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18 April 2019 | Story Eugene Seegers | Photo Stephen Collett
Prof Chris Hermans
Prof Chris Hermans, extraordinary professor at the UFS, presents his inaugural lecture, titled Theology in an Age of Contingency.

“The road ahead is empty / It’s paved with miles of the unknown.”

Prof Chris Hermans quoted these lines from the song The Road Ahead, by Dutch vocal group City to City to introduce his inaugural lecture in the Faculty of Theology and Religion on 27 February 2019. Prof Hermans, a veteran researcher in pastoral theology, empirical, and practical religious studies at the Radboud University Nijmegen in the Netherlands and an extraordinary professor at the UFS, chose as his theme Theology in the Age of Contingency, stating that the uncertainty of life has affected all disciplines in the academy, from the sciences, philosophy, and pedagogy, to theology itself.

Although contingency is often defined as a “future event ... which is possible but cannot be predicted with certainty” (Oxford English Dictionary), Prof Hermans stated that, in the context of theology, it has more to do with complexity, unpredictability, coexistence of cultures, and an increasing number of decisions people need to make in modern-day life. 

Changing lanes

Prof Hermans recounted a memory from his childhood to illustrate some aspects of contingency: “Growing up, my parents told me to cycle on the right side of the road. They knew what the right side was. Everything had a right side: What norms and values to live by, what was right or wrong, when to pray and which words to use. ... We now live in a different world.”

Prof Hermans’ inaugural lecture reflected on four tasks of practical theology and missiology. He further asserted that the content and aim of these tasks change from the perspective of contingency.

Contingency perspectives

From a sociological perspective, said Prof Hermans, contingency is a characteristic of the age of modernisation in which we live. He stated that in the modern age, people have a much greater choice of individual ‘action options’ as well as a growing number of experiences as a result. Expounding on this, he said, “The fact that I am a Christian, and another person Hindu or Muslim, is largely due to the fact that I was born within a Christian family. The fact that I am Christian is a possibility and an actuality, but not a necessity.”

Prof Hermans also helped listeners to understand other areas in which contingency plays a role, such as the binary logic used when determining modalities of truth, or changing world views and philosophies of being, or even in our ethos, our art of living, and outlook on life.

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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