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04 January 2021 | Story Igno van Niekerk | Photo Francois van Vuuren (iFlair)
Anton Roodt

 The Afrikaans words, weerlose meganika, can be roughly translated as ‘vulnerable mechanics’. If you do not know the exact meaning of this, rest assured, you are not alone. At least one person does. Anton Roodt of Roodt Architects has been summoning a storm of positive reviews in the literary world with his debut offering, which is neither an environmentally friendly building nor creative historical restoration for which he is renowned, but a book.

Weerlose meganika was written as part of the requirements for Roodt’s fourth MA degree – all obtained at the University of the Free State (UFS), where the Roodts have been part of the UFS family for three generations. Anton’s father was the Head of the department of Architecture, and his son recently completed his studies in the same department. His wife, Zarine, has been involved as lecturer and research fellow in the Department of Communication Science. Roodt’s wide spectrum of interests shows in the variety of his MA degrees (Architecture, Town and Regional Planning, Environmental Management, and now – Creative Writing).

Roodt, renowned for his creativity and innovative manner of working, has barely stepped into the world of literature; yet the book, published by Tafelberg Publishers, is being described in words probably never used by critics: “verrassend vernuwend” (surprisingly refreshing), “baldadig,” (which I can only translate as ‘wildly playful’), and nostalgic science fiction.

In a Zoom conversation, Roodt shared that he wrote mostly in his spare time. Many hours of study in the buzz of architecture classrooms taught him to focus anywhere and anytime. According to Roodt, the chapters that had to be removed in the final edits of Weerlose meganika comprise sufficient material for a second book. 

Anton and his son, Leon-Pierre, both worked on the cover of Weerlose meganika: Anton designed it and Leon-Pierre was responsible for the graphics. Although publishers usually prefer to appoint their own designers, Tafelberg liked and kept the design as presented. This was no surprise, as design is not new to Anton who, as a student, was involved in the design of rag posters. During a particular rag, he realised that the poster design was extremely successful, as about 90% of them were stolen by students from lampposts and other areas. 

Roodt’s recipe for success? He is naturally curious and wants to learn more about many things. This allows him to connect with interesting people such as his fellow students and lecturers (Dr Francois Smith and Prof Henning Pieterse) in the Creative Writing course, where they kept on pushing each other to improve their work. It is clear that Roodt is on a lifelong journey of learning. And, in case you are wondering – yes, he recently started his PhD studies. At the UFS, of course.

When I asked Anton about the strange title, Weerlose meganika, he explained that he has always been fascinated by juxtapositions. He loves bringing seemingly unrelated elements together. 

Looking at the reviews, he has been successful once again. 

*** If you are curious to know more, Weerlose meganika is available at most bookstores, as well as online.

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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