school of geosciences - university of edinburghfigure 2. a) cosmogenic nuclide depth profiles can...

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Cosmogenic nuclide concentrations are commonly used to determine ‘exposure ages’ and ‘erosion rates’. Some common examples include: Exposure dating • Glacier erosion/deposition surfaces: striated bedrock, erratics, moraines • Fluvial and glaciofluvial terraces • Buried sediments: caves, glacial till • Rockfalls • Fault scarps • Lava flows • Flood deposits • Alluvial fans Rates of landscape change • Rock surface erosion rates • Land surface degradation rates • Basinwide erosion rates • River incision rates • Modern erosion (meteoric 10 Be) • Faultslip rates 1 INTRODUCTION 5 APPLICATIONS 3 CAPABILITIES 2 FACILITY DESCRIPTION Terrestrial cosmogenic nuclides form in rock minerals exposed in the upper ~2 m of Earth’s surface through interaction with cosmic radiation (Fig. 1). The concentration of cosmogenic nuclides in near surface rocks will increase through time until their production is matched by their losses through physical erosion and radioactive decay. Thus, the concentration of cosmogenic nuclides in rock or sediment is a balance between its exposure time and erosion rate. This knowledge can be applied in a range of settings to quantify dates and rates of Earth surface processes. This facility is designed to make possible the measurement of cosmogenic nuclides in rock and sediment. Here, we chemically extract cosmogenic isotopes from rock and sediment and prepare targets ready for measurement by Accelerator Mass Spectrometry (AMS). We are able to support preparation work for all of the major cosmogenic isotopes including cosmogenic 10 Be, 26 Al, 36 Cl, 21 Ne, 3 He and 14 C. The AMS or MS analyses are conducted at the Scottish Universities Environment Research Centre or other collaborative institutions. Rock crushing and sieving Dedicated lab space Disk mill Sieves Frantz magnetic separator Sample splitter Extraction of quartz from rock/sediment Dedicated lab space Shaker tables Ultrasonic baths Frantz magnetic separator HFrated fume cupboard with scrubber Scales Ovens Preparation of 10 Be, 26 Al and 36 Cl targets 2xDedicated clean labs 3xHF/Perchloric acidrated fume cupboards and scrubbers Laminar flow fume cupboard Ultrapure water system Scales Press Ovens What can be analysed? Most nuclides are measured from within quartz minerals. Therefore, any quartzrich rock or sediment can be analysed. However, chlorine can be measured in nearly any rock, and is particularly useful for carbonate rocks such as limestone. We have a fulltime laboratory technician, post docs and PhD students associated with the lab. Charges are set for analyses to recover costs through a model recognised by UK Research Councils. We offer a reduced rate for PhD research projects. If you are considering a project that would involve cosmogenic nuclide analysis, please speak to us! Contact: Dr. Andrew Hein 6 FURTHER INFORMATION Targetnucleus 16 O 10 Be 10 Be ~98% production 16 O(n,4p3n) 10 Be 28 Si(n,6p3n)2 10 Be 26 Al ~98% production 28 Si(n,p2n) 26 Al Fig. 1. Cosmogenic nuclide production occurs in near surface rocks, mainly through spallation reactions (left diagram): a fast incoming particle hits the nucleus of an atom. Nucleons (protons and neutrons) are sputtered off leaving a lighter residual nucleus behind. Spallation reaction Sample Crush Mill and sieve Acid etch 10 Be concentration! 26 Al concentration! 36 Cl concentration! Crush Chemical isolation and purification of 10 Be, 26 Al AMS target • isolate target mineral • remove meteoric variety 4 THE PROCESS Figure 3. A) Cosmogenic 10 Be dating of glacial erratics to contrain the timing of thinning of the Antarctic Ice Sheet. B) Use of multiple cosmogenic nuclides ( 26 Al, 10 Be and 21 Ne) can give insight on the exposure history; it is possible to determine if a rock has been continuously exposed, or if it has been buried for a significant period of time. C) We have used this information to constrain the history of the West Antarctic Ice Sheet (Hein et al., 2016a, 2016b). C B A Figure 3. Cosmogenic nuclides can be used to constrain basinwide erosion rates. In this case, providing data that can be used to constrain land surface erosion models (Hurst et al., 2013). A B Figure 2. A) Cosmogenic nuclide depth profiles can add valuable information on the age, erosion rate and inheritance. Here a 10 Be depth profile is use to constrain the age of a glacial outwash terrace. B) Modelling can then be used to optimise the best fit to the data (Hein et al., 2009). [email protected] School of GeoScienc es

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Page 1: School of GeoSciences - University of EdinburghFigure 2. A) Cosmogenic nuclide depth profiles can add valuable information on the age, erosion rate and inheritance. Here a 10Be depth

