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17 January 2025 | Story Lunga Luthuli | Photo Supplied
Intsika Food Garden
The newly redeveloped Intsika Garden on the UFS Qwaqwa Campus, designed to promote accessibility, sustainability, and community engagement. The garden's flexible spaces offer opportunities for students to relax, collaborate, and connect with one another.

The UFS Qwaqwa Campus is transforming its landscape to provide more than just a physical connection between buildings. The redevelopment of the garden in front of the Intsika Building marks a shift towards integrating communal spaces that support interaction, inclusivity, and sustainability. 

According to Nico Janse van Rensburg, Senior Director: Facilities Planning at University Estates, the primary aim of the redevelopment is to celebrate the diversity of the university as its ‘greatest asset’ by creating spaces that promote community engagement. “Previously, the garden was underutilised and did not connect properly to the rest of the campus’ circulation network. We identified an opportunity to develop it into a social space where academia and visitors can connect,” Van Rensburg explained.  

Accessibility and sustainability  

The Intsika Garden redevelopment aligns with the broader strategic goals of the institution, particularly in infrastructure planning. The project focuses on making the space universally accessible, ensuring that it caters for people with disabilities while improving overall circulation on the campus. “The development strives to improve the accessibility to different functions on the campus by making the space and circulation routes universally accessible,” said Van Rensburg.  

This initiative is also embedded in the university’s commitment to sustainability, as waterwise plants, artificial grass, and low maintenance finishes have been carefully selected to reduce the environmental footprint. “Artificial grass was used in combination with natural vegetation, which requires minimal water and maintenance,” he added.  

In addition to accessibility, sustainability plays a central role in the redevelopment. The project is designed to contribute to the university’s goal of reducing its carbon footprint by promoting pedestrian-friendly spaces and minimising the reliance on fossil-fuel-driven vehicles.  

Van Rensburg highlighted the efficiency gains in the management of green spaces, noting that the design will reduce the frequency of maintenance, which in turn reduces carbon emissions and energy consumption. “By promoting pedestrian circulation and integration with public transport, the use of vehicles using fossil fuels is minimised,” he said. Walking, he added, is not only a more environmentally friendly option, but also promotes the health and well-being of the campus community.  

Social spaces for collaboration  

The redevelopment introduces six new social nodes across the campus, each offering unique opportunities for student engagement and collaboration. “Smaller pockets have been created, which form part of the larger public space, resulting in a microclimate where people can relax and socialise,” Van Rensburg explained.  

The spaces are designed with flexibility in mind, featuring various seating arrangements, including spaces for meetings and group collaborations. Among the new additions is an amphitheatre, which provides a multifunctional space for lectures, performances, and other activities. “Flexible communal spaces were created for recreational opportunities, resulting in a balanced campus lifestyle,” Van Rensburg added.  

Recognising the increasing reliance on technology, the redevelopment also incorporates features such as charging stations and Wi-Fi connectivity. The spaces are envisioned as ‘information zones’, providing students and staff with convenient access to online resources while they relax or connect outdoors. “With Wi-Fi connectivity, the spaces function as an extension to traditional libraries,” noted Van Rensburg.   

While the Intsika Garden redevelopment is a significant step forward, plans are already underway for further infrastructure and green initiatives. “The soft landscaping and signage contracts were awarded for the Intsika Garden,” Van Rensburg confirmed. He also revealed that much-needed renovations to the front of the Intsika Building are in the pipeline, with a contractor soon to be appointed for the construction work. The planned upgrade will align with the garden’s aesthetics by drawing inspiration from indigenous art and culture, creating a cohesive identity for the campus. 

As these developments progress into 2025, the Qwaqwa Campus will continue to evolve, offering students and staff spaces that not only enhance their academic experience, but also contribute to a more sustainable and connected environment. 

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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