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Magnetostratigraphy Wout Krijgsman & Cor Langereis
Paleomagnetic Laboratory Fort Hoofddijk Department of Earth Sciences Utrecht University
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Magnetostratigraphy Possibilities, pitfalls and applications
Cor Langereis, Wout Krijgsman Paleomagnetic Laboratory Fort Hoofddijk Dept. of Earth Sciences, Utrecht University Giovanni Muttoni Dept. of Earth Sciences, University of Milan Manfred Menning Geoforschungs Zentrum Potsdam, Germany
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Magnetostratigraphy a dipole reversing at irregular times
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Origin of reversals Mantle Liquid outer core Solid inner core
Convection time scale ~100 Myr Reversal frequency, superchrons Solid inner core Diffusion time scale 3-5 kyr Stabilises geodynamo process Kuang & Bloxham, 1997 Liquid outer core Convection time scale yr Geodynamo action: Secular variation, excursions, reversals
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GPTS: Geomagnetic Polarity Time Scale
Lavas & K/Ar dating ? Sediments (DSDP) & biostratigraphy Barcode: may give unique solutions - but of an essentially BINARY nature - and can be distorted in the rock record Marine magnetic anomalies
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Magnetostratigraphy part of integrated stratigraphy
Biostratigraphy: first-order chronology - taxonomy, reworking, diachrony, ages Magnetostratigraphy: globally synchonous barcode - depends on good paleomagnetic signal & recording Cyclostratigraphy: astronomical dating, fine-tuning - astronomical solutions (> 20 Ma) - interpretation of phase relations
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Integrated stratigraphy
Biostratigraphy - first-order chronology Magnetostratigraphy - globally synchonous barcode Cyclostratigraphy - fine-tuning & astronomical dating
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Geomagnetic time scales
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K/Ar dating of lavas Cox et al., 1964
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Magneto-bio-stratigraphy
Opdyke et al., 1966 - Advent of deep-sea cores: inclination only - Biostratigraphy (faunal zones) for dating
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Marine magnetic anomalies
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Marine magnetic anomalies
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Marine magnetic anomalies
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Pitman and Heirtzler, 1966
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Marine Magnetic Anomalies
Deep Sea Cores vs.
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Continental drift
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Developing the GPTS
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Paleomagnetism DRM vs. CRM: - inclination error - delayed NRM acquisition
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Accuracy of recording reversals
Watkins, 1968
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Geomagnetic Polarity Time Scale (GPTS) or …
Polarity zones (subchrons) or excursions (cryptochrons) ? Geomagnetic Polarity Time Scale (GPTS) or … Geomagnetic Instability Time Scale (GITS) ‘reversal excursions’
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Magnetostratigraphic resolution
Laj & Channell (2007) proposed: Resolution depends on: - sampling resolution (easy … just take more samples) - sediments: sedimentation rate & suitable recording medium - diagenesis, lock-in depth, overprints, etc., etc.
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Magnetostratigraphic resolution
Nomenclature OK … but for practical (integrated) stratigraphy and constraints on chronostratigraphy ?
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Marine magnetic anomalies
World crustal age
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Triassic magnetostratigraph … beyond the sea floor record
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Even older: magneto-stratigraphy ?
