Royal Society of NSW News & Events

Royal Society of NSW News & Events
JAN
01

Sydney Meetings - 2006

The venue for all meetings was, unless otherwise indicated, Conference Room 1, Darlington Centre, University of Sydney (City Road). Meetings commenced at 7 pm.

​Wednesday
22nd February

"A cradle-to-grave concept for Australia's uranium"

The Four Societies Meeting

Dr Clarence Hardy, Secretary ANA, Vice-President Pacific Nuclear Council.
​Friday
10th March

​The Royal Society of New South Wales Annual Dinner

Held at the Forum Restaurant, Darlington Centre, Sydney University

Dr Tim Entwisle, Executive Director of the Royal Botanic Gardens, was the guest speaker
​Friday
17th March

"Can the physicists' description of reality be considered complete?"

2006 Pollock Lecture

Prof. Brian Josephson FRS, Nobel Laureate
​Wednesday
5th April

​"Cold fusion, the alchemists' dream?"

Annual General Meeting and Presidential Address, Prof. Jak Kelly
​Wednesday
3rd May

​"The genetics behind our drinking water turning toxic"

Prof. Brett Neilan, School of Biotechniology and Biomolecular Sciences, University of NSW.
​Wednesday
7th June

"Global evolution of ocean basins"

A/Prof. Dietmar Muller, School of Geosciences, University of Sydney
​Wednesday
5th July

"Asian honey bees: biology, conservation and human interactions"

A/Prof. Ben Oldroyd, School of Biological Sciences, Sydney University
​Wednesday
2nd August

"The overshadowed centenary - the discovery of the pinch effect in 1905"

A/Prof. Brian James, School of Physics, Sydney University.
​Wednesday
6th September

"The frontier of measurement: leading-edge standards for length and time"

Bruce Warrington, Head of Time and Frequency, National Measurement Institute
​Wednesday
4th October

"Pandemics, bird flu and the globalisation of fear"

Prof. Peter Curson, Director Health Studies Program, Macquarie University.
​Wednesday
1st November

"The cervical cancer vaccine"

Prof. Ian Frazer, Director of the Centre for Immunology and Cancer Research, University of
Queensland and Princess Alexandra Hospital, Brisbane, and 2006 Australian of the Year
AUG
06

1173rd Ordinary General Meeting

"What will coral reefs look like in 2050?"

Associate Professor Peter Ralph, Executive Director, Plant Functional Biology and Climate Change Cluster (C3), University of Technology, Sydney

Wednesday 5 August 2009 at 7 pm
Conference Room 1, Darlington Centre, University of Sydney

Corals have existed for millions of years and survived in a wide range of climates; but coral bleaching seems to have pushed corals to the brink. Research in to coral bleaching has been at the forefront of the climate change agenda for many years. It attracts much public interest, but we still do not know why corals die at temperatures only a few degrees higher than their optimum. Given the onset of coral bleaching and the combined stress of ocean acidification, I will describe how I see the Great Barrier Reef in 2050. Will the reef be dominated by fleshy macroalgae, soft corals or just a film of bacteria covering the dead coral skeletons?

The speaker's presentation can be found here: Peter Ralph Talk (36 MB PDF).

Peter Ralph is an Associate Professor at UTS and the Executive Director of the Plant Functional Biology and Climate Change Cluster (C3). He has over 15 years experience in the areas of photosynthetic physiology and ecology of marine plants and is widely regarded as a world expert in this field. His research team has made significant contributions to the physiology of marine plants, including corals, Antarctic sea-ice algae, seagrasses and macroalgae. His group includes senior research fellows, 3 post docs, 7 PhD students and 4 Honours. His team has on-going research collaborations with Danish, German, UK, US and Canadian photobiologists. Peter has been addressing questions fundamental to advancing knowledge of marine photosynthetic organisms that survive at the edge of their environmental envelope. His group is currently developing mechanistic models of microalgal photo-physiology, as well as developing a fluorescence-based proxy of primary production.
JUL
02

1172nd Ordinary General Meeting

"Accurate measurement: the vital backbone of Australian science & industry"

Dr Laurie Besley, Chief Executive & Chief Metrologist, National Measurement Institute

Wednesday 1 July 2009 at 7 pm
Conference Room 1, Darlington Centre, University of Sydney

Measurement pervades all aspects of our society, from the sale of food by weight in the supermarket, to the management of data transfer systems to better than nanosecond precision for the telecommunications sector. The National Measurement Institute (NMI) is the national core of Australia's expertise in measurement and has the responsibility to address this entire spectrum of needs. It not only maintains, develops and disseminates the primary measurement standards for Australia in physics, chemistry and biology, but also operates specialist laboratories based on these measurement skills, such as a mainstream forensic laboratory, Australia's only WADA-accredited sports drugs laboratory, and a high-voltage laboratory for the electrical utilities. The talk will discuss how NMI addresses this myriad of challenges and outline the outcomes to Australia from its activities.

Dr Besley's scientific and management career has spanned a diversity of fields. including, for the last dozen years, metrology in chemistry. After beginning his career in cryogenic temperature measurement and spending 20 years working in physical metrology, he applied his PhD in chemistry to transplanting the metrological approach from physics to chemistry and initiated work in this area within what was then the National Measurement Laboratory (NML) in Australia. He then became Director of the National Analytical Reference Laboratory within the Australian government body AGAL. When AGAL and NML both became part of the new organisation NMI in 2004, he was first appointed to a role as general manager of the metrology in chemistry branch and late in 2007 was given his present role as Chief Executive. Dr Besley has a publication list of some 75 journal publications in a variety of different fields of metrology.

Dr Besley is a member of the Royal Australian Chemical Institute and a Fellow of the Institute of Physics (UK). He is also a member of the NATA Council. He is active in a number of international forums including being a consultant to the Executive Committee of the Asia-Pacific Metrology Programme. He is a member of the editorial boards of the international journals "Metrologia", "IET Science Measurement & Technology", and "Accreditation and Quality Assurance". He has worked on a number of occasions as a consultant for the Technical Cooperation programme of the German metrology institute (PTB), mostly in Thailand, and most recently in Sri Lanka.


