Discipline of Geology hosts IGRM25.

When: 28th February to 2nd March 2025.

Where: Trinity College Dublin (Edmund Burke theatre and adjacent concourse)

How to attend: Please register for your ticket via Eventbrite. (For those wishing to present please fill out additional submission forms below by the extended deadline of 21st February.)

Discipline of Geology, Trinity College Dublin are delighted to be hosting this year's IGRM. The 68th Irish Geoscience Research Meeting 2025 (IGRM25) will take place in the Edmund Burke Theatre on Trinity's Main Campus. This 3-day weekend event will run from Friday 28th February to Sunday 2nd March 2025.

Your ticket will cover all 3 days of this event. Once you have registered for your ticket you are asked to complete the Additional Registration Form to confirm dietary requirements for refreshments and bookings for Ice-Breaker and Dinner, along with confirmation of any submissions.

It is an honour to host such a prestigious annual event, and we hope you will join us for this gathering. The format will be similar to previous years, with guest speakers on the Friday and Saturday evenings, and general sessions taking place over the weekend, finishing by 15.30 on Sunday 2nd March.

Registration, as always, is free. For information on travel and accommodation, please see www.visitdublin.com. Places book up quickly, so secure your accommodation early to avoid disappointment.

Presentations and Abstract submission

For those wishing to present at the meeting, please complete the Additional Registration Form.

Please submit your abstract via the following form(here). The deadline for submitting abstracts has been extended to 21st February.

Guest Speakers

Friday 28th February: 

Prof Gavin Foster, University of Southampton

Title: Past, Present and Future of Stable Isotopes in Palaeoclimate 

The measurement of the stable oxygen isotope composition of marine carbonates such as foraminifera has underpinned the study of ancient climates for over 75 years since Nobel laureate Harold Urey “…suddenly found [himself] with a geologic thermometer…” in 1948.  Since then, advances in mass spectrometry technologies, hand in hand with the establishment of deep ocean drilling, have not only led to foraminiferal oxygen isotopes becoming the workhorse of modern palaeoclimatology, but have also enabled us to describe the climate of the past 65 million years (and beyond) in exquisite detail.  Foraminiferal carbonates contain a number other major elements and impurities and it seems that as soon as methods are developed to measure the stable isotopic composition of these elements they are applied by ingenious palaeoclimatologists to study the climate of our past.  One element present in parts per million level in the shells of foraminifera that is proving particularly useful is boron, which has two stable isotopes 11B and 10B first measured in foraminifera in 1991.  It was quickly recognised that the ratio of 11B/10B in marine carbonates was a close function of the pH of the seawater in which the foraminifera lived.  Since surface water pH is in turn tightly related to the CO2 content of the atmosphere this gave palaeoclimatologist a means to reconstruct CO2 back in time – way beyond the reach of the gas bubbles trapped in Antarctic ice cores.  We now have a palaeo-CO2 record from boron isotopes in foraminifera stretching back 65 million years consisting of >700 analyses.  By marrying this CO2 record with climate records from oxygen isotopes and other methods, we have been able to not only test the climate models used to predict our changing future but can also constrain the sensitivity of natural climate change to CO2.  Both these provide vital constraints on the causes of past climate change and also help narrow the uncertainties in our projections of anthropogenic climate change.  Advances in mass spectrometry continue at pace and the determination of the boron isotopic composition of single foraminifera has become possible in the last couple of years using laser ablation methods.  This allows an unprecedented picture of ancient climate but is of course not without its challenges. 

 In this talk I will outline how we got to where we are today in terms of stable isotope geochemistry and conclude with presenting some of my groups latest research on single foraminiferal boron isotopes, showcasing a new way to study the climate of our past.

Saturday 1st March: 

Prof Frances Wall, University of Exeter

Title: Critical Rare Earths

Critical minerals are back at the top of the agenda, with talk of tariffs and trade wars and proposals to buy Greenland, as well as the concern about changes in the global dynamic, as the power of access to deposits of the minerals needed for all our green and digital technologies takes over from the geopolitical power that currently comes from fossil fuel resources.

Rare earths are always near the top of critical minerals lists. Their magnetic and luminescent properties make them essential components of digital and low carbon technologies but their supply is vulnerable to disruption because the whole value chain of mining, processing and manufacturing is dominated by China.

The rare earth elements (REE) comprise 17 elements that include scandium, yttrium and the 15 elements lanthanum through to lutetium. The name ‘rare earth’ was given by early chemists in reference to the difficulty in separation of the elements from each other – nothing to do with rare earths being scarce. The crustal abundance of light REE is about the same as copper and even the less abundant heavy REE are much more abundant than precious metals such as gold.

So, it should be easy to open up a few more mines and diversify supply outside of China, right? Well, history has proved this wrong. Since REE first hit the headlines in 2010, there is still only one new major REE miner outside of China. The geology, mineralogy and geochemistry of REE, combined with finance and geopolitical constraints have all conspired to slow down new REE production.

This talk considers the vital role that geologists, working with colleagues in minerals processing, responsible sourcing and finance, play in the REE story.

We will consider carbonatite-related deposits, that host most REE mines; alkaline rocks, like those that occur in large deposits in Greenland but have mineralogical challenges; ion adsorption clays that are a responsible sourcing disaster story in China and Myanmar but might prove a viable source of REE elsewhere; and mineral sands that can produce monazite as a by-product. The talk will review the many studies have sought to produce REE as by-products of other mines, ranging from coal, to bauxite and phosphate but none have yet come to fruition. The last deposit type for geologists to consider is the urban mine, our anthropogenic REE deposits that are in products all around us.

 

Conference Meals

Please note that lunch is not included as part of this event, however there are many options within walking distance of the event venue.

There will be a conference dinner held on the Saturday evening in the Harbourmaster.

Cost will be €65 per person. If you would like to attend the meal, please book this in via the Additional Registration Form. Payment will be taken upon arrival at the Registration desk.

 

Organising Committee

David Chew, Quentin Crowley, Gerald Dickens, Chris Nicholas, Emma Tomlinson.

The 68th IGRM has been organised by:

Discipline of Geology, Trinity College Dublin, The University of Dublin.

 

 

 

 

 

Our Sponsors

The 68th IGRM is supported by:

             

 

 

 

     

       

 

 

 

 

 

 

 

Contact:

For further information or if you have any queries, please contact IGRM@tcd.ie

IGRM Code of Conduct: IGRM Code of Conduct