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14 May 2025 | Story Tshepo Tsotetsi | Photo Supplied
Africa Month 2025
Africa: Our identity, our journey, our future.

Each May, countries across the continent mark Africa Month, reflecting on the formation of the Organisation of African Unity in 1963 (now the African Union) and the shared vision for a united, thriving Africa. In 2025, the AU draws attention to justice and reparations for Africans and people of African descent. At the University of the Free State (UFS), the commemorative period invites reflection on African identity, futures, and connectedness through learning, dialogue, and cultural expression.

Throughout the month, a range of campus events will celebrate African identity, highlight voices from within the UFS community, and foreground indigenous knowledge systems and the arts – all integral to the institution’s vision of shaping a future grounded in African values and global relevance.

Prof Lynette Jacobs, Acting Director of the Office for International Affairs, believes the continent’s greatest potential lies in its people, cultures, and ways of knowing. “Africa is the heart of humankind … What excites me most is the growing recognition that Africa’s richness lies not only in its resources but also in its people, cultures, and knowledges, both ancient and contemporary,” she says.

Prof Jacobs highlights the university’s role in fostering ethical leadership and driving innovation rooted in African priorities. “We need to produce locally grounded graduates who can hold their own amongst the world’s best; we need to foster ethical, service-oriented leadership; and to serve as hubs for interdisciplinary research. By nurturing innovation, collaboration, and critical thinking, institutions like UFS can help shape an Africa that is not only self-reliant but also a key contributor to global progress.”

Portia Mtawarira, the SRC representative for international students on the Bloemfontein Campus, echoes this belief. “I envision Africa as a continent where we embrace and celebrate diversity – a future where people come together for a common goal: to improve access to quality education, fight social injustice and corruption, reduce unemployment, and promote globalisation and internationalisation,” she says.

She adds that UFS provides a space where this kind of leadership can grow. “The university has created platforms where students can develop the skills needed to become ethical leaders, problem-solvers, and change-makers … It’s now our responsibility to go back into our communities and put into practice the knowledge we’ve acquired here.”

From international collaborations and mobility networks to the everyday spirit of mutual support on campus, Prof Jacobs says she sees interdependence as the African spirit embodied at UFS. “It reflects the deep awareness across African societies that our progress is bound together, and that solutions emerge from solidarity, not divisiveness.”

As UFS continues on its Vision 130 journey, Africa Month affirms the institution’s enduring commitment to connection, celebration, and co-creating a future shaped by African excellence.

 

Africa Month Events Calendar:

 

Intercultural Sports Day

The offices of SRC International Students and SRC Sports will host an Intercultural Sports Day that will celebrate cultural diversity through sports.

Date: 16 May 2025

Time: 13:00–17:00 

Location: Bloemfontein Campus

 

Africa Day Memorial Lecture

The Centre for Gender and Africa Studies will host its annual Africa Day Memorial Lecture presented by Prof Cyril Obi, Program Director at the Social Science Research Council, New York. The theme of the lecture is ‘Caught between De-Democratisation and Re-Democratisation: Grappling with Africa’s Complex Conjunctures through the Lens of Political Dialectics’.

Date: 21 May 2025

Time: 18:00

Venue: Equitas, Bloemfontein Campus


 

Africa Day commemoration podcast panel discussion

The Office for International Affairs will host its annual Africa Day commemoration podcast panel discussion featuring UFS Chancellor Prof Bonang Mohale and the former Minister of International Relations and Cooperation, Dr Naledi Pandor. The theme is ‘Africa’s Future: Higher Education and Global Impact’. 

Date: 22 May 2025 

Time: 19:00–20:30 

Venue: Albert Wessels Auditorium, Bloemfontein

Click to view document Click here to RSVP

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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