Be-10 inheritance in young New Zealand boulders


Glacial landforms, especially moraines, have long been used as indicators of decreased temperature or increased precipitation in the past. Cosmogenic exposure dating of moraine boulders provides a method for estimating moraine ages. However, geomorphic processes interfere with cosmogenic exposure dating. To improve the accuracy of the cosmogenic exposure dating method, quantitative methods for assessing the effects of geomorphic processes on cosmogenic exposure dating are needed. To address this need, this dissertation describes models of two geomorphic processes and their effects on the cosmogenic exposure dating of moraines. These processes are moraine degradation and inheritance. Both models use Monte Carlo techniques to estimate the statistical distributions of exposure dates from moraine boulders, given specific assumptions about the histories of the boulders.

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Most commonly employed among these are cosmogenic exposure dating, uranium-series dating, optically stimulated luminescence, and radiocarbon dating. Because the geologic samples collected may have experienced very different pre-, syn-, and post-formation histories, the dates may be interpreted as max ages, min ages, or something in between, with implications for whether a fault slip rate should be considered an upper or lower limit. For this reason, the practice of using multiple geochronometers to constrain a range of possible surface ages and slip rates is ideal and has become common enough to begin assessing how well dates obtained using different methods agree.

Where two dating methods were used, it was most common to compare exposure dates to those obtained using another method. Inheritance in exposure ages from clasts remains challenging estimate, and only in rare cases does subtracting the nuclide concentration found in the modern wash from that measured on surface bring the latter into concordance with independent dates.

Cosmogenic depth profiles are useful for estimating inheritance in the clast size sampled, but 2 in 3 depth profiles exhibited distributions too scattered for a date to be calculated.

This suggests that initial 7 Be/ 10 Be in concrete may be sensitive to dry component inheritance. Additional measurements from a variety of concrete sources would be necessary to determine whether this inheritance is systematic or highly variable.

At the time that Darwin’s On the Origin of Species was published, the earth was “scientifically” determined to be million years old. By , it was found to be 1. In , science firmly established that the earth was 3. Finally in , it was discovered that the earth is “really” 4. In these early studies the order of sedimentary rocks and structures were used to date geologic time periods and events in a relative way. At first, the use of “key” diagnostic fossils was used to compare different areas of the geologic column.

Although there were attempts to make relative age estimates, no direct dating method was available until the twentieth century. However, before this time some very popular indirect methods were available.

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Chronology of last earthquake on Firouzkuh Fault using by C14 The Firouzkuh fault with about 70 km length extending from east of Mosha fault in Aminabad villag Geologically this fault bounded between Jurassic – Cretaceous deposits in east hanging wall and Plio-Quaternary sediments in the west foot wall fault, Aghanabati and Hamedi, This fault with NE-SW trend, located at northern part of south Firouzkuh high lands, and is partially compatible with F magnetism Yossefi and Firedburg, This fault initially was known as south trending thrust fault Berberian et al.

In bigger scale, presence of eastern mountains and pattern of younger deformation in fault plain, especially in Firouzkuh domain, there is an evidence of left-Lateral dextral fault with vertical component for Firouzkuh fault.

dating of morphotectonic features In order to date the time of deposition or abandonment of the different terraces, we used radiocarbon as well as in-situ produced cosmogenic .

In the sciences, it is important to distinguish between precision and accuracy. If we use the analogue of a clock we can investigate this further. Your wrist watch may measure time with a precision of one second. A stop watch may time your race with a precision of one hundredth of a second. However, if the clocks change and you forget to reset your wrist watch, then you have a very precise time but it is not very accurate — you will be an hour early or late for all of your meetings!

Scientists want measurements that are both accurate and precise… but it can be difficult to tell sometimes whether very precise measurements are actually accurate without an independent reference age see top right image versus bottom right image. Accurate measurements fall in the bulls eye.

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While surface exposure dating using cosmogenic 10Be and 26Al would seem to be an ideal dating method, the surfaces are composed of individual clasts, each with its own complex history of exposure and burial. The stochastic nature of burial depth and hence in nuclide production in these clasts during exhumation and fluvial transport, and during post-depositional stirring, results in great variability in clast nuclide concentrations.

We present a method for dealing with the problem of pre-depositional inheritance of cosmogenic nuclides. We generate samples by amalgamating many individual clasts in order to average over their widely different exposure histories.

