Constraining the age of the Matuyama-Brunhes reversal using intercalibrated 40Ar/39Ar and astronomical ages of the Bishop Tuff and Australasian Tektite

Tiffany Rivera, Michael Storey, Heiko Palike, Christian Zeeden

    Publikation: KonferencebidragKonferenceabstrakt til konferenceForskning

    Resumé

    Recent high-resolution δ18O records from North Atlantic (I)ODP cores, with reliable paleomagnetic signals, have placed the mean age of the Matuyama-Brunhes (MB) geomagnetic polarity reversal ca. 8 ka younger than previous estimates when correlated to ice-volume age models (Channell et al., 2010). However, this age offset is not synchronous with a new astronomically intercalibrated 40Ar/39Ar age for the normal-polarity Quaternary Bishop Tuff, stratigraphically above the MB boundary by approximately 15 ka. In order to best constrain the age of the boundary, an astronomically calibrated radio-isotopic age is needed on a datable unit from the reversed-polarity side of the MB boundary. The Australasian tektite is a suitable unit from the Matuyama chron for dating the MB boundary because the positions of microtektite layers relative to the MB boundary have been documented in (I)ODP and other drill cores. Previous analyses of the drill cores have estimated the duration between the tektite layer and the MB boundary between 8 and 12 ka, and an astronomical age has been assigned to this unit (Horng et al., 2002). Using a Nu Instruments Noblesse multi-collector noble gas mass spectrometer, we present 40Ar/39Ar step-heating and fusion age data, relative to the astronomically calibrated Fish Canyon sanidine, on the Australasian tektite, and have updated the tuning model for this layer using the La2004 orbital solutions. Using 40Ar/39Ar ages for these two units that bracket the boundary along with sedimentation rates determined through drill core analysis, we approach the MB boundary from both sides to arrive at a boundary age that is consistent with independent astronomical ages proposed for the polarity transition. This novel approach provides a best-fit age for the MB boundary that incorporates radio-isotopic dating, astrochronologies, and sedimentation rates.

    The research leading to these results has received funding from the European Community's Seventh Framework Programme [FP7/2007-2013] under grant agreement no. 215458.
    OriginalsprogEngelsk
    Publikationsdatoaug. 2011
    StatusUdgivet - aug. 2011
    BegivenhedGeological Society of America Annual meeting & Exposition - Minneapolis, MN, USA
    Varighed: 9 okt. 201112 okt. 2011

    Konference

    KonferenceGeological Society of America Annual meeting & Exposition
    LandUSA
    ByMinneapolis, MN
    Periode09/10/201112/10/2011

    Citer dette

    Rivera, T., Storey, M., Palike, H., & Zeeden, C. (2011). Constraining the age of the Matuyama-Brunhes reversal using intercalibrated 40Ar/39Ar and astronomical ages of the Bishop Tuff and Australasian Tektite. Abstract fra Geological Society of America Annual meeting & Exposition, Minneapolis, MN, USA.
    Rivera, Tiffany ; Storey, Michael ; Palike, Heiko ; Zeeden, Christian. / Constraining the age of the Matuyama-Brunhes reversal using intercalibrated 40Ar/39Ar and astronomical ages of the Bishop Tuff and Australasian Tektite. Abstract fra Geological Society of America Annual meeting & Exposition, Minneapolis, MN, USA.
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    title = "Constraining the age of the Matuyama-Brunhes reversal using intercalibrated 40Ar/39Ar and astronomical ages of the Bishop Tuff and Australasian Tektite",
    abstract = "Recent high-resolution δ18O records from North Atlantic (I)ODP cores, with reliable paleomagnetic signals, have placed the mean age of the Matuyama-Brunhes (MB) geomagnetic polarity reversal ca. 8 ka younger than previous estimates when correlated to ice-volume age models (Channell et al., 2010). However, this age offset is not synchronous with a new astronomically intercalibrated 40Ar/39Ar age for the normal-polarity Quaternary Bishop Tuff, stratigraphically above the MB boundary by approximately 15 ka. In order to best constrain the age of the boundary, an astronomically calibrated radio-isotopic age is needed on a datable unit from the reversed-polarity side of the MB boundary. The Australasian tektite is a suitable unit from the Matuyama chron for dating the MB boundary because the positions of microtektite layers relative to the MB boundary have been documented in (I)ODP and other drill cores. Previous analyses of the drill cores have estimated the duration between the tektite layer and the MB boundary between 8 and 12 ka, and an astronomical age has been assigned to this unit (Horng et al., 2002). Using a Nu Instruments Noblesse multi-collector noble gas mass spectrometer, we present 40Ar/39Ar step-heating and fusion age data, relative to the astronomically calibrated Fish Canyon sanidine, on the Australasian tektite, and have updated the tuning model for this layer using the La2004 orbital solutions. Using 40Ar/39Ar ages for these two units that bracket the boundary along with sedimentation rates determined through drill core analysis, we approach the MB boundary from both sides to arrive at a boundary age that is consistent with independent astronomical ages proposed for the polarity transition. This novel approach provides a best-fit age for the MB boundary that incorporates radio-isotopic dating, astrochronologies, and sedimentation rates.The research leading to these results has received funding from the European Community's Seventh Framework Programme [FP7/2007-2013] under grant agreement no. 215458.",
    author = "Tiffany Rivera and Michael Storey and Heiko Palike and Christian Zeeden",
    year = "2011",
    month = "8",
    language = "English",
    note = "Geological Society of America, Annual Meeting 2011 ; Conference date: 09-10-2011 Through 12-10-2011",

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    Rivera, T, Storey, M, Palike, H & Zeeden, C 2011, 'Constraining the age of the Matuyama-Brunhes reversal using intercalibrated 40Ar/39Ar and astronomical ages of the Bishop Tuff and Australasian Tektite' Geological Society of America Annual meeting & Exposition, Minneapolis, MN, USA, 09/10/2011 - 12/10/2011, .