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The times they are a-changin’
(Bob Dylan, 1964) Wout Krijgsman
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Time: dates and rates Tools: Biostratigraphy Magnetostratigraphy
Astrochronology Isotopic dating Aims: Marine-continental Paratethys-Mediterranean Synchrony-diachrony Event stratigraphy
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Geological Time Scale Gradstein et al. (2004) GTS2004
Neogene: based on astronomical ages Why is it so important that both methods are identical? The new GTS as published last year is based on astronomical ages for the Neogene part of the time scale and on radio-isotopic ages for e.g. the Paleogene part. The geological time scale is the framework for deciphering the history of the Earth and therefore it is crucial that astronomical and radio-isotopic dating methods produce identical results. The base of the Neogene is defined in the Lemme-Carrosio section in northern Italy. This section correlated to ODP site 926 based on detailed calcareous nannofossil correlations. ODP site 926 is astronomically tuned to La2004 and yields an age of Ma. Wilson et al. (2002), Naish et al. (2001) published Ma n=19 and Ma n=52 relative to FCT 27.84, single crystal anorthoclase for two tuffs bracketing Oligocene-Miocene boundary….Still to be explained…. Paleogene: based on radio-isotopic ages
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Magnetostratigraphy & Cyclostratigraphy
Astronomical Tuning Climate cycles Astronomical solutions Hilgen et al., 2004
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Astronomical Polarity Time Scale (APTS) for the Mediterranean Neogene
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Sicily, 2 weeks ago
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Sampling, 15 years ago Sicily, 2 weeks ago
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Cyclostratigraphy & astronomical tuning ... ATNTS in GTS2004
Accurate definition of GSSP (Oued Akrech, Hilgen et al., 2000) Lourens et al., 2004
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Biostratigraphy vs. Magnetostratigraphy
Problems: Taxonomy Diachrony Reworking Ages Problems: Correlation Primary signal vs. overprint Ages
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Correlation Requires unique pattern fit Magneto age 7.6 ± 0.1 K/Ar age
6.16 ± 0.30 Garces et al., 2001
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Ages GPTS not independent of other dating techniques
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The times they are a-changing’
Ages change with time …
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Astrochronology Problems: Cycle recognition Phase relation Correlation
Astronomical solution
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Astrochronology: correlation of cyclic variations in the geological record to computed astronomical (age) curves
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Milankovitch cycles
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Sapropel-marl cycles, upper Miocene, Sicily
Eccentricity minimum Precession minimum Gibliscemi, Sicily, Italy
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Partial Unit-Stratotype of the Zanclean stage (Lower Pliocene)
Punta di Maiata, Sicily, Italy
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Lignite-marls cycles, Mio-Pliocene, Greece
Precession minimum Ptolemais quarry, Greece
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Sand-marls cycles, Mio-Pliocene, Romania PONTIAN
Acc. rate in C3r = 137cm/kyr Periodicity cycles = 22.7kyr Putna river section, eastern Carpathians Another aspect is the Cyclic pattern of the sedimentary rocks .Vertically bedded sandstones units, alternating with finer sediments on Putna Valley. The calculated duration of each cycle is very close to 21.7 which is very close to the average duration of the Precession Cycle.
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Clay-carbonate cycles, Miocene, Spain
Orera section, Spain
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Clay-carbonate cycles, Triassic, USA
Painted desert/Petrified forrest, Arizona
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Miocene APTS Astrochronology for the Late Miocene
Sections on Crete correlated bed-to-bed to Sicily Hilgen et al. (1995)
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Northern Apennines (Italy)
Messinian evaporites Northern Apennines (Italy)
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Messinian Chronology
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Messinian Salinity Crisis Evaporites synchronous
all over Mediterranean at ~5.96 Ma Krijgsman et al. 1999
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Chronology evaporites
Cyclostratigraphy Italy: Evaporites 16 cycles (Marabini and Vai, 1988)
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Chronology evaporites
Cyclostratigraphy Spain: Evaporites cycles (Dronkert, 1976; M.S.G.l. Fortuin et al., 2000; Sed. Geol.)
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Chronology evaporites Top of Lower Evaporites 5.60-5.52 Ma
(Krijgsman et al. 2001; Sed. Geol.)
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La93 <> La2004
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Radio-Isotopic dating
Problems: Technique (K/Ar vs. Ar/Ar) Error determination Mineral dating standards
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Error determination Ar/Ar ratio: mass spectrometer precision depends on e.g. measurement protocol, mass discrimination Decay constant J is an irradiation parameter and its accuracy depends on an accurately known age of a mineral standard.
