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18 February 2022 | Story Leonie Bolleurs | Photo Leonie Bolleurs
Faculty of Theology and Religion opening
Present at the Faculty of Theology and Religion’s Theology Day were from the left: Dr Eugene Fortein, Dr Siphiwe Dube, Prof Rantoa Letšosa, and Prof Charlene van der Walt.

This year, the Faculty of Theology and Religion at the University of the Free State (UFS) resumed its annual tradition of celebrating the new academic year, after being halted by the COVID-19 pandemic in 2020.

The focus was on a theology of vulnerability for our times, with the theme supported by the text verse from 2 Corinthians 4:7: “We have this treasure in clay jars.” 

God embodies vulnerability

Dean of the faculty, Prof Rantoa Letšosa, left delegates with the inspiring message that one of the treasures in these clay jars is the power of God; power that enables us to stand strong and move forward in trying circumstances, such as the COVID-19 pandemic. He wished all attendees, both in person and online, to experience this extraordinary strength and power of God in the new year. 

Prof Rian Venter from the Department of Historical and Constructive Theology, who led the worship service, talked about humanity that has achieved so much – in the areas of health, space, communication, transport, etc. “Despite all these achievements, we are more insecure, with an intensified sense of vulnerability,” he said. 

“However, the One in whom we believe as our Saviour and Lord is a vulnerable God; he embodied vulnerability. We cannot talk about God as if he is not affected by our vulnerability. He is love. He is affected by us,” he said. 

Depriving people of humanity 

But to be vulnerable can also be seen as to be weak, defenceless, open to harm, in need of care, and deprived of one’s humanity. 

Dr Siphiwe Dube from the University of the Witwatersrand integrated the topic of vulnerability into the paper he delivered, speaking from a decolonialism point of view on the research topic: Towards a Decolonial Political Theology of Vulnerability: Reflections from the Margins. In one of his statements, he said that black people are living in the reality constructed for them and have not discovered what blackness is. He urged the young attendees to make use of spaces created for discussion of this matter. 

Bringing to the table another perspective on this topic, was Prof Charlene van der Walt from the School of Religion, Philosophy and Classics at the University of KwaZulu-Natal. Her paper was on the othering, stigmatisation, and exclusion experienced by the LGBTIQA+ people in the African context in general and the African faith communities in particular. She connected the shame experienced by queer people in a family setting to the story of Joseph in the book of Genesis in the Bible. In her paper: Reflecting on Joseph in the context of Izitabane vulnerability, violence, identity erasure and the imperative of recognition and accompaniment, she stated that Joseph’s otherness informed the vulnerability, exclusion, violence, and identity erasure that happens within the confines of family. 

According to Prof Van der Walt, she wished to not argue for LGBTIQA+/ Izitabane people to be seen or that they somehow ‘pass’ and slip below the radar, but that the recognition called for implied a different kind of seeing: it implied a compassionate witnessing and a humanising recognition. “It implies process, interrogation of power, empathy and imagination, weeping and a commitment to community,” she said. 

Another interesting perspective on the theology of vulnerability was that of Dr Eugene Fortein from the Department of Historical and Constructive Theology at the UFS. In his paper on Vulnerability by Design: On a Theology of Prophetic Solidarity, he asked why the vulnerable is vulnerable? What led to them being vulnerable?
 
“The presence of the vulnerable in South Africa is not an accident. It is not because of fate, but because of a design that is 370 years in the making; deliberately to keep people poor for generations to come.” 

He said it started with Jan van Riebeeck. Legislation such as the Natives Land Act of 1913, the Group Areas Act of 1950, and the Bantu Education Act of 1953 also played a key role. “These were designed to oppress one group and enabling the other to thrive.”

“The scars of this legislation are still haunting us today,” he said. 

The One in whom we believe as our Saviour and Lord is a vulnerable God; he embodied vulnerability. We cannot talk about God as if he is not affected by our vulnerability. He is love. He is affected by us. – Prof Rian Venter

“The vulnerable have names and faces. They are experiencing the effects of being vulnerable on their bodies and that is not to be taken lightly.”

“Do not only pray for the poor and the vulnerable, but work actively to bring restitution,” he said. The church now has the opportunity to be a true servant of Christ,” Dr Fortein added. 

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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