Astronomical calibration of the Paleocene time
The first complete cyclic sedimentary successions for the early Paleogene from drilling multiple holes have been retrieved during two ODP expeditions: Leg 198 (Shatsky Rise, NW Pacific Ocean) and Leg 208 (Walvis Ridge, SE Atlantic Ocean). These new records allow us to construct a comprehensive astro...
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creator | Westerhold, Thomas Röhl, Ursula Raffi, Isabella Fornaciari, Eliana Monechi, Simonetta Reale, Viviana Bowles, Julie Evans, Helen F. |
description | The first complete cyclic sedimentary successions for the early Paleogene from drilling multiple holes have been retrieved during two ODP expeditions: Leg 198 (Shatsky Rise, NW Pacific Ocean) and Leg 208 (Walvis Ridge, SE Atlantic Ocean). These new records allow us to construct a comprehensive astronomically calibrated stratigraphic framework with an unprecedented accuracy for both the Atlantic and the Pacific Oceans covering the entire Paleocene epoch based on the identification of the stable long-eccentricity cycle (405-kyr). High resolution X-ray fluorescence (XRF) core scanner and non-destructive core logging data from Sites 1209 through 1211 (Leg 198) and Sites 1262, 1267 (Leg 208) are the basis for such a robust chronostratigraphy. Former investigated marine (ODP Sites 1001 and 1051) and land-based (e.g., Zumaia) sections have been integrated as well. The high-fidelity chronology is the prerequisite for deciphering mechanisms in relation to prominent transient climatic events as well as completely new insights into Greenhouse climate variability in the early Paleogene. We demonstrate that the Paleocene epoch covers 24 long eccentricity cycles. We also show that no definite absolute age datums for the K/Pg boundary or the Paleocene–Eocene Thermal Maximum (PETM) can be provided by now, because of still existing uncertainties in orbital solutions and radiometric dating. However, we provide two options for tuning of the Paleocene which are only offset by 405-kyr. Our orbitally calibrated integrated Leg 208 magnetostratigraphy is used to revise the Geomagnetic Polarity Time Scale (GPTS) for Chron C29 to C25. We established a high-resolution calcareous nannofossil biostratigraphy for the South Atlantic which allows a much more detailed relative scaling of stages with biozones. The re-evaluation of the South Atlantic spreading rate model features higher frequent oscillations in spreading rates for magnetochron C28r, C27n, and C26n. |
doi_str_mv | 10.1016/j.palaeo.2007.09.016 |
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These new records allow us to construct a comprehensive astronomically calibrated stratigraphic framework with an unprecedented accuracy for both the Atlantic and the Pacific Oceans covering the entire Paleocene epoch based on the identification of the stable long-eccentricity cycle (405-kyr). High resolution X-ray fluorescence (XRF) core scanner and non-destructive core logging data from Sites 1209 through 1211 (Leg 198) and Sites 1262, 1267 (Leg 208) are the basis for such a robust chronostratigraphy. Former investigated marine (ODP Sites 1001 and 1051) and land-based (e.g., Zumaia) sections have been integrated as well. The high-fidelity chronology is the prerequisite for deciphering mechanisms in relation to prominent transient climatic events as well as completely new insights into Greenhouse climate variability in the early Paleogene. We demonstrate that the Paleocene epoch covers 24 long eccentricity cycles. We also show that no definite absolute age datums for the K/Pg boundary or the Paleocene–Eocene Thermal Maximum (PETM) can be provided by now, because of still existing uncertainties in orbital solutions and radiometric dating. However, we provide two options for tuning of the Paleocene which are only offset by 405-kyr. Our orbitally calibrated integrated Leg 208 magnetostratigraphy is used to revise the Geomagnetic Polarity Time Scale (GPTS) for Chron C29 to C25. We established a high-resolution calcareous nannofossil biostratigraphy for the South Atlantic which allows a much more detailed relative scaling of stages with biozones. 