Cosmogenic Nuclide Laboratory

The facility supports in-house research, as well as academic and external services in preparing samples for the measurement of terrestrial cosmogenic nuclides within rock and sediment.

Terrestrial cosmogenic nuclides form in rock minerals exposed in the upper ~2 m of Earth’s surface through interaction with cosmic radiation. 

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.

Female scientist wearing lab coat and gloves holding up a dropper in an aluminium beryllium laboratory

Cosmogenic nuclide concentrations are commonly used to determine:

  • ‘exposure ages’ such as glacier erosion surfaces, lava flows, buried sediments, landslide deposits and flood deposits and fault-slip surfaces
  • ‘erosion rates’ such as rock surface erosion rates, land surface degradation rates and river incision rates

This facility is designed to make possible the measurement of terrestrial cosmogenic nuclides within rock and sediment. Here, we chemically extract cosmogenic isotopes from rock and sediment and prepare targets ready for measurement by Accelerator Mass Spectrometry (AMS) or Mass Spectrometry (MS). We are set up to extract all of the commonly-used cosmogenic isotopes.

The AMS or MS analyses are conducted at the Scottish Universities Environment Research Centre (SUERC) or other collaborative institutions.

Information about our facility, and the process and applications for analysis are included in our poster available for download:

Laboratories and equipment

Our facility has several purpose-built laboratories, which were refurbished in 2016. Find out more about our range of facilities and equipment.

Our facility can chemically extract cosmogenic isotopes from rock and sediment and prepare targets ready for measurement by Accelerator Mass Spectrometry (AMS) or Mass Spectrometry (MS). 

We are able to support preparation work for all of the major cosmogenic isotopes including cosmogenic 10Be, 26Al, 36Cl, 21Ne, 3He and 14C. 

A female scientist wearing lab coat and gloves dripping chemicals into a column of analysis receptacles for anion analysis

What can be analysed? 

Most nuclides are measured from within quartz minerals (10Be, 26Al, 21Ne, 14C). Therefore, any quartz-rich rock or sediment can be analysed. 3He is often measured within individual olivine crystals, while 36Cl can be measured in nearly any rock, making it particularly useful for carbonate rocks such as limestone. 

We have preparation equipment that allows us to crush, sieve, and acid etch bulk rock to extract the mineral and size fraction required for analysis. We have clean laboratories and equipment that allow us to extract and purify the cosmogenic isotope of interest.

Capabilities

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 

  • Two dedicated clean labs 
  • Three HF/Perchloric acid‐rated fume cupboards and scrubbers 
  • Laminar flow fume cupboard 
  • Ultrapure water system 
  • Scales 
  • Press 
  • Ovens

Facilities

The Cosmogenic Nuclide Laboratory has:

  • Two clean rooms with filtered air and positive pressure
  • Two fume cupboards with wash-down facilities rated for HF and HClO 4
  • Four large volume ultrasonic baths for acid etching of quartz
  • Two orbital shaker table
  • Two centrifuge
  • Two analytical balances
  • Bench-top rock crusher
  • Recirculating fume cupboard for use with cation and anion exchange columns
  • Mineral separation lab with magnetic separator, sieve sets, and facilities for heavy mineral separations using non-toxic polylithium tungstate compounds

Our laboratories

The rock crushing and sieving laboratory reduces rock fragments into sand-sized particles using a Fritsch Disk Mill.  

The crushed rock is sieved to obtain the desired grain size for cosmogenic nuclide analysis or other purposes. We also have a Frantz magnetic separator that allows separation of ferromagnetic, paramagnetic and diamagnetic minerals, which is often used in the first stage of mineral isolation.  

The lab contains a rotating sample splitter with glass recovery bottles, which is used to obtain equal and representative splits of sand samples necessary for 36Cl analysis.


geos-facilities-underpinning- geography rock crushing 1

The geochemistry laboratory is where we undertake acid etching and isolation of target minerals. Most of the work we do involves isolating quartz or feldspar from a variety of rock types.  Samples undergo repeated etching in hexafluorosilicic acid H2[SiF6] on a shaker table to weaken silicate minerals. 