Cosmogenic Exposure Dating and the Age of the Earth Cosmogenic nuclides are nuclides formed by the interaction of ‘target’ atoms with cosmic radiation. Such nuclides are formed in space, in the atmosphere (e.g. 14 C and 10 Be), and in situ within minerals at or near the earth’s surface (e.g. 10 Be, 26 Al, and 21 Ne).

Quaternary Science Reviews 26 — Abstract Surface-exposure 10Be ages have been obtained on boulders from three post-Pinedale end-moraine complexes in the Front Range, Colorado. Boulder rounding appears related to the cirque-to-moraine transport distance at each site with subrounded boulders being typical of the 2-km-long Chicago Lakes Glacier, subangular boulders being typical of the 1-km-long Butler Gulch Glacier, and angular boulders being typical of the few-hundred-m-long Isabelle Glacier.

We suggest that this moraine was deposited during the 8. The surface-exposure ages of eight of nine subrounded boulders from the Chicago Lakes area fall within the The general lack of inheritance in the eight samples probably stems from the fact that only a few thousand years intervened between the retreat of the Pinedale glacier and the advance of the Chicago Lakes glacier; in addition, bedrock in the Chicago Lakes cirque area may have remained covered with snow and ice during that interval, thus partially shielding the bedrock from cosmogenic radiation.

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Advanced Search Summary 10Be and 36Cl cosmic ray exposure CRE and optically stimulated luminescence OSL dating of offset terraces have been performed to constrain the long-term slip rate of the Dehshir fault. For each terrace, there is a statistical outlier with a younger age of The late sediments aggraded before the abandonment of T2 and inset levels, T1 b and T1a, yielded OSL ages of, respectively, These discrepancies between the CRE and OSL ages exemplify the variability of the inheritance and indicate the youngest cobble on a terrace, that minimizes the inheritance, is the most appropriate CRE age for approaching that of terrace abandonment.

However, the upper bound on the age of abandonment of a terrace that is young with respect to the amount of inheritance is best estimated by the OSL dating of the terrace material.

Post-depositional impacts on ‘Findlinge’ (erratic boulders) and their implications for surface-exposure dating Keywords Cosmogenic 10Be Findling Inheritance Exhumation Human impact Alpine Foreland 1 Introduction An erratic boulder, ‘Findling’ in German, is an allochtho-.

Five limestone boulders from an end moraine in the Galicica Mountains The 36Cl concentrations from the five boulders are identical within their measurement uncertainties ruling out major effects of inheritance, erosion, or snow cover. The calculated ages are very consistent ranging from The applied corrections for weathering and snow shielding cause a shift to older ages in the order of magnitude of ca. The ages point to a moraine formation during the Younger Dryas period, consistent with the timing of the last deglaciation in the Galicica Mountains derived from previous geomorphological studies in the area.

The formation of a glacier was likely favoured by several topoclimatic factors, accounting for additional snow input. An explanation might be a combination of the small size of the cirque glacier, generating only small amounts of debris, and the karstic bedrock, which hampers fluvial transport and acts by its aquifer system as a natural sediment trap, as the fluvial transport of the sediments to the lakes is absorbed by the karst system.

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Repka a, Robert S. Anderson a, , Robert C. While surface exposure dating using cosmogenic10Be and 26Al would seem to be an ideal dating method, the surfaces are composed of individual clasts, each with its owncomplex history of exposure and burial. The stochastic nature of burial depth and hence in nuclide production in these clastsduring exhumation and fluvial transport, and during post-depositional stirring, results in great variability in clast nuclideconcentrations.

We present a method for dealing with the problem of pre-depositional inheritance of cosmogenic nuclides. We generate samples by amalgamating many individual clasts in order to average over their widely different exposurehistories.

Cosmogenic nuclide depth-profiles are used to calculate the age of landforms, the rates at which erosion has affected them since their formation and, in case of deposits, the paleo-erosion rate in the source area. However, two difficulties are typically encountered: 1) old deposits or strongly affected by cosmogenic nuclide inheritance often appear to be saturated, and 2) a full propagation of.

Cosmogenic Exposure Dating and the Age of the Earth Cosmogenic nuclides are nuclides formed by the interaction of ‘target’ atoms with cosmic radiation. Such nuclides are formed in space, in the atmosphere e. The accumulation of cosmogenic nuclides in minerals at or near the earth’s surface provides a basis for exposure ‘dating‘ of landforms, the quantification of erosion rates, and other geologic applications Bierman, ; Cerling and Craig, ; Gosse and Phillips, Independent evidence discussed below strongly suggests that production rates of these nuclides have remained constant or nearly so, validating their use in geochronometry.