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These new records allow us to construct a comprehensive astronomically calibrated stratigraphic framework with an unprecedented accuracy for both the Atlantic and the Pacific Oceans covering the entire Paleocene epoch based on the identification of the stable long-eccentricity cycle (405-kyr). High resolution X-ray fluorescence (XRF) core scanner and non-destructive core logging data from Sites 1209 through 1211 (Leg 198) and Sites 1262, 1267 (Leg 208) are the basis for such a robust chronostratigraphy. Former investigated marine (ODP Sites 1001 and 1051) and land-based (e.g., Zumaia) sections have been integrated as well. The high-fidelity chronology is the prerequisite for deciphering mechanisms in relation to prominent transient climatic events as well as completely new insights into Greenhouse climate variability in the early Paleogene. We demonstrate that the Paleocene epoch covers 24 long eccentricity cycles. We also show that no definite absolute age datums for the K/Pg boundary or the Paleocene–Eocene Thermal Maximum (PETM) can be provided by now, because of still existing uncertainties in orbital solutions and radiometric dating. However, we provide two options for tuning of the Paleocene which are only offset by 405-kyr. Our orbitally calibrated integrated Leg 208 magnetostratigraphy is used to revise the Geomagnetic Polarity Time Scale (GPTS) for Chron C29 to C25. We established a high-resolution calcareous nannofossil biostratigraphy for the South Atlantic which allows a much more detailed relative scaling of stages with biozones. The re-evaluation of the South Atlantic spreading rate model features higher frequent oscillations in spreading rates for magnetochron C28r, C27n, and C26n.</description><subject>Biostratigraphy</subject><subject>Cyclostratigraphy</subject><subject>K/Pg boundary</subject><subject>Magnetochrons</subject><subject>Marine</subject><subject>ODP</subject><subject>Orbital tuning</subject><subject>Paleocene</subject><subject>PETM</subject><issn>0031-0182</issn><issn>1872-616X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2008</creationdate><recordtype>article</recordtype><recordid>eNp9kE9LxDAUxIMouK5-Aw89eWt9SZo0exGWxX-woAcFbyFNXjBL26xJV_Db26WePTwGhpmB9yPkmkJFgcrbXbU3ncFYMYCmglU1mSdkQVXDSknlxylZAHBaAlXsnFzkvAMAJjlbkGqdxxSH2AdrumK60CYzhjgU0RfjJxavpsNoccBiDD1ekjNvuoxXf7ok7w_3b5uncvvy-LxZb0vDJYwlFysBwii3Qu8celEzpaRxwgAysKaVTV3XRnrGRO0FUIetb1TLgSvXcORLcjPv7lP8OmAedR-yxa4zA8ZD1gyElKDUFKznoE0x54Re71PoTfrRFPQRjt7pGY4-wtGw0pM51e7mGk5PfAdMOtuAg0UXEtpRuxj-H_gF6ZJuuA</recordid><startdate>20080201</startdate><enddate>20080201</enddate><creator>Westerhold, Thomas</creator><creator>Röhl, Ursula</creator><creator>Raffi, Isabella</creator><creator>Fornaciari, Eliana</creator><creator>Monechi, Simonetta</creator><creator>Reale, Viviana</creator><creator>Bowles, Julie</creator><creator>Evans, Helen F.</creator><general>Elsevier B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7SN</scope><scope>7TG</scope><scope>7TN</scope><scope>C1K</scope><scope>F1W</scope><scope>H96</scope><scope>KL.</scope><scope>L.G</scope></search><sort><creationdate>20080201</creationdate><title>Astronomical calibration of the Paleocene time</title><author>Westerhold, Thomas ; Röhl, Ursula ; Raffi, Isabella ; Fornaciari, Eliana ; Monechi, Simonetta ; Reale, Viviana ; Bowles, Julie ; Evans, Helen F.