Latest News Archive

Please select Category, Year, and then Month to display items
Previous Archive
11 October 2022 | Story Nonsindiso Qwabe
Qwaqwa research conference
Unpacking the role of research in society. From left: Lukhona Mnguni, Prof Pearl Sithole, Prof Dipane Hlalele, and Prof Percy Hlangothi

From socio-political dynamics and creativity in the Basotho language, to the improvement of water conditions in the upper Tugela River and antifungal studies of Cydonia oblonga extracts (known as kwepere in Sesotho) – these are just some of the highlights of the research presented at the UFS Qwaqwa Campus research conference.

With a theme focused on research as a tool for the betterment of humanity, the two-day research conference provided a space for the campus to showcase its research for sustainable development in the Afromontane region and beyond, conducted by academics and postgraduate students alike. The two-day event comprised oral student and staff presentations and sessions, with shorter presentations on the second day.

As global trends continue to challenge society to solve big and immediate problems, there has been a natural turn towards research that can make a lasting impact on local and global platforms. Through student and academic presentations, the conference provided insights into how the UFS is playing an active role in responding to some of these challenges by being outwardly focused in their approaches to problem-solving.

Balancing the sciences, industry, and society

With an intentional focus on interdisciplinarity, the guest speakers – all in different science fields – offered solutions to conducting impactful research through the lens of their own work. Prof Percy Hlangothi is currently an Associate Professor of Physical and Polymer Chemistry at Nelson Mandela University (NMU) and inaugural Director of the Centre for Rubber Science and Technology, a research entity in the Faculty of Science at the same institution. By describing his work, particularly on the production of tyres, he focused on the importance of achieving rapport between the sciences, industry, and society.

The second keynote speaker was Lukhona Mnguni, a governance, politics and development specialist and PhD candidate in Political Science at the University of KwaZulu-Natal. He currently serves as the Head of Policy and Research at the Rivonia Circle. Mnguni focused his talk on the breakthroughs of research as stemming from people, and not academic disciplines themselves. Mnguni issued a hard call towards a reflection of what the intellectual and scholarly quest for knowledge is doing to society, emphasising the need for societal involvement in issues pertaining to crises in society.

Prof Dipane Hlalele, Professor of Education at UKZN and a C2 NRF-rated researcher (2022-2027), was the final speaker for the conference. He anchored his talk on the importance of having philosophical frames behind scholarship, and spoke against approaching rural areas as lacking knowledge, to a stance of mutual understanding of knowledge schemes and models of intervention.

Campus focused on making an impact outwardly

Marking the opening of the conference, Dr Martin Mandew, Qwaqwa Campus Principal, said the campus was trying to punch above its weight and evolve its research and knowledge outputs. “We cannot just be consumers of knowledge and finished products that come from abroad. We have to produce our own knowledge that speaks to our own unique circumstances and makes complete sense of our capacities,” he said.

The conference also served as the launch platform for the campus research strategy. During the launch, Prof Pearl Sithole, Campus Vice-Principal: Academic and Research, said the strategy was centred on five frontiers. “We are trying to align what we do outwardly in terms of impact and are working on ourselves as per the commitments of the strategy. We do this excellently, because we want to advance knowledge – there is no question about that – and we put pressure on each other to do that. It does not mean that it will be easy, but we are going to engineer it such that originality and the advancement of knowledge is happening.”

The conference concluded with a prize-giving session for the best oral student presentations.

News Archive

UFS physicists publish in prestigious Nature journal
2017-10-16

Description: Boyden Observatory gravitational wave event Tags: Boyden Observatory, gravitational wave event, Dr Brian van Soelen, Hélène Szegedi, multi-wavelength astronomy 
Hélène Szegedi and Dr Brian van Soelen are scientists in the
Department of Physics at the University of the Free State.

Photo: Charl Devenish

In August 2017, the Boyden Observatory in Bloemfontein played a major role in obtaining optical observations of one of the biggest discoveries ever made in astrophysics: the detection of an electromagnetic counterpart to a gravitational wave event.
 
An article reporting on this discovery will appear in the prestigious science journal, Nature, in October 2017. Co-authors of the article, Dr Brian van Soelen and Hélène Szegedi, are from the Department of Physics at the University of the Free State (UFS). Both Dr Van Soelen and Szegedi are researching multi-wavelength astronomy.
 
Discovery is the beginning of a new epoch in astronomy
 
Dr van Soelen said: “These observations and this discovery are the beginning of a new epoch in astronomy. We are now able to not only undertake multi-wavelength observations over the whole electromagnetic spectrum (radio up to gamma-rays) but have now been able to observe the same source in both electromagnetic and gravitational waves.”
 
Until recently it was only possible to observe the universe using light obtained from astronomical sources. This all changed in February 2016 when LIGO (Laser Interferometer Gravitational-Wave Observatory) stated that for the first time they had detected gravitational waves on 14 September 2015 from the merger of two black holes. Since then, LIGO has announced the detection of two more such mergers. A fourth was just reported (27 September 2017), which was the first detected by both LIGO and Virgo. However, despite the huge amount of energy released in these processes, none of this is detectable as radiation in any part of the electromagnetic spectrum. Since the first LIGO detection astronomers have been searching for possible electromagnetic counterparts to gravitational wave detections. 
 
Large international collaboration of astronomers rushed to observe source
 
On 17 August 2017 LIGO and Virgo detected the first ever gravitational waves resulting from the merger of two neutron stars. Neutron star mergers produce massive explosions called kilonovae which will produce a specific electromagnetic signature. After the detection of the gravitational wave, telescopes around the world started searching for the optical counterpart, and it was discovered to be located in an elliptical galaxy, NGC4993, 130 million light years away. A large international collaboration of astronomers, including Dr Van Soelen and Szegedi, rushed to observe this source.
 
At the Boyden Observatory, Dr Van Soelen and Szegedi used the Boyden 1.5-m optical telescope to observe the source in the early evening, from 18 to 21 August. The observations obtained at Boyden Observatory, combined with observations from telescopes in Chile and Hawaii, confirmed that this was the first-ever detection of an electromagnetic counterpart to a gravitational wave event. Combined with the detection of gamma-rays with the Fermi-LAT telescope, this also confirms that neutron star mergers are responsible for short gamma-ray bursts.  
 
The results from these optical observations are reported in A kilonova as the electromagnetic counterpart to a gravitational-wave source published in Nature in October 2017.
 
“Our paper is one of a few that will be submitted by different groups that will report on this discovery, including a large LIGO-Virgo paper summarising all observations. The main results from our paper were obtained through the New Technology Telescope, the GROND system, and the Pan-STARRS system. The Boyden observations helped to obtain extra observations during the first 72 hours which showed that the light of the source decreased much quicker than was expected for supernova, classifying this source as a kilonova,” Dr Van Soelen said.

We use cookies to make interactions with our websites and services easy and meaningful. To better understand how they are used, read more about the UFS cookie policy. By continuing to use this site you are giving us your consent to do this.

Accept