Cosmogenic nuclide concentrations are commonly used to determine ‘exposure ages’ and ‘erosion rates’.  Some common examples include:

Exposure dating• Glacier erosion/deposition surfaces: striated bedrock, erratics, moraines• Fluvial and glaciofluvial terraces• Buried sediments: caves, glacial till• Rockfalls• Fault scarps• Lava flows• Flood deposits• Alluvial fans

Rates of landscape change• Rock surface erosion rates• Land surface degradation rates• Basin‐wide erosion rates• River incision rates• Modern erosion (meteoric 10Be)• Fault‐slip rates

1 INTRODUCTION 5 APPLICATIONS3 CAPABILITIES

2 FACILITY DESCRIPTION

Terrestrial cosmogenic nuclides form inrock minerals exposed in the upper ~2 mof Earth’s surface through interactionwith cosmic radiation (Fig. 1). Theconcentration of cosmogenic nuclides innear surface rocks will increase throughtime until their production is matched bytheir losses through physical erosion andradioactive decay. Thus, theconcentration of cosmogenic nuclides inrock or sediment is a balance betweenits exposure time and erosion rate. Thisknowledge can be applied in a range ofsettings to quantify dates and rates ofEarth surface processes.

This facility is designed to makepossible the measurement ofcosmogenic nuclides in rock andsediment. Here, we chemicallyextract cosmogenic isotopes fromrock and sediment and preparetargets ready for measurement byAccelerator Mass Spectrometry(AMS). We are able to supportpreparation work for all of the majorcosmogenic isotopes includingcosmogenic 10Be, 26Al, 36Cl, 21Ne, 3Heand 14C. The AMS or MS analysesare conducted at the ScottishUniversities Environment ResearchCentre or other collaborativeinstitutions.

Rock crushing and sieving‐Dedicated lab space‐Disk mill‐Sieves‐Frantz magnetic separator‐Sample splitter

Extraction of quartz from rock/sediment‐Dedicated lab space‐Shaker tables‐Ultrasonic baths‐Frantz magnetic separator‐HF‐rated fume cupboard with scrubber‐Scales‐Ovens

Preparation of 10Be, 26Al and 36Cl targets‐2xDedicated clean labs‐3xHF/Perchloric acid‐rated fume cupboards and scrubbers‐Laminar flow fume cupboard‐Ultrapure water system‐Scales‐Press‐Ovens

What can be analysed?Most nuclides are measured fromwithin quartz minerals. Therefore, anyquartz‐rich rock or sediment can beanalysed. However, chlorine can bemeasured in nearly any rock, and isparticularly useful for carbonate rockssuch as limestone.

We have a full‐time laboratory technician, post docs and PhD students associatedwith the lab. Charges are set for analyses to recover costs through a modelrecognised by UK Research Councils. We offer a reduced rate for PhD researchprojects. If you are considering a project that would involve cosmogenic nuclideanalysis, please speak to us!

Contact: Dr. Andrew Hein

6 FURTHER INFORMATION

‘Target’ nucleus16O

10Be

10Be ~98% production16O(n,4p3n)10Be28Si(n,6p3n)210Be

26Al ~98% production28Si(n,p2n)26Al

Fig. 1. Cosmogenic nuclide production occurs in nearsurface rocks, mainly through spallation reactions (leftdiagram): a fast incoming particle hits the nucleus of anatom. Nucleons (protons and neutrons) are sputteredoff leaving a lighter residual nucleus behind.Spallation reaction

SampleCrush

Mill and sieve Acid etch

10Be concentration!26Al concentration!36Cl concentration!

Crush

Chemical isolation and purification of 10Be, 26Al

AMS target

• isolate target mineral• remove meteoric variety

4 THE PROCESS

Figure 3. A) Cosmogenic 10Be dating of glacial erratics tocontrain the timing of thinning of the Antarctic Ice Sheet. B)Use of multiple cosmogenic nuclides (26Al, 10Be and 21Ne)can give insight on the exposure history; it is possible todetermine if a rock has been continuously exposed, or if ithas been buried for a significant period of time. C) We haveused this information to constrain the history of the WestAntarctic Ice Sheet (Hein et al., 2016a, 2016b).

C

B

A

Figure 3. Cosmogenic nuclides can be used to constrainbasin‐wide erosion rates. In this case, providing data thatcan be used to constrain land surface erosion models (Hurstet al., 2013).

A B

Figure 2. A) Cosmogenic nuclide depth profiles canadd valuable information on the age, erosion rateand inheritance. Here a 10Be depth profile is use toconstrain the age of a glacial outwash terrace. B)Modelling can then be used to optimise the best fitto the data (Hein et al., 2009).

[email protected]

School of GeoSciences