JUN
04

1171st Ordinary General Meeting

"New environmentally friendly approaches to cooling buildings"

Professor Geoff Smith, Department of Physics and Advanced Materials, University of Technology, Sydney

Wednesday 3 June 2009 at 7 pm
Conference Room 1, Darlington Centre, University of Sydney

The potential for energy savings in the cooling of buildings is very large and of growing importance as living standards rise, as global warming impacts, and as the "heat island" effect gets worse with increased urbanisation. There are two aspects: (i) passive systems which minimise heat gains, and (ii) active systems and strategies which minimise or eliminate the need for electrically powered cooling. This talk will examine novel materials and systems which play a role in both active and passive reductions in the demand for electrically powered cooling. It will also include results with special paints and nanostructured coatings developed at UTS.

Amplification of night sky radiative cooling using nanostructures and heat mirrors will be outlined, in which material spectral properties and system design in combination optimally exploit the spectral and directional properties of incoming atmospheric thermal radiation. Useful cooling powers under clear skies at temperatures down to ~15℃ below ambient are feasible in well engineered systems, while simple low cost systems can achieve useful cooling powers in the range 5℃ to 10℃ below ambient. There are a many ways such capabilities can be put to use.

The speaker's presentation can be found here: Geoff Smith's Talk (4.6 MB PDF).

Geoff Smith is Professor Emeritus in Applied Physics at the University of Technology, Sydney Australia. He has worked on the science and applications of nanomaterials for over 30 years. His group, in partnership with local and international industry, has pioneered developments in the fields of solar energy, energy efficient windows and paints, radiative cooling, natural lighting and LED lighting. Products and several patents have followed. Key contributions to nano-photonics, thin film optics and polymer optics feature in his work with over 180 reviewed papers and several book chapters. He is chair of the Australian Standards committee on roof glazing and skylights, helped formulate Australia's recent energy efficient building codes, and has chaired an annual International Conference in the USA (SPIE - Nanostructured Thin Films) since 2006. Geoff has a number of overseas and local awards in the renewables and energy field including an honorary doctorate from the University of Uppsala in Sweden in 2003. He is a Fellow of the AIP and of the Institute of Energy.

A summary of the July lecture by Dr Jim Franklin

There is a hole in the atmosphere that can be used to cool buildings. This is important because the electricity used for air-conditioning is a major contributor to greenhouse gas emissions and building running costs. Professor Geoff Smith from UTS explained that at wavelengths below 8 micrometers, the atmosphere is opaque because of absorption from water vapour. Above 13 micrometres it is opaque because of absorption from carbon dioxide and water vapour. So for long and short wavelengths we see a hot opaque atmosphere and no radiative cooling is possible.

However, between 8 and 13 micrometers the atmosphere is fairly transparent (opacity is 17 % at the vertical, increasing to 100 % at the horizon). So at this "wavelength hole", an object can radiate its heat away through the atmosphere into space and receive little heat back from the atmosphere. The cooling effect is greatest towards the vertical. Professor Smith has shown that net-cooling powers can in principle exceed 200 W/m2. Experimental systems developed by his group can run 10°C below ambient at night and pump 135 W/m2. Or they can achieve much lower temperatures with smaller cooling powers. The key is to use an optical design in which the radiator only sees the "cool" sky at the zenith. If these systems are shielded from the direct sun, they can also give good cooling during the day. Prof Smith has investigated special selective surfaces that radiate most efficiently in the "wavelength hole" with little emission at other wavelengths. Surprisingly, these selective surfaces offer little advantage, except when one is striving for the lowest possible temperature.

Professor Smith then discussed new building materials he has worked on that can help cool buildings. With BASF and others he has helped develop special paints that reflect the infrared part of sunlight but look like ordinary pigments to the naked eye. A special white paint developed by UTS can greatly decrease solar heating. When tested on a Queensland supermarket it cut air-conditioning power consumption by two thirds.

Another interesting material described by Prof Smith is Micronal sheeting (made by BASF). This is plasterboard with a high loading of microcapsules of an alkane wax that changes phase at room temperature. This gives the material superb heat storage capabilities. A 3 cm sheet has the same heat capacity as 18 cm of concrete or 23 cm of brick. A building using this material can have enhanced comfort and reduced costs with minimal air conditioning or heating. In summer one lets in the cold night air to chill the sheets, and then uses them to cool the building during the hot part of the day. In winter, the noon sun warms the sheets, which can heat the building at night. Clearly radiative cooling and new, high tech materials have an important future in cooling buildings.

MAY
07

1170th Ordinary General Meeting

"A scientist vs. the law"

Professor D. Brynn Hibbert
Chair of Analytical Chemistry, University of New South Wales

Wednesday 6 May 2009 at 7 pm
Conference Room 1, Darlington Centre, University of Sydney

A largely anecdotal review of the author's work in the courts, including bogus health products, unsuccessful defences of murderers and racehorse trainers, and highly lucrative patent cases.

One example is Ion mobility spectrometry. This is embodied in instruments such as the Ion Scan and is used at airports to detect drugs or explosives at trace levels. The author has given evidence in trials of drug importation in which an Ion Scan has revealed the presence of a drug with subsequent seizure of substantive amounts. In an early trial, during the author's evidence the "invisible hand" defence was coined when the trial judge misheard a question from counsel and caused the following conversation. Judge: "Did you say the hand that touched the cocaine was invisible?". Counsel: "No your honour, I said the cocaine that the hand touched was invisible".

The Ion Mat sold for around $3,000 and apart from claiming to improve your sex life, it cured cancers (various) and ameliorated bad breath. The mattress did this by creating "beneficial negative ions" despite the author's opinion that the electric field was about the same as a toaster and whereas we do not expect our household appliances to make us better, this would not either. The prosecution by the ACCC was a success, but at the end of the trial the principals of the company fled with, it is said, $12 million.

There will be some discussion of statistics (Lies, damned lies and ...), dendrites and fractals, stolen wine, contaminated beer and defunct batteries. This will lead to a reflection on expert opinion and the role of professional societies in maintaining standards of professionalism.

The speaker's presentation can be found here: Bryn Hibbert's Talk (1.3 MB PDF).

Professor Hibbert occupies the Chair of Analytical Chemistry at the University of New South Wales in Sydney. He is the second incumbent and arrived in Australia from England in 1987. His research interests are in electroanalytical chemistry and chemometrics and metrology in chemistry, but he also does a sideline in expert opinion, scientific fraud and presenting science to the public. He has published around 200 papers, 6 books and 2 patents. His most recent book Quality Assurance in the Analytical Chemistry Laboratory published by Oxford University Press won the RACI Olle Prize for 2007. He is past Chair of the Analytical Division of the RACI, Secretary of the IUPAC Analytical Division and was co-chair of Interact 2002.

APR
30

Pollock Memorial Lecture 2009

"The universe from beginning to end"

Dr Brian Schmidt, Federation Fellow, Mount Stromlo Observatory, ANU

Wednesday 29 April 2009 at 6.30 pm
Eastern Avenue Auditorium, University of Sydney

The Pollock Memorial Lecture is presented jointly by the University of Sydney and the Royal Society of NSW. The Lectureship has been awarded about every four years since 1949 and is sponsored by the University of Sydney and the Royal Society of NSW in memory of Professor J.A. Pollock, Professor of Physics at the University of Sydney (1899-1922) and a member of the Society for 35 years.

Despite hundreds of years of dedicated scientific research, we only know what 4% of the Universe is made up of. In the last 15 years we have realised that there is another 96% of missing stuff that we just can't see. This missing stuff is made up of two mysterious substances, Dark Matter and Dark Energy, that are battling for domination of the Universe.

In the Pollock Memorial Lecture, Professor Brian Schmidt, from the Australian National University, will describe exciting new experiments, including those using the SkyMapper telescope, that are monitoring the struggle between these two dark forms. The aim is to predict the ultimate fate of the Cosmos!

Professor Brian Schmidt is a Federation Fellow at the Australian National University's Mount Stromlo Observatory. While at Harvard University in 1994 he formed the High Z SN Search team, a group of 20 astronomers on five continents who used distant exploding stars to trace the expansion of the Universe back in time. This group's discovery of an accelerating Universe was named Science Magazine's Breakthrough of the Year for 1998. Brian is continuing his work using exploding stars to study the Universe, and is leading Mt Stromlo's effort to build the SkyMapper telescope, a new facility that will provide a comprehensive digital map of the southern sky from ultraviolet to near infrared wavelengths.

FEB
26

The Four Societies Lecture 2009

Australian Nuclear Association, Nuclear Panel of Engineers Australia, Australian Institute of Energy and The Royal Society of NSW

"An industry update on global nuclear power and the opportunities for Australia"

Dr Selena Ng, Areva NC, Australia

Wednesday 25 February 2009 at 6 pm
Engineers Australia Lecture Theatre, 8 Thomas St, Chatswood

Countries world-wide are committing to nuclear power as an integral part of their future energy mix, as they struggle to meet increasing electricity demands in a competitive and secure way while reducing their carbon emissions. Here in Australia, nuclear power, uranium mining, nuclear weapons, and radioactive waste - just to name a few - do make appearances on the public and political agenda from time to time, although the issues are sometimes confused, and often clouded by conflicting 'facts'. This talk will aim to set the record straight from an industry perspective, covering some of the long-argued topics such as proliferation, safety, and waste. It will also look at projected industrial developments over the coming decades, and the opportunities for Australia to get involved.

Dr Selena Ng is currently responsible for developing AREVA's nuclear activities in Australia. Prior to returning to Australia in 2007, she spent a number of years at AREVA's headquarters in Paris, dealing with the recycling of used nuclear fuel and waste management, and issues such as nuclear non-proliferation, a topic about which she has co-authored and presented papers at various international forums. Selena holds a BSc(Hons) from Monash University, a PhD in theoretical physics from the University of Cambridge, and a diploma in management from the College des Ingenieurs.

JAN
28

Sydney Meetings - 2005

​Wednesday
2nd February

Rev. W. B. Clarke - 19th Century Polymath and his Scientific Correspondence

Dr Ann Moyal AM

Time: 7.00 pm
Venue: Conference Room 1, Darlington Centre.

Dr Moyal will speak on the topic of her book that was recently launched at the State Library: The Scientific Correspondence of the Rev. W B Clarke, Australia's Pioneer Geologist. As most members will also be aware, The Rev. W.B. Clarke was an early founding member of the Society and served as inaugural and an influential Vice President for seven years.
​Wednesday
23rd February

​Four Societies Meeting: Geothermal Energy in Australia

Dr Doone Wyborn

The Four Societies Meeting is a meeting of the Nuclear Engineering Panel of Engineers Australia, Australian Institute of Energy, Australian Nuclear Association and
the Royal Society of NSW.

Time: 7.00 pm
Venue: Harricks Auditorium, Ground Floor, Eagle House, 118 Alfred Street, Milsons Point.

This year the Four Societies Meeting will be separate from our February 1132nd General Meeting above and will be hosted by Engineers Australia. Dr Doone Wyborn, Executive Director, Geodynamics has agreed to be the Guest Speaker on the topic of Geothermal Energy in Australia. Geodynamics have drilled one well in the Cooper Basin of South Australia to a depth of 4.5 km, intersecting rock in excess of 240C, and have a second well underway. They expect to start production in 2006.
​Wednesday
11th March

​The Royal Society of New South Wales Annual Dinner

Time: 7.00 for 7.30 pm
Venue: Forum Restaurant, Darlington Centre, Sydney University (City Road)

The Society's Patron, His Excellency, Major General Michael Jeffery AC CVO MC (ret'd), Governor-General of the Commonwealth of Australia, presented the 2004 Awards.
​Wednesday
6th April

A Hundred Years after Einstein's Extraordinary Year

The Annual General Meeting and the 1133rd Ordinary General Meeting

The President, Ms Karina Kelly, will deliver the Presidential Address

Time: 7.00 pm
Venue: Conference Room 1, Darlington Centre, City Road
​Wednesday
4th May

Biocosmology: a New Science

Dr Charley Lineweaver, Senior Fellow Planetary Science Institute, Australian National University

Time: 7.00 pm (bar open from 6.00 pm)
Venue: Conference Room 1, Darlington Centre, City Road
​Wednesday
1st June

Bactrian Camels in Antiquity

Prof. Dan Potts,
Edwin Cuthbert Hall Professor of Middle Eastern Archaeology, University of Sydney

Time: 7.00 pm
Venue: Conference Room 1, Darlington Centre, City Road
​Wednesday
6th July

Why did the Vertebrate Brain Become Lateralised?