This essay focuses on cosmogenic exposure dating, a method of dating rock surfaces which has been compared to using the redness of someone’s skin in order to estimate the duration of exposure to sunlight an analogy attributed to Edward Evenson; Gosse and Phillips, Cosmogenic Nuclide Production The earth is constantly being bombarded by so-called galactic cosmic radiation. This radiation interacts with nuclei in the atmosphere to produce garden variety or ‘meteoric’ cosmogenic nuclides e.

These interactions produce a cascade of secondary particles, primarily neutrons and muons, which interact with target nuclei within minerals such as quartz and olivine at the earth’s surface, producing terrestrial cosmogenic nuclides TCN. The primary nuclear processes by which cosmogenic nuclides are produced are spallation, muon capture, and neutron activation Bierman, p. The cosmogenic nuclides most widely utilized for geologic applications are the radionuclides 10Be, 26Al, and 36Cl, and the stable nuclides 3He and 21Ne.

The stable nuclide 3He is produced primarily by spallation from O, Mg, Si, Ca, Fe, Al, and is most often measured in olivine and pyroxene.

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Burgette , Nathaniel Lifton , Katherine M. Previous studies have suggested that deformation rates on this fault vary spatially as part of the broader plate boundary system, or that the locus of deformation has migrated southward into the Los Angeles basin over the Quaternary. A well-preserved flight of fan terraces in the Arroyo Seco area of Altadena and Pasadena, CA provides a location to assess whether there is a long-term reduction in strain on the SMF.

Our approach uses cosmogenic 10Be and 26Al exposure dating, but targets glacial outwash associated with these limits and uses depth-profiles and surface cobble samples, thereby accounting for surface deflation and inheritance.

Suggested articles Citations A complete and easily accessible means of calculating surface exposure ages or erosion rates from Be and Al measurements. A new tectonic discontinuity in the Betic Cordillera deduced from active tectonics and seismicity in the Tabernas Basin. A numerical modelling technique that can account for alternations of uplift and subsidence revealed by Late Cenozoic fluvial sequences.

A postglacial chronology for some alluvial valleys in Wyoming. Geological Survey Water Supply Paper United States Government printing office, A robust feldspar luminescence dating method for Middle and Late Pleistocene sediments. A two-step process for the reflooding of the Mediterranean after the Messinian Salinity Crisis.

Explicit treatment of inheritance in dating depositional … – GSA Journals

Hidy FS Abstract We tested the feasibility of using cosmogenically produced beryllium-7 7Be and beryllium 10Be isotopes to date concrete, a common tunnel construction material. A series of experimental concrete and concrete component samples were analyzed for 7Be and 10Be, which led to the following key findings: Both 7Be and 10Be are present at levels detectable by accelerator mass spectrometry AMS in concrete and many concrete components cement, sand, aggregate, precipitation.

However, neither is detectable in tap water. Isotopic concentrations measured over time in concrete change as predicted by decay laws. Sustained exposure to air does not significantly contribute to 7Be or 10Be; exposure to rain water contributes significantly to 7Be levels, but not to 10Be levels.

Cosmogenic Radionuclide (CRN) Dating CRN geochronological studies constrain the age of abandonment of each alluvial surface, which, combined with measured vertically off- inheritance or prior exposure of the sampled sur-face. Inheritance, or prior exposure of sampled surfaces, can yield older surface exposure ages.

Cosmic rays break atoms in surface rocks at predictable rates. Thus, the ages of moraines are directly related to the concentrations of cosmic ray-produced nuclides in rocks on the moraine surfaces, under ideal circumstances. However, many geomorphic processes may interfere with cosmogenic exposure dating. Because of these processes, boulders sometimes arrive at the moraines with preexisting concentrations of cosmogenic nuclides, or else the boulders are partly shielded from cosmic rays following deposition.

Many methods for estimating moraine ages from cosmogenic exposure dates exist in the literature, but we cannot assess the appropriateness of these methods without knowing the parent distribution from which the dates were drawn on each moraine. Here, we make two contributions. First, we describe numerical models of two geomorphic processes, moraine degradation and inheritance, and their effects on cosmogenic exposure dating.


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