eocene Carbon Isotope Excursions (CIEs) (Cramer et al, 2003;Galeotti et al, 2010) and its association with a negative oxygen isotope excursion suggests that it may involve a hyperthermal event. Considering the magnitude of the CIE (1-1.5 ‰) and its position close to the basis of NP11, ETM2 (Lourens et al, 2005) is a likely candidate for this potential hyperthermal.…”
Section: Isotope Stratigraphymentioning
confidence: 99%