Repeated etching by ultrasonic heating and agitation in a dilute aqueous HF and HNO3 solution is then used to preferentially dissolve non-quartz minerals and to partially dissolve quartz grains to remove meteoric 10Be. The end result is ultrapure (<200 ppm Al) quartz separates that are free from meteoric 10Be. The lab is fitted with 18.2 M-ohm deionised water, HF-rated fume cupboard with scrubber, ultrasonic baths, shaker tables, acid neutralisation facilities, scales, ovens and microscopes.


The clean laboratory is where wet chemistry to isolate and purify 26Al and 10Be occurs. Samples are dissolved and passed through anion-exchange chromatography columns to remove Fe, and subsequently through cation exchange columns to remove Ti and B, and to split the Al and Be fractions. The Al and Be fractions are then precipitated as hydroxides and then oxidised in a furnace oven.  The BeO and Al2O2 are mixed with Nb and Ag metals, respectively, and pressed in copper cathodes ready for AMS analysis. The lab is fitted with filtered air and ultrapure 18.2 M-ohm deionised water. It contains 2xHF and Perchloric acid-rated fume cupboards with scrubbers, a laminar flow fume cupboard, a centrifuge, scales, a furnace and a press.


This dedicated clean laboratory is where we undertake chemistry to isolate and purify 36Cl. We are set up to work with both carbonates and silicates. The samples are dissolved, and AgCl is precipitated with the addition of AgNO3.  Sulphates are removed with the addition of Ba(NO3)2, and the final AgCl is purified and dried in an oven, then pressed with an AgBr substrate in a copper cathode ready for AMS analysis. The lab is fitted with red-lights, filtered air, and ultrapure 18.2 M-ohm deionised water. The lab contains an HF-rated fume cupboard, centrifuge, refrigerator, ovens, scales, and shaker tables.


There are also various facilities available at our Kings Building's campus, which is about 2 miles from our laboratory.

These include:

  • X-Ray Diffraction Facility
  • X-Ray Fluoresence Facility
  • NERC Ion Micro-Probe Facility
  • Electron Probe Microanalysis Facility
  • Scanning Electron Microscope Facility 

Applications

Find out about applications for cosmogenic nuclide concentrations. For example, cosmogenic nuclide concentrations are commonly used to determine ‘exposure ages’ and ‘erosion rates’.

Some common examples include:

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

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

Contact information

For more information or to access our services, please contact: 

Dr Andy Hein  Senior Lecturer/ Laboratory  Manager

Location:

The Cosmogenic Nuclide Laboratory is in the Institute of Geography, University of Edinburgh.  The Institute is located in central Edinburgh, within the historic Old Town and close to Old College.

Address:  Institute of Geography, School of GeoSciences, University of Edinburgh, 1 Drummond St, Edinburgh EH8 9XP

Additional facilities are located at our Kings Buildings campus, which is around two miles (3km) north of Edinburgh city centre.


The Cosmogenic Nuclide Laboratory is available for use by:

  • Students and staff at the University of Edinburgh ​
  • Students and staff from other universities
  • Other external users such as research bodies or commercial organisations

We have a full‐time laboratory technician, postdoctoral researchers and PhD students associated with the laboratory. 

If you are considering a project that would involve cosmogenic nuclide analysis, please speak to us!

Important information

Availability
  • Access is subject to availability.
Costs
  • 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. 
  • Prices may vary depending on work involved. 
  • Prospective users should contact the facility to discuss requirements and costs involved. 
  • Staff and students within the School of GeoSciences must complete a technical request form.

For the wider University and all external users: 

  • Please contact the facility to discuss availability, as well as analytical requirements and charging information.  

For staff and students in the School of GeoSciences: 


Small Research Facility (SRF)

Our Cosmogenic Nuclide Laboratory is operated as a Small Research Facility (SRF).

A Small Research Facility (SRF) is a facility or service provided by the School and used for research and teaching.  They are also available for use by the wider community such as external academic or commercial use.  Our SRF's are available for hire or on a consultancy basis.  These charges are recognised by grant funders and can therefore form part of a grant submission.