Professor Lesley Rogers, Professor of Neuroscience and Animal Behaviour, University of New England

Time: 7.00 pm
Venue: Conference Room 1, Darlington Centre, City Road
​Wednesday
3rd August

Tails of Dingoes: their Past and their Future

Dr Alan Wilton,
School of Biotechnology and Biomolecular Sciences, University of NSW

Time: 7.00 pm
Venue: Conference Room 1, Darlington Centre, City Road
​Wednesday
7th September

​Clarke Memorial Lecture and 1138th Ordinary General Meeting

The Ediacara and its Fauna

Professor Pat Vickers-Rich, School of Geosciences, Monash University

Time: 6.00 pm
Venue: Conference Room 1, Darlington Centre, City Road
​Wednesday
5th October

TB: A New Vaccine and Some Observations on the Influence of Genetics

Professor Warwick Britton, Head, Mycobacterial Research Group, Centenary Institute of Cancer Medicine and Cell Biology, University of Sydney

Time: 6.00 pm
Venue: Conference Room 1, Darlington Centre, City Road
​Wednesday
2nd November

The Role of DNA studies in the Story of Human Evolution

Dr Sheila van Holst Pellekaan,
Visiting Senior Research Fellow, University of NSW

Time: 6.00 pm
Venue: Conference Room 1, Darlington Centre, City Road
MAR
08

The Four Societies Lecture 2012

Lecture delivered at the annual meeting of the Royal Society of NSW, the Australian Nuclear Association, the Nuclear Panel of Engineers Australia, and the Australian Institute of Energy.

"Counting atoms for a living"

Dr Andrew Smith, ANSTO

Wednesday 7 March 2012 at 6 pm

Hamilton Room, Trade & Investment Centre, Industry & Investment NSW, Level 47, MLC Centre, 19 Martin Place, Sydney

Meeting report by Donald Hector

Andrew Smith counts cosmogenic radionucleides for a living! These are radioactive cosmic rays (or, more accurately, cosmic particles) most of which are generated in the Sun and the far reaches of the universe. The facilities at ANSTO users accelerator mass spectrometry (AMS) which is an assembly of tandem accelerators to detect rare isotopes of intermediate half-life.

Cosmic rays were discovered in 1904. They are energetic particles that impinge upon the Earth's atmosphere – about 90% are protons, 10% are helium nuclei (alpha particles) and less than 1% are heavier" nuclei. They are generated by the Sun, supernova and what astronomers refer to as "unknown events". When these particles hit the Earth's atmosphere and collide with other molecules, the products of these collisions can be observed and measured.

One of the applications of this technology is in carbon-dating. Carbon-dating technology relies on the fact that the atmospheric concentration of the 14C, the radioactive isotope of carbon, is constant with about 7.5 kg being produced in the atmosphere every year. While an organism is alive, it is in equilibrium of the atmosphere. When it dies the "clock" starts because 14C update ceases and radioactive decay gradually reduces the 14C concentration. The older technology is radiometry which is a passive technique that requires a relatively large sample (up to several grams) but using AMS (the ANSTO equipment uses the 2 MV STAR accelerator) is an "active" only requires a much smaller sample of around 0.1 mg.

One area of particular interest for Dr Smith and his team is using is highly sensitive analytical technique to examine the polar sheet in Antarctica. As it falls, snow traps atmospheric gas and particles and once the ice has accumulated to it thickness of 50-100 m, the air pockets are closed off, trapping the gas. To investigate theories relating to climate change, establishing historical concentrations of greenhouse gases is of particular interest. Carbon dioxide, methane and nitrous oxide (these three constitute only about 0.1% of the atmosphere) are trapped in the bubbles in the ice. Both natural sources of methane (termites, geologically produced methane, clathrates – these are methane molecules trapped in a cage of water molecules due to very high pressure and are found extensively in deep parts of the ocean – and anaerobic decay) and anthropogenic sources (landfills, livestock, rice cultivation, and waste water treatment) each has its own unique signature of carbon isotopes.

The experimental work being done in ANSTO over the last several years has been drilling down to extract cores from ice which has been deposited over several thousand years. Large quantities of ice are needed to get even the tiny samples needed for analysis (Dr Smith's recent expedition to the area near Casey base collected 7½ tons of ice). Once the samples go through a very careful preparation process and are analysed (including corrections for cosmic ray generation of 14C and the changes in 14C concentration caused by nuclear testing in the 1950s and 1960s when its concentration doubled) some very interesting information emerges. For example, historically there have been some very sharp changes in methane concentration. This could be due to clathrates releasing their methane in previous eras. If so, this indicate a major problem should global warming cause large methane releases either from clathrates or peat bogs as permafrost melts.

Another area of investigation that ANSTO is pursuing is whether there is a connection between sunspot activity and climate change. Historical astronomical records suggest that during the Maunder minimum (a period that has been described as "a mini ice age" in Europe from about 1635 to 1700) sunspot activity was unusually low. The first step is to measure the ratio of 7Be to 10Be which is well correlated to sunspot activity. This investigation is very complex and will have some years to run while such issues as beryllium transfer through the ice sheet needs to be understood. Dr Smith's team is at the cutting-edge of climate change research and is just one example of ANSTO's unique contribution to world-leading science.

APR
05

The Royal Society of NSW Forum 2012

"The influence of media on scientific research"

Mark Scott AO, Managing Director of the ABC, and Professor Jill Trewhella FRSN, Deputy Vice-Chancellor (Research) at the University of Sydney

Wednesday 4 April 2012 at 6.30 pm

Powerhouse Museum, Ultimo

Meeting report by Donald Hector

The Society's second annual Forum was held on Wednesday 4 April at the Powerhouse Museum. The discussion was between Mark Scott AO, Managing Director of the ABC and Professor Jill Trewhella FRSN, Deputy Vice Chancellor, Research and Innovation at Sydney University. The topic of the discussion was "The influence of media on scientific research". The forum was moderated by Robyn Williams AM of the ABC.

Mark pointed out that the role of national broadcasters (originally established to produce programmes that commercial companies could not or would not) has changed very significantly. The internet has made available thousands of TV and radio stations worldwide. The consumer is flooded with content. Gone are the days when listeners needed a licence – now all that is necessary is an internet connection. Nor are there barriers to entry for broadcasters. There are over 200 million web-sites worldwide and 60,000 blogs are introduced to the internet every day.

The role of the ABC is now even more important than it was formerly. It now provides a "town square" for content and opinion. It provides a broad plurality of views. Whereas the challenge for science is the narrowness of focus of much research is, the ABC provides a place where there is breadth not narrowness of interest. The gap between the ABC and content providers is growing every day due to the challenge facing commercial providers in delivering a profit in a rapidly changing media sector. The challenge for scientists is to become effective communicators and, particularly, to cultivate interest among journalists.

Jill said how important it was to have institutions like the ABC that produce quality content and encourage public education and debate. The key roles of the media are to educate, to inspire and to promote public discourse, particularly as the world faces critical issues, not least the state of the natural world.