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a360t-359505a8d9efddef542886ad5a0e20cab67444a6f2254f501debf78b3038d73e3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2008</creationdate><topic>Biostratigraphy</topic><topic>Cyclostratigraphy</topic><topic>K/Pg boundary</topic><topic>Magnetochrons</topic><topic>Marine</topic><topic>ODP</topic><topic>Orbital tuning</topic><topic>Paleocene</topic><topic>PETM</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Westerhold, Thomas</creatorcontrib><creatorcontrib>Röhl, Ursula</creatorcontrib><creatorcontrib>Raffi, Isabella</creatorcontrib><creatorcontrib>Fornaciari, Eliana</creatorcontrib><creatorcontrib>Monechi, Simonetta</creatorcontrib><creatorcontrib>Reale, Viviana</creatorcontrib><creatorcontrib>Bowles, Julie</creatorcontrib><creatorcontrib>Evans, Helen F.</creatorcontrib><collection>CrossRef</collection><collection>Ecology Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Oceanic Abstracts</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><jtitle>Palaeogeography, palaeoclimatology, palaeoecology</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Westerhold, Thomas</au><au>Röhl, Ursula</au><au>Raffi, Isabella</au><au>Fornaciari, Eliana</au><au>Monechi, Simonetta</au><au>Reale, Viviana</au><au>Bowles, Julie</au><au>Evans, Helen F.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Astronomical calibration of the Paleocene time</atitle><jtitle>Palaeogeography, palaeoclimatology, palaeoecology</jtitle><date>2008-02-01</date><risdate>2008</risdate><volume>257</volume><issue>4</issue><spage>377</spage><epage>403</epage><pages>377-403</pages><issn>0031-0182</issn><eissn>1872-616X</eissn><abstract>The first complete cyclic sedimentary successions for the early Paleogene from drilling multiple holes have been retrieved during two ODP expeditions: Leg 198 (Shatsky Rise, NW Pacific Ocean) and Leg 208 (Walvis Ridge, SE Atlantic Ocean). These new records allow us to construct a comprehensive astronomically calibrated stratigraphic framework with an unprecedented accuracy for both the Atlantic and the Pacific Oceans covering the entire Paleocene epoch based on the identification of the stable long-eccentricity cycle (405-kyr). High resolution X-ray fluorescence (XRF) core scanner and non-destructive core logging data from Sites 1209 through 1211 (Leg 198) and Sites 1262, 1267 (Leg 208) are the basis for such a robust chronostratigraphy. Former investigated marine (ODP Sites 1001 and 1051) and land-based (e.g., Zumaia) sections have been integrated as well. The high-fidelity chronology is the prerequisite for deciphering mechanisms in relation to prominent transient climatic events as well as completely new insights into Greenhouse climate variability in the early Paleogene. We demonstrate that the Paleocene epoch covers 24 long eccentricity cycles. We also show that no definite absolute age datums for the K/Pg boundary or the Paleocene–Eocene Thermal Maximum (PETM) can be provided by now, because of still existing uncertainties in orbital solutions and radiometric dating. However, we provide two options for tuning of the Paleocene which are only offset by 405-kyr. Our orbitally calibrated integrated Leg 208 magnetostratigraphy is used to revise the Geomagnetic Polarity Time Scale (GPTS) for Chron C29 to C25. We established a high-resolution calcareous nannofossil biostratigraphy for the South Atlantic which allows a much more detailed relative scaling of stages with biozones. The re-evaluation of the South Atlantic spreading rate model features higher frequent oscillations in spreading rates for magnetochron C28r, C27n, and C26n.</abstract><pub>Elsevier B.V</pub><doi>10.1016/j.palaeo.2007.09.016</doi><tpages>27</tpages></addata></record> |
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subjects | Biostratigraphy Cyclostratigraphy K/Pg boundary Magnetochrons Marine ODP Orbital tuning Paleocene PETM |
title | Astronomical calibration of the Paleocene time |
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