2017
DOI: 10.1002/2017pa003197
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Reducing Disparity in Radio‐Isotopic and Astrochronology‐Based Time Scales of the Late Eocene and Oligocene

Abstract: A significant discrepancy of up to 0.6 Myr exists between radio‐isotopically calibrated and astronomically tuned time scales of the late Eocene‐Oligocene. We explore the possible causes of this discrepancy through the acquisition of “high‐precision” 206Pb/238U dating of zircons from 11 volcanic ash beds from the Umbria‐Marche sedimentary succession, which hosts the Global Stratotype Section and Point for the base of the Oligocene. Our results indicate that the four 40Ar/39Ar dates from the Umbria‐Marche succes… Show more

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Cited by 24 publications
(37 citation statements)
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References 96 publications
(291 reference statements)
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“…Although these data are not from the Karaburun section, instead coming from localities to the south and northwest, they provide further useful age constraints on the formation. Zircon U-Pb ages of 33.9 (±0.4) Ma (Kıyıköy locality; Okay et al, 2020), 32.5 Ma, 31.7 Ma, and 31.04 Ma (localities to the south of Karaburun; Okay et al, 2019) have been recorded, all of which are compatible with the age determination of the Karaburun section (age calibration model of Sahy et al, 2017).…”
Section: Integrated Conclusionsupporting
confidence: 71%
“…Although these data are not from the Karaburun section, instead coming from localities to the south and northwest, they provide further useful age constraints on the formation. Zircon U-Pb ages of 33.9 (±0.4) Ma (Kıyıköy locality; Okay et al, 2020), 32.5 Ma, 31.7 Ma, and 31.04 Ma (localities to the south of Karaburun; Okay et al, 2019) have been recorded, all of which are compatible with the age determination of the Karaburun section (age calibration model of Sahy et al, 2017).…”
Section: Integrated Conclusionsupporting
confidence: 71%
“…The Eocene-Oligocene boundary lies close to the Chadronian-Orellan boundary (Zanazzi et al, 2009). As such, both the Eocene-Oligocene boundary and Chadronian-Orellan Boundary were placed at 33.84 ±0.10 Ma (Ogg and Smith, 2004) but are now placed at 34.09 ± 0.08 Ma (Sahy et al, 2017). Mesohippus…”
Section: Appendix A: Biostratigraphymentioning
confidence: 96%
“…Thus, the new ash dates from the Toadstool Geologic Park sequence should provide a stronger geochronologic framework for calibrating the section than dates from the polarity reversals from the marine record. The Orellan-Chadronian boundary is placed at 33.9 Ma which is synchronous with the UPW at 33.939 ±0.033 Ma (Sahy et al, 2015), and near the Eocene-Oligocene boundary at 34.09 ± 0.08 Ma (Sahy et al, 2017). The accuracy of these dates is vital to correlating the terrestrial and marine climate records.…”
Section: Uncertainty In Magnetic Polarity Zonesmentioning
confidence: 99%
“…An obvious requirement is that geologic records are complete and that composite records from deep-sea cores are properly constructed in addition to adequate full recognition of cycles and their modulations. Uncertainties in radioisotopic dating, mostly linked to issues regarding the age calibration of standards, are pivotal to astronomical tuning as they are used as a first order constraint (see Sahy et al, 2017;Westerhold et al, 2012, for discussion). A final essential limitation is the accuracy of the orbital solution target curves which is known to worsen beyond some age back in the past (Laskar et al, 2004(Laskar et al, , 2011a(Laskar et al, , 2011b.…”
Section: Orbital Tuning Of the Middle Eocene Interval And Assessment mentioning
confidence: 99%