Nonetheless it is regrettable that the media often confuse opinion, fact and belief. Too much of the current debate focuses on belief. But belief is not important in many issues – what is important are matters of fact. This is particularly significant in major issues such as health and climate change where scientific knowledge is important. For example, in health investment in research is generally seen as overwhelmingly good. And it probably is but what about the unavoidable trade-offs in research in other areas? It is also regrettable that advertising is a major influence on public opinion and political processes.

Robyn then moderated a discussion that included questions from the audience and covered such issues as the "priesthood status" of peer-review, the polarisation of public opinion, climate change, the state of critical argument in Australia and the necessity for the scientists to produce a compelling story in order to engage the media.

The Forum was broadcast on ABC Radio National's Big Ideas on Thursday 17 May 2012: click broadcast to download the programme.

NOV
27

2010 Liversidge Lecture in Chemistry

"Belief in science"

Professor John White CMG FAA FRS, Australian National University

Friday 26 November 2010 at 5.30 pm

Lecture Theatre 1, Merewether Building, University of Sydney

The achievements of science in the last 400 years have been of great benefit to humanity and are appreciated widely. Less well understood is how personal attributes of awareness, excitement, frustration and recognition of beauty are central to successful science. These very human qualities play a role in making discoveries. Scientists' optimism, suspended disbelief, and a reliance on empiricism are as much part of the scientific method as clear logic. Science requires absolute honesty and care about conclusions to be believable. Science is not autonomous and the sometimes necessarily tentative opinions are often incomprehensible and even unacceptable to the public – we must do better in explaining! Professor White's lecture will also examine some of his recent work on the structure and function of industrially valuable explosive emulsions – understood by the novel neutron scattering methods of 'contrast variation' pioneered in his research.

John White is currently Professor of Physical and Theoretical Chemistry at the Research School of Chemistry at the Australian National University. Graduating from Sydney University, he went to Oxford University on an 1851 scholarship in 1959. He became a Research Fellow of Lincoln College before finishing his DPhil and an official Fellow of St John's College Oxford in 1963. He is one of the discoverers of isotopic contrast variation in neutron scattering – which is currently used worldwide for understanding the structure of "soft matter".

NOV
04

1186th General Meeting

"Powering the US grid from solar and wind"

Dr David Mills, co-founder of Ausra, Inc.

Wednesday 3 November 2010 at 7 pm

Conference Room 1, Darlington Centre, University of Sydney

Solar and wind are our two largest energy resources and are well distributed globally. In these respects, they are ideal to re-power humanity with little climate or political impact. Some say that such a strategy is not practical because the solar resource disappears at night and each wind generator can be highly variable in output. However, the impact of already commercially available solar thermal storage technology, together with the overlap effects of wind energy from many sites may prove otherwise.

The first example used is the USA 2006 electrical load calculated on an hourly basis from government data and the second is a total energy supply scenario. A high voltage DC grid backbone (commercially available today) is assumed to allow full access of delivered power to all parts of the country. National wind and solar output are calculated hourly using government resource data. The initial results of the analysis are presented together with a discussion of the roles of solar and wind in such a new system, in comparison to conventional baseload/peaking thinking.

The talk will begin with an update of Dr Mills' company's activities in the United States since his leaving Sydney in early 2007, followed by an update of today's solar technology. The main part of the talk describes private work in progress by the author and his colleagues in the United States to take a first look at the feasibility of powering the United States energy system entirely from wind and sun by mid-century.

Dr Mills is the former Head of the Solar Energy Group at the University of Sydney and past President of the International Solar Energy Society. He is the co-founder and former chairman of the SHP and Ausra companies.

JUN
07

1200th Ordinary General Meeting

"Transit of Venus 2012 - what we and others saw"

Dr. Andrew Jacob, Assistant Curator, Sydney Observatory

Wednesday 6 June 2012 at 6.30 pm

Sydney Observatory, Observatory Hill, Sydney

Meeting report by Donald Hector

Early in the 17th century, Johannes Kepler predicted that every 120 years or so Venus would pass between the Earth and the Sun and on each occasion, there would actually be two transits about seven years apart. This was a particularly important prediction: Kepler's third Law had provided the means to accurately calculate of the relative distances of each of the planets from the sun but there was no way to determine the absolute distance between them. By observing a transit of Venus from different points on the Earth, observing the times at which the transits start and finish and the exact location of the observation it is relatively simple to calculate the absolute distance between the Earth and Sun (referred to as one Astronomical Unit). From Kepler's third Law it is then possible to calculate the distance of the other planets from the sun but, more importantly, it then enables the calculation of distant astronomical bodies using the Astronomical Unit as a baseline.

The Society was fortunate to be able to mark the transit of Venus at the Sydney Observatory with a talk given by Dr Andrew Jacob, the Observatory's assistant curator. Not only is the transit of Venus an important and rare astronomical event, astronomy and, in particular, the transit of Venus, play and important part in both the history of Australia and history of the Society.

The first predicted transit was in 1631 but there is no record of any successful observation is being made. The next, in 1639, was observed by Jeremiah Horrocks who was able to calculate the Astronomical Unit to an accuracy of about 50%. The next pair of transits were in 1761 and 1769. Lieutenant James Cook was ordered to sail to Tahiti to observe the 1769 transit which he did successfully and the rest, as they say, is history.

The next pair of transits in the 19th century (1874 and 1882) were observed using much more sophisticated instruments, including photography and these observations enabled very precise estimates of the Astronomical Unit.

The first of the 21st-century transits in 2004 was noted as an interesting phenomenon but not of any particular scientific importance. However, in the few years between 2004 and the 2012 transit, the discovery of hundreds of "exo-planets" (planets orbiting far-away stars) led astronomers to realise that precise observations of the phenomena caused by the transit of Venus could allow a much more precise and detailed characterisation of exo-planets.

It is notable that the Royal Society of NSW traces its origins to 1821 when the Philosophical Society of Australasia invited the Governor, Sir Thomas Brisbane, to become its first president. Brisbane was a keen astronomer and made important contributions to the science both in Australia and when he returned to Scotland.

OCT
07

1185th General Meeting

"Is the climate right for nuclear power?"

Dr Ziggy Switkowski, Chair of the Australian Nuclear Science and Technology Organization

Wednesday 6 October 2010 at 7 pm

Conference Room 1, Darlington Centre, University of Sydney

The world is experiencing a strong warming trend believed to be driven by greenhouse gas emissions associated with the burning of fossil fuels for energy production. Australia's demand for electricity, and energy in general, is expected to double by 2050. The challenge is to moderate and meet this growing demand in an environmentally responsible way. Nuclear power is already widely used around the world and the debate for its deployment in Australia is well under way.

