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22 February 2024 | Story Leonie Bolleurs | Photo SUPPLIED
Action Learning Workshop 2024
Along with Prof Richard Teare (far right) are some of the workshop attendees, which consisted of a group of 15 students, academics, and community organisation leaders.

The Directorate Community Engagement at the University of the Free State (UFS) recently hosted Prof Richard Teare, the President of the Global University of Lifelong Learning (GULL). During his visit, he presented a workshop on action learning.

GULL, established 17 years ago, offers lifelong learning opportunities for people in communities and workplace organisations around the world. It provides frameworks and awards in support of lifelong learning.

Prof Teare described what the process of action learning entails and how it differs from the notion of ‘training’. According to him, action learning occurs when people learn from each other, create their own resources, identify their own problems, and form their own solutions. He stated, “The process is so enriching that every learner is able to identify personal and life-transforming outcomes. These commonly include expressions of enhanced self-confidence, self-belief, renewal, enthusiasm for learning, a new sense of direction and purpose for career and life – along with news skills, insights, and the sense of being equipped for the future.”

The workshop, attended by a group of 15 students, academics, and community organisation leaders, had an element of self-directed development, according to Dr Karen Venter, Head of the Division of Service Learning at the University of the Free State (UFS). “Participants learned how action learning can enable self-directed personal and professional development,” she said.

Skills and leadership characteristics

GULL pathways were also profiled to outline some of the innovative ways in which it can be used to facilitate continuous development aligned with professional certification. It offers three generic pathways, each with five levels (or certification points) leading to professional bachelor’s, master’s, and doctoral degrees,” explained Dr Venter.

“In practice, community leaders who have obtained one of these professional degrees can now become change agents for community development in their own community organisations, using the action learning pathway and certification offered by GULL,” she said.

Dr Venter added that a group of students from the UFS – the Active Community Citizens through Engaged Scholarship for Sustainability (ACCESS) group – embarked on a Professional Bachelor pathway certified by GULL last year. Not only did the group of 11 students successfully earn certification, including one Level Two certificate, five Level Three diplomas, three advanced diplomas, and one bachelor’s degree at the Engaged Scholarship Awards 2023, but they also developed a range of skills and leadership characteristics during the process. These include eco-brick making, vermiculture and gardening, eco-entrepreneurship, soap and candle making, and creative recycling, to name a few. 

Furthermore, the pathway is underpinned by community-based research to drive initiatives of student structures towards implementing impactful community engagement in three clusters, namely sustainable environment, well-being, and social justice.

Addressing SDGs and embracing Vision 130

Lifelong action learning is one of the innovative approaches for the development of graduate attributes. In this light, the outcomes of not only the action learning workshop, but also the learning opportunities presented by GULL, align with the UFS Vision130. “Using action learning for bringing social change, students can address the United Nations Sustainable Development Goals (SDGs) and embrace the values of the UFS’ Vision130 – impact, care, excellence, sustainability, accountability, and social justice,” stated Dr Venter.

One of the attendees communicated the experience as follows: “I learned that action learning is a process for self-determined personal and professional development – the change starts with me developing myself and then sharing it with others.” 

For further opportunities presented by GULL, visit the website here.

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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