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01 October 2024 | Story Anthony Mthembu | Photo Kaleidoscope
S4F2024
The Science-for-the-Future (S4F) unit in the Faculty of Education hosted a summit on 13 September 2024. The event, which was held on the University of the Free State Bloemfontein Campus, was well attended by nearly 300 guests from across the country.

Teachers from across the country and representatives of nine other universities recently gathered at the University of the Free State (UFS) to celebrate the achievements of the S4F Teacher Professional Development programmes as well as the successful collaboration between the UFS and other universities in this regard.

The Science-for-the-Future (S4F) unit in the Faculty of Education hosted a summit in the Centenary Complex on the Bloemfontein Campus on 13 September 2024. The acting Vice-Chancellor and Principal of the UFS, Prof Anthea Rhoda, delivered the keynote address at the summit. Representatives from the South African National Roads Agency (SANRAL) – the official funder of the Science for the Future initiative – were also present, along with about 300 attendees, representing teachers, participating universities, representatives from the Department of Basic Education, and other stakeholders.

In her welcoming address, Prof Matseliso Mokhele Makgalwa, Vice-Dean of the Faculty of Education, said the event focuses, among others, on fostering collaboration and innovation across academic and professional communities. She later highlighted the fact that the project implementation period of three years makes provision for continued visits to the participating schools to sustain the continuity over time.

Dr Cobus van Breda, Programme Director of S4F and Project Manager of the Universities Collaboration initiative, elaborated on the rationale of the project as well as the collaboration with nine other universities. He stated, “We know from research that there are many factors that prevent learners, especially in rural areas in South Africa, from excelling in Mathematics and Science. These include subject content knowledge, lack of teaching resources at school and at home, language of learning and teaching that differs from home language, along with a lack of parental involvement, among others.” He said the project aims to address these rampant challenges by not only empowering teachers with the necessary teaching skills and content knowledge, but also providing classroom resources to benefit learners and adding a parental involvement component to the project. 

To scale the project benefits for the rest of the country, the UFS has partnered with nine other universities; collectively, more than one hundred thousand project participants (teachers, learners, and parents) could be impacted during 2024. The collaborating universities are Nelson Mandela University, the Walter Sisulu University, the University of Limpopo, the University of KwaZulu-Natal, the University of Mpumalanga, Sol Plaatje University, the University of Venda, Stellenbosch University, and Nort-West University.

Representatives from the Department of Basic Education and other institutions were also given the opportunity to highlight the impact of the initiative in their respective institutions. Maki Molale, Senior Education Specialist  from the Free State Department of Basic Education, reflected on the contribution of the project and said, “In the Department of Education we report on these key areas: teacher development, direct learner support, parental involvement, the utilisation of resources and partnerships … they are all addressed in this project.” She thanked the University of the Free State and the funder, SANRAL. Dr Glynnis Daries from Sol Plaatje University spoke on behalf of the collaborating universities and explained from an academic perspective to attendees how the project implementation strategy of S4F relates to Bronfenbrenner’s bioecological theory of human development and how the respective project components showcase the five levels of this theory.

During the keynote address, Prof Rhoda emphasised the importance of Mathematics skills, teaching children the capacity to solve problems and how it is extremely important to be analytical in one’s approach to resolving complexities and to work through problems in a methodical and logical manner. In the end, if one does this, no challenge is insurmountable. She commended the teachers present for fulfilling a vital task and pointed out the heavy responsibility on their shoulders. In this regard, she said, “As the UFS, and through the Science for the Future project, we are proud to support you in your work. The project is a vehicle through which we fulfil the central goals of the UFS, which are to impact the community in a positive way, and to instil a culture of excellence in a caring environment. We will continue to support you in your work and do all that we can to make your work more fulfilling and impactful – this is the promise of the UFS to our partners through this project.”

In acknowledging the contribution of the respective collaborating universities, Prof Rhoda emphasised that partnerships and collaborations are not easy to build, and most importantly, to maintain … “but what I’m hearing through these engagements today is that these partnerships are not just being maintained, they are expanded … the collaboration impacted the different institutions as well as, most importantly, the communities, close to and around them”. She alluded to the fact that universities’ roles are not just to retain and accept students, but universities have an important role in being the anchor within the society and communities in which they find themselves. According to her, the contribution of SANRAL and other project funders thus extends far beyond teachers’ professional development and community empowerment, it contributes towards assisting universities in engaged scholarship activities.

In reflecting on the parental involvement component of the programme, Themba Mhambi – Chairperson of the SANRAL Board – said that apart from being a maths and science project, and a project that is developmental, that is nation building, “… it becomes a kind of template for perhaps how our education system needs to be re-constructed … reclaiming the old times when parents and teachers worked together with the child in the centre”.  

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.

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