This presentation will review the nuclear fuel cycle in the context of low emission energy technology and point to the potential role of nuclear power in Australia's energy and climate change strategy.

Dr Ziggy Switkowski is the Chair of the Australian Nuclear Science and Technology Organization. He is also a non-executive director of Suncorp, Tabcorp and Healthscope, and Chair of Opera Australia. He is a former chief executive of Telstra, Optus and Kodak (Australia).

In 2006 he chaired the Prime Minister's Review of Uranium Mining, Processing and Nuclear Energy which returned nuclear power to the country's strategic debate. He has a PhD in nuclear physics from the University of Melbourne and is a Fellow of the Australian Academy of Technological Sciences and Engineering.

JUL
05

1201st Ordinary General Meeting

"Autoimmune diseases: obesity, nutrition, exercise and eating disorders: what shape are Australians in?"

Professor Ian Caterson AM, Boden Professor of Human Nutrition, Sydney Medical School, University of Sydney

Wednesday 4 July 2012 at 6.30 pm

Union, University and Schools Club, 25 Bent Street, Sydney

Meeting report by Donald Hector

At 1201st Ordinary General Meeting of the Society held at the Union University and Schools Club on Wednesday 4 July 2012, Professor Ian Caterson AM talked about the serious obesity epidemic that confronts Australia. This is not confined to Australia – it is a major health problem all developed countries and increasing alarmingly in the developing world, due to the low cost and ready availability of high-energy foods.

Professor Caterson discussed how the epidemiology involved. From the time of World War II when there was worldwide food rationing to the present, where there is generally a surplus of food, average weight has consistently increased. Currently, young adults are gaining, on average, 1 kg per year. The problem is not how much you weigh, rather it is how fat you are. More particularly the problem is how much visceral fat you have (visceral fat sits around the organs inside the abdominal cavity). Unfortunately for many of us "the fatter you are, the younger you die". A good indicator of obesity due to visceral fat is body-mass index (BMI), defined as your mass in kilograms divided by the square of your height in metres. Normal BMI is in the range of 18.5-24.9. A BMI in the range of 25-29.9 is considered to be pre-obese and a BMI of over 30 is considered to be obese. In Australia, 62% of men and about 50% of women have a BMI greater than 25.

Obesity is implicated in a wide range of debilitating disorders: cardiovascular disease, diabetes, sleep apnoea, hypertension, cancer and infertility (the average BMI of women enrolled in fertility programmes is 32. Losing 6 kg in weight increases fertility fifteen-fold).

At a BMI of about 25 (which is about the median in Australia) the biggest health risk is developing diabetes. Professor Caterson gave interesting case of Sumo wrestlers. They eat a high fat diet (in excess of 6,000 calories per day) but they are very strong and very fit. But when they stop fighting, within a year, 35% of them have developed diabetes and many die of heart disease in their 40s. While they are fit all their weight is outside their abdominal cavity but when they stop fighting and lose their fitness, their visceral fat increases rapidly.

Professor Caterson discussed the impact of this major health issue in terms of "disability-adjusted life-years lost". This is an indicator used by the World Health Organisation that combines into a single measure the debilitating effects of serious disease and mortality. The bad news is that if you smoke, are obese, and you are physically inactive you can look forward to losing about 14 years of good-quality life. But the news was not all bad.

In epidemiological terms, for every kilogram you lose, your death rate decreases by 6%. Changing diet can have a big impact. Eating slightly smaller portions, increasing protein, reducing saturated fat intake (replacing it where possible with monounsaturated fats, such as olive oil), increasing dietary fibre, eating fresh fruit and vegetables and getting regular exercise (ideally, one-two hours a day) can have a relatively quick and significant impact on BMI and overall health.

SEP
02

1184th General Meeting

"Long-term changes in solar activity – including the current Grand Minimum"

Ken McCracken, Jellore Technologies and Senior Research Associate, University of Maryland

Wednesday 1 September 2010 at 7 pm
Conference Room 1, Darlington Centre, University of Sydney

The sunspot record since Galileo's time, and the cosmogenic nuclides 10Be (in ice cores) and 14C (in tree rings) show that the degree of activity of the Sun has varied greatly over time. The solar activity, manifested by the occurrence of sunspots, solar flares, and coronal mass ejections may be quite high, as it has been since 1946; and was during Roman times, or very small as during the Maunder Minimum (1645-1715); the Dalton Minimum (1810-20) or the Gleissberg Minimum of 1900-10. In the first part of the lecture, the speaker will discuss his recent studies with Swiss colleagues of the last 10,000 years of 10Be data from the Arctic and Antarctic that shows that the Sun has exhibited a number of persistent periodicities in solar activity, the most important being of duration 2300yr, 210yr, ~85yr, and the well known 11/22 year solar cycle. He will also outline the last 30 years of satellite data that show that the solar irradiance varies by ~0.1% over the 11 year solar cycle.

Against that background, he will then describe the substantial reduction in solar activity that commenced in 2006. Since then, the sunspot behaviour has been similar to that during the Dalton minimum (1810-20). The interplanetary magnetic fields have been lower than at any time during the space age, and the cosmic radiation intensities are well above those at any time during the past 60 years. The solar irradiance has decreased well below that observed in the previous 30 years. The evidence indicates that the magnetic properties of the Sun are now very different from those at any time in the "Space Age". Based on the 10,000 year 10Be record, he will speculate that the Sun will remain relatively inactive (and cool) for the next 20 years, and it will then resume a steadily increasing state of activity until it reaches a peak of the Hallstatt (2300 year) cycle ~200 years in the future.

Ken McCracken has had a long and varied life as a scientist, technologist, and contrarian. Starting his research career in Tasmania and New Guinea in the 1950s, he was then deeply involved in the early days of the US space program for seven years while at the Massachusetts Institute of Technology and the University of Texas. He designed and built scientific instruments that were flown on seven spacecraft that went to the orbits of Mars and Venus in the 1960s to provide the information needed to protect the US astronauts from being killed, or losing their virility, en route to the Moon. Following a professorship at the University of Adelaide, CSIRO appointed him to inaugurate a new research laboratory to improve geophysical exploration for minerals in the harsh Australian environment. Moving to the Southern Highlands in 1989, he operated a consultancy providing scientific advice to the mining industry. Over the past decade he and his Swiss, US, and Australian colleagues have used results from ice cores from Greenland and Antarctica to understand how the Sun has waxed and waned in activity over the past 10,000 years, and how this has paralleled the twenty two little ice ages, and many warming periods in the Earth's climate over the past 10,000 years. With his wife Gillian, he owns and operates the 850 acre beef breeding property "Jellore" in High Range.

