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04 September 2019 | Story Leonie Bolleurs | Photo Charl Devenish
Jon Jacobson
Delivering the 31st Sophia Gray Memorial Lecture and Exhibition in Bloemfontein, was Jon Jacobson from Metropolis Design in Cape Town.

What is inside and what is outside? What is coming alive in the light? Minimalism. Hugeness. Shadows. Soft. Art. Complex. Conversation. