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19 November 2018 Photo Sonia Small
On Statues and Statutes MT Steyn statue creates a vital precedent
Prof Francis Petersen, UFS Rector and Vice-Chancellor

Opinion article by Prof Francis Petersen

Every morning on my way to the office, I pass this imposing figure. Elevated on a granite plinth in front of the Main Building of the University of the Free State’s Bloemfontein Campus, cast in bronze, more than twice the size of a normal person, the statue of President Marthinus Theunis Steyn is by all accounts an impressive work of art.
  
Why such a contentious figure?

Unlike Cecil John Rhodes, who has become the embodiment of colonialism in South Africa, history paints the last president of the independent Orange Free State a little more amicably: MT Steyn was an outspoken anti-imperialist, a pacifist who tried until the very end to avoid war with Britain, a humanitarian who did a lot for Boer women and children after the war.
  
However, he was also the leader of a republic that didn’t acknowledge the rights of all its ethnic groups. From a modern-day human rights perspective, his Free State was decidedly unequal and unjust.
  
In its recent report, the ministerial task team on the transformation of the heritage landscape points out that statues are never just “innocent pieces of architecture.”  They embody a strong “symbolic power” and project “the foundational values of the state and those in power.” It’s never about the persona alone, but about the totality of values he/she represents.

Situated where it is – in front of the building housing the university’s executive – the question is whether we, as the leadership of this institution, align ourselves with these values.

And if there’s any doubt, how should we go about to consider changing the status quo?

Removal of statues in the past

As South Africans, we are acutely aware of how unhappiness about statues and what they represent have been dealt with on our university campuses in the past.

Statues have been defaced, damaged, and toppled by protestors – not only in South Africa, but around the world. At the University of the Free State (UFS), it also happened with the statue of CR Swart on the Bloemfontein Campus; the same as with the statue of Cecil John Rhodes at the University of Cape Town.

There is of course a legitimate driving force behind students’ conduct: frustration about the perceived slow pace of transformation.
  
However, what should also be considered, is the heritage legislation that is in place to protect symbols that hold historical value and significance – specifically aimed at preserving our country’s cultural heritage for all its citizens.

Process followed

At the UFS, discussions regarding the possible repositioning of the MT Steyn statue date as far back as 2003. In January this year, our Integrated Transformation Plan (ITP) was launched, and the statue was identified as a priority within the work stream dealing with ‘Names, Symbols and Spaces.’

At a student engagement earlier this year, the student community, through the Student Representative Council (SRC), once again asked for the statue to be removed. It was clear that it made certain students feel unwelcome because it represented a period in history that they did not feel part of.

I realised the urgency of the matter and appointed a Special Task Team to fast-track the review of the statue’s position. Four options had to be considered during the review process: (i) retention of the statue in its current position; (ii) reinterpretation; (iii) relocation on campus; (iv) relocation to a site off campus.

The task team, made up of representatives of various campus communities, appointed an independent heritage consultant to conduct a Heritage Impact Assessment (HIA) as prescribed by the heritage legislation, consulted widely, and gathered qualitative data. This encompassed a two-month-long public participation process.

Great effort went into inviting people to comment on the position of the statue, like erecting a giant reflective column in front of the statue, effectively erasing it out from a frontal view of the Main Building. Seven questions in English, Afrikaans, and Sesotho about the statue and the person it represents, cement benches to invite reflection, and a suggestion box for comments completed the picture. In addition, I also had various individual meetings with relevant role players, including members of the Afrikaans community on campus, the SRC, and alumni.
  
Robust discussion sessions were facilitated on campus, and various opinion articles were carried widely in the media.

As there is no precedent for such a process under current South African legislation, the task team was guided at all times by principles of fairness, inclusivity, and objectivity.

The Special Task Team has now presented the university’s executive with a report, and a final decision on the position of the statue will be made during a meeting of the University Council on 23 November 2018.

What we learned

I have repeatedly been asked whether the time, effort, and resources we’ve poured into the process around deciding the statue’s future have been worth it. My answer is consistently a resounding “yes”. 

Through this process, everyone involved with our university were given the opportunity to express their opinions on this aspect of its future. It was a chance to really listen to one another.

Where discussions sometimes became one-sided and overbearing, we could use it as an opportunity to lay down the rules for respectful debating as a quid pro quo for future discussions on any matter.

In short: The two-month public participation period was a fruitful time of discussion, reflection, and communication. 

A time of deliberate stocktaking on the values which are important for all our communities.
  
Road ahead

Whatever the final decision on the Steyn statue, it is bound to dissatisfy some. That much is unavoidable. 

However, I believe that this should not inevitably lead to division on our campuses. I see the wake of the statue journey as an opportunity to foster a new university citizenship based on the value of caring – a value that we all treasure.

The past few months have given us a chance to think deeply about what it truly means to care; also, to reflect on how we should apply this value in order to be a university where equality, social justice, tolerance, and forward-looking is actively lived out every day. 

A place where everyone truly feels welcome – and involved.

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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