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Mineral dating standards:
Fish Canyon Tuff
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Magnetostratigraphy Tortonian Salinity Crisis: Fortuna Basin
Betic Corridor problem K/Ar age of 6.16 ± 0.30 Ar/Ar age of 7.71 ± 0.11 Magnetostratigraphy Tortonian Salinity Crisis: Fortuna Basin (Garces et al. 1998; 2001)
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Method Garces et al. (2001) Magnetic age: 7.6 ± 0.1 Ma
Bellon et al. (1983) K/Ar age: 6.16 ± 0.30 Ma Kuiper et al. (2002) Ar/Ar age: 7.71 ± Ma
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Isotopic ages and astronomical ages
Intercalibration Isotopic ages and astronomical ages Faneromeni section: Messinian, Crete
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40Ar/39Ar vs. astronomical ages
6.94 Ma Fan-a1, Crete Miocene, marine 2: 0.01 Ma; N = 44 3 different irradiations 6.65 6.75 6.85 6.95 7.05 7.15 Age (Ma) Kuiper et al., 2003
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40Ar/39Ar vs astronomical ages
Ptolemais SR3M Ptolemais SLM3T 4.31Ma 4.39 Ma 4 4.1 4.2 4.3 4.4 4.5 4 4.1 4.2 4.3 4.4 4.5 Age (Ma) Age (Ma) Messadit Me-11 Messadit Me-1 6.45 Ma 6.58 Ma 6.2 6.3 6.4 6.5 6.6 6.7 6.2 6.3 6.4 6.5 6.6 6.7 Age (Ma) Age (Ma)
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Intercalibration Isotopic ages and astronomical ages Morocco / Spain
Kuiper et al., 2008
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Intercalibration Inter-laboratory calibration
Kuiper et al., 2008 (Science)
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Intercalibration Isotopic ages and astronomical ages
K/T Boundary Zumaia (Spain): new age of Ma
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Mediterranean vs Paratethys
Late Miocene -Early Pliocene Since the end of Oligocene, Paratethys area evolved as the northern branch of the Neo- Tethys Ocean while its southern branch is the actual Mediterranean region. It is very important to know the connections between water masses. When they were open or closed we do not know. We do not know even all of them were there or not. Taking into account that we that for Mediterranean already exists a very good time frame we want to do the same for the eastern Paratethys. EVOLVED
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‘Evolution’ of the Time Scales from Eastern Paratethys
~3Ma ~0.3Ma 10 TIMES longer
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Carpathians foredeep Pontian Dacian Stoica et al., submittted
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Carpathians foredeep EC SC Vasiliev et al., 2004; 2005
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Putna Valley PONTIAN Acc. rate in C3r = 137cm/kyr
Periodicity cycles = 22.7kyr Another aspect is the Cyclic pattern of the sedimentary rocks .Vertically bedded sandstones units, alternating with finer sediments on Putna Valley. The calculated duration of each cycle is very close to 21.7 which is very close to the average duration of the Precession Cycle.
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Eastern Southern Carpathians Carpathians
Schematic time scale for Mediterranean. The local stage boundaries show no direct connection with the changing from Mediterranean. The desiccation and the Pliocene flooding from Mediterranean seems to not be reflected at all in the western most part of the eastern Paratethys. Anyway the presumed influx of Paratethyan water into Mediterranean did not left any sign in Paratethys. no clue. The Meotian/Pontian boundary which was associated previously with the Tortonian/Messinian boundary can be maybe connected now with the onset of the Messinian Salinity crisis. The change in the magnetic components from oxic to anoxic conditions reveal a huge change in the basin configuration occurring at the Me/Po boundary, in the C3r chron. It may be related to the MsC or not. Eastern Carpathians Southern Carpathians
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The evolution of Paratethys: the lost sea of Central Eurasia
Vici project 2011 3 PhD / 2 Postdoc positions
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