    Constraining the age of the Matuyama-Brunhes reversal using intercalibrated 40Ar/39Ar and astronomical ages of the Bishop Tuff and Australasian Tektite. / Rivera, Tiffany; Storey, Michael; Palike, Heiko; Zeeden, Christian.

    2011. Abstract fra Geological Society of America Annual meeting & Exposition, Minneapolis, MN, USA.

    Publikation: KonferencebidragKonferenceabstrakt til konferenceForskning

    TY - ABST

    T1 - Constraining the age of the Matuyama-Brunhes reversal using intercalibrated 40Ar/39Ar and astronomical ages of the Bishop Tuff and Australasian Tektite

    AU - Rivera, Tiffany

    AU - Storey, Michael

    AU - Palike, Heiko

    AU - Zeeden, Christian

    PY - 2011/8

    Y1 - 2011/8

    N2 - Recent high-resolution δ18O records from North Atlantic (I)ODP cores, with reliable paleomagnetic signals, have placed the mean age of the Matuyama-Brunhes (MB) geomagnetic polarity reversal ca. 8 ka younger than previous estimates when correlated to ice-volume age models (Channell et al., 2010). However, this age offset is not synchronous with a new astronomically intercalibrated 40Ar/39Ar age for the normal-polarity Quaternary Bishop Tuff, stratigraphically above the MB boundary by approximately 15 ka. In order to best constrain the age of the boundary, an astronomically calibrated radio-isotopic age is needed on a datable unit from the reversed-polarity side of the MB boundary. The Australasian tektite is a suitable unit from the Matuyama chron for dating the MB boundary because the positions of microtektite layers relative to the MB boundary have been documented in (I)ODP and other drill cores. Previous analyses of the drill cores have estimated the duration between the tektite layer and the MB boundary between 8 and 12 ka, and an astronomical age has been assigned to this unit (Horng et al., 2002). Using a Nu Instruments Noblesse multi-collector noble gas mass spectrometer, we present 40Ar/39Ar step-heating and fusion age data, relative to the astronomically calibrated Fish Canyon sanidine, on the Australasian tektite, and have updated the tuning model for this layer using the La2004 orbital solutions. Using 40Ar/39Ar ages for these two units that bracket the boundary along with sedimentation rates determined through drill core analysis, we approach the MB boundary from both sides to arrive at a boundary age that is consistent with independent astronomical ages proposed for the polarity transition. This novel approach provides a best-fit age for the MB boundary that incorporates radio-isotopic dating, astrochronologies, and sedimentation rates.The research leading to these results has received funding from the European Community's Seventh Framework Programme [FP7/2007-2013] under grant agreement no. 215458.

    AB - Recent high-resolution δ18O records from North Atlantic (I)ODP cores, with reliable paleomagnetic signals, have placed the mean age of the Matuyama-Brunhes (MB) geomagnetic polarity reversal ca. 8 ka younger than previous estimates when correlated to ice-volume age models (Channell et al., 2010). However, this age offset is not synchronous with a new astronomically intercalibrated 40Ar/39Ar age for the normal-polarity Quaternary Bishop Tuff, stratigraphically above the MB boundary by approximately 15 ka. In order to best constrain the age of the boundary, an astronomically calibrated radio-isotopic age is needed on a datable unit from the reversed-polarity side of the MB boundary. The Australasian tektite is a suitable unit from the Matuyama chron for dating the MB boundary because the positions of microtektite layers relative to the MB boundary have been documented in (I)ODP and other drill cores. Previous analyses of the drill cores have estimated the duration between the tektite layer and the MB boundary between 8 and 12 ka, and an astronomical age has been assigned to this unit (Horng et al., 2002). Using a Nu Instruments Noblesse multi-collector noble gas mass spectrometer, we present 40Ar/39Ar step-heating and fusion age data, relative to the astronomically calibrated Fish Canyon sanidine, on the Australasian tektite, and have updated the tuning model for this layer using the La2004 orbital solutions. Using 40Ar/39Ar ages for these two units that bracket the boundary along with sedimentation rates determined through drill core analysis, we approach the MB boundary from both sides to arrive at a boundary age that is consistent with independent astronomical ages proposed for the polarity transition. This novel approach provides a best-fit age for the MB boundary that incorporates radio-isotopic dating, astrochronologies, and sedimentation rates.The research leading to these results has received funding from the European Community's Seventh Framework Programme [FP7/2007-2013] under grant agreement no. 215458.

    M3 - Conference abstract for conference

    ER -

    Rivera T, Storey M, Palike H, Zeeden C. Constraining the age of the Matuyama-Brunhes reversal using intercalibrated 40Ar/39Ar and astronomical ages of the Bishop Tuff and Australasian Tektite. 2011. Abstract fra Geological Society of America Annual meeting & Exposition, Minneapolis, MN, USA.