JUL
20

The Dirac Lecture 2012

"The accelerating universe"

Professor Brian Schmidt

Thursday 19 July 2012

In conjunction with the University of New South Wales and with the Australian Institute of Physics, the Society proudly presented the 2012 Dirac Lecture on Thursday, 19 July 2012. This year's lecture was delivered by Professor Brian Schmidt, 2011 Nobel Laureate for Physics.

Professor Schmidt took us on a fascinating journey of astronomy and cosmology, describing the work that he and his colleagues have done over the last two decades and where it fits in our understanding of the nature of the universe.

To establish a reference framework, we were taken on a quick tour of the universe using the speed of light as a ruler (the Moon is less than two light seconds from us. The Sun is 8 light minutes away. The nearest star, Alpha Centauri, is 4.3 light years away. We are 30,000 light years from the centre of our galaxy, the Milky Way. The nearest galaxy, Andromeda, is 2 million light years from us. The cosmic ray background establishes that the age of the universe is about 13.7 billion years, with the Hubble telescope being able to detect objects 12 billion light years away).

Although astronomy is one of the oldest sciences, modern cosmology had its beginnings in the 19th and 20th centuries when techniques such as spectral analysis began to be applied to light from the skies. Of particular importance was phenomenon known as the Doppler effect – objects that are moving towards us have their light shifted towards the blue end of the spectrum, while objects moving away have their light shifted to towards red. By analysing the spectra of galaxies, in 1916, Vesto Slipher found that all galaxies he observed were shifted towards red and therefore were moving away from us. The conclusion from this was that the universe is expanding.

Einstein's special theory of relativity published in 1907 proposed that acceleration due to gravity and acceleration due to motion are equivalent. This led to his general theory of relativity and the notion that space is curved. The solution to Einstein's equations are dynamic, implying that the universe should be in motion. To avoid the conclusion that the universe was expanding, Einstein introduced a "fudge factor" called the cosmological constant (Einstein later referred to this as his greatest blunder!).

One conclusion from the concept of an expanding universe is that at one point must have been a big bang. Observations suggest that the age of the universe could be as young as 9 billion years if its expansion was slowing due to gravity but this is contrary to observations that the oldest stars appear to be at least 12 billion years old.

Not only was Brian Schmidt interested in solving this problem and determining the age of the universe but he wanted to understand what its eventual fate might be. In the 1990s, by observing faintness/brightness plotted against high/low red shift it had been found that supernovae appeared to have very constant brightness and therefore could be used as a standard "candle". (It was later found that this was not quite so but further work to better understand Type 1A supernovae allowed for corrections that gave a very good correlation.)

Improved digital detection technology and data processing capability in the 1990s set the stage for major advances in astronomy. Many more supernovae could be observed and this gave the team led by Brian (whose area of specialisation was data processing) to study many high-resolution images and by tracking these images and filtering out background noise, to find supernovae candidates for much more detailed analysis. Brian's team found that distant supernovae were outside the range expected for a universe whose expansion was slowing. Detailed analysis of their data suggested that the expansion of the universe was in fact accelerating. This was contrary to the mainstream view of physicists at the time and, indeed was contrary to the findings of another team using a different approach to analysing the data. Professor Schmidt's team published their work and in 2011 were awarded the Nobel Prize.

The notion of a universe whose expansion is accelerating poses some interesting questions for cosmologists, not the least of which is what could be pushing it apart? Einstein's theory allows for the concept of "dark energy". The data from analysis of Type 1A supernovae can be explained if the forces are assumed to be about 30% "pull" from gravity and about 70% "push" from dark energy. For the universe to be flat (and an analysis of the background radiation of the universe shows that indeed it is flat, that is, the universe is not closed and it is not open), 27% of the universe would need to be matter and 73% would need to be dark energy. But the problem is that this is much more matter than appears to exist. The solution to this currently most favoured by cosmologists is the concept of "dark matter" - matter that we cannot see. And it is no small amount - less than 5% of all matter is thought to be observable.

Professor Schmidt concluded his lecture with some long-range forecasts for the future of the universe. In some places, gravity will win and matter will merge; in others, space will accelerate faster and light from those areas will never reach us. There could even be a "big rip". In this scenario, a few million years before the end, gravity would be too weak to hold the Milky Way and other galaxies together. Our solar system would become gravitationally unbound, the stars and planets would be torn apart and at the very end, individual atoms would be ripped apart.

AUG
05

1183rd General Meeting

"The dynamic brain: modeling sleep, wake, and activity in the working brain"

Professor Peter Robinson, University of Sydney

Wednesday 4 August 2010 at 7 pm

Conference Room 1, Darlington Centre, University of Sydney

The brain's activity varies around the clock in response to stimuli, light inputs, and the buildup and clearance of sleep-promoting chemicals - somnogens. Signatures of brain activity have been observed for over a century and are widely used to probe brain function and disorders, often via the electroencephalogram (EEG) recorded by electrodes on the scalp, or through functional magnetic resonance imaging (fMRI), which measures a combination of blood volume and deoxygenation. Here, a quantitative physiologically based model of the working brain is described that responds correctly to the day-night cycle, somnogens, caffeine and pharmaceuticals, and generates activity in the cortex consistent with brain imaging measurements. Successful applications to numerous experiments are described, including EEGs, seizures, sleep deprivation and recovery, fatigue, and shift work. Aside from its scientific uses, this working brain model is currently finding clinical and industrial applications to brain function measurement and to prediction and monitoring of alertness.

Peter Robinson received his PhD in theoretical physics from the University of Sydney in 1987, then held a postdoc at the University of Colorado at Boulder until 1990. He then returned to Australia, joining the permanent staff of the School of Physics at the University of Sydney in 1994, and obtaining a chair in 2000. He is currently an Australian Research Council Federation Fellow working on topics including sleep, brain dynamics, space physics, plasma theory, and wave dynamics.

JUL
08

1182nd General Meeting

"Pluto and the uber-nerds"

Fred Watson, Anglo-Australian Observatory at Coonabarabran

Wednesday 7 July 2010 at 7 pm

Conference Room 1, Darlington Centre, University of Sydney

When is a planet not a planet? When it's a dwarf-planet, perhaps? So what's the difference? In 2006, astronomy's governing body, the International Astronomical Union, wrestled with this very question at their General Assembly in Prague. Before we knew it, media all around the world had declared that Pluto had been "dumped" from its status as the ninth planet, hinting that it had been unfairly thrown out of the Solar System. And in 2008 things got worse, with Pluto joining the lowly ranks of a new class of objects with the unflattering name of Plutoids. In this entertaining and fully illustrated journey through Pluto's eventful history, Fred Watson debates whether pragmatism and good science should prevail over sentiment and tradition.

Fred Watson says he has spent so many years working in large telescope domes that he has started to look like one. He is Astronomer in Charge of the Anglo-Australian Observatory at Coonabarabran, where his main scientific interest is gathering information on very large numbers of stars and galaxies. He is also an adjunct professor at the Queensland University of Technology, the University of Southern Queensland, and James Cook University. Fred is the author of "Stargazer: The Life and Times of the Telescope", and is a regular broadcaster on ABC radio. His new book "Why is Uranus upside down?" is based on listener questions, and was published in October 2007 and won the 2008 Queensland Premier's Literary Prize for Science Writing. In 2003, Fred received the David Allen Prize for communicating astronomy to the public, and in 2006 was the winner of the Australian Government Eureka Prize for Promoting Understanding of Science. Fred has an asteroid named after him (5691 Fredwatson), but says that if it hits the Earth it won't be his fault ...

AUG
02

1202nd Ordinary General Meeting

"Photonic circuits for the new information age: faster, smaller, smarter and greener"

Ben Eggleton, Professor of Physics, ARC Federation Fellow, Director of the Centre of Excellence for Ultrahigh-bandwidth Devices for Optical Systems (CUDOS) and Director of the Institute of Photonics and Optical Science (IPOS)

Wednesday 1 August 2012 at 6.30 pm

Union, University and Schools Club, 25 Bent Street, Sydney

Meeting report by Donald Hector

The ARC Centre for Excellence for Ultrahigh-Bandwidth Devices for Optical Systems (CUDOS) is a world-leader in research in photonics and the development of photonic devices. Its director, Professor Ben Eggleton, gave a wide-ranging talk about the Centre's work and photonics generally.

The use of light to communicate information is by no means a novel concept. Signals such as flags and lights for sending information have been used for many hundreds if not thousands of years. In the last couple of hundred years, various systems have been devised such as collimators and various lens systems. Three major breakthroughs of the last half-century or so were the invention of microelectronic devices, the invention of the laser and, importantly, the discovery by Charles Kao in 1966 that the physical properties of glass fibres were ideal for transmitting optical signals. Photonics, which combines these technologies, provides extraordinary capability for extremely high-speed transmission of data through optical fibre.

The reason that glass fibre is suitable is that there is a narrow part of the absorption spectrum in glass about 25 THz wide where attenuation of the signal is only about 0.2 dB per kilometre. Lasers can generate discrete packets of visible light light that can be transmitted down the fibre. Importantly, the photons do not interfere with one another and can be separated at the other end and the data encoded in the packets of light can be read. The relatively small signal loss can be managed by periodically installing amplifiers along the fibre-optic cable. There are now fibre-optic networks joining all major continents and these are the primary means for moving digitised data around the world.

A significant advantage of this fibre-optic technology has been its scalability. Developments in photonics and vastly increased the capacity of fibre-optic cables since the first ones were laid over 20 years ago. The National Broadband Network that Australia is currently installing is intended to deliver 1 Mb per second to well over 90% of households in Australia. There has been some speculation that this may become obsolete but this is unlikely as technological pathways to upgrade this to one terabit per second are already on the horizon.

One of the areas that CUDOS is working in is the application of nanotechnology and the development of materials with physical properties that do not occur in nature. These are giving rise to some novel applications such as "cloaking" (where photonics can be applied to make things appear invisible in certain parts of the spectrum). Other real possibilities of nanotechnologies are the development of a three-dimensional microchips that would allow major steps forward in processing speed.

Although in principle, photons do not interact with one another in a vacuum, in a medium such as glass, high-intensity laser excitation can cause a non-linear response of the glass medium and cause the photons to interact with one another. Conceptually, this may make possible the development of ultrahigh speed devices, switching as quickly as 1 trillionth of a second. This would make them up to 1000 times faster than current optical devices.

The Centre for Excellence for Ultrahigh-Bandwidth Devices for Optical Systems is recognised as one of the top few photonics research centres in the world. It is a collaboration of eight of Australia's top universities and number of industry participants. Expectations are high that it will make a major contribution in the emerging field of photonics.

Royal Society Events

The Royal Society of NSW organizes events in Sydney and in its Branches throughout the year. 

In Sydney, these include Ordinary General Meetings (OGMs) held normally at 6.00 for 6.30 pm on the first Wednesday of the month (there is no meeting in January), in the Gallery Room at the State Library of NSW. At the OGMs, society business is conducted, new Fellows and Members are inducted, and reports from Council are given.  This is followed by a public lecture presented by an eminent expert and an optional dinner.  Drinks are served before the meeting.  There is a small charge to attend the meeting and lecture, and to cover refreshments.  The dinner is a separate charge, and must be booked in advance.  All OGMs are open to members of the public.

Since April 2020, during the COVID-19 pandemic, face-to-face meetings have been replaced by virtual meetings, conducted as Zoom webinars, allowing the events program to continue uninterrupted.  It is hoped that face-to-face meetings can be resumed in the latter half of 2021. 

The first OGM of  the year, held in February, has speakers drawn from the winners of the Royal Society Scholarships from the previous year, while the December OGM hears from the winner of the Jak Kelly award, before an informal Christmas party.  The April or May event is our black-tie Annual Dinner and Distinguished Fellow lecture.

Other events are held in collaboration with other groups, including:

  • The Four Societies lecture — with the Australian Institute of Energy, the Nuclear Panel of Engineers Australia (Sydney Division), and the Australian Nuclear Association
  • The Forum — the Australian Academy of Science, with the Australian Academy of Technology and Engineering, the Australian Academy of the Humanities, and the Academy of the Social Sciences in Australia
  • The Dirac lecture — with UNSW Sydney and the Australian Institute of Physics
  • The Liversidge Medal lecture — with the Royal Australian Chemical Institute

We use cookies on our website. Some of them are essential for the operation of the site, while others help us to improve this site and the user experience (tracking cookies). You can decide for yourself whether you want to allow cookies or not. Please note that if you reject them, you may not be able to use all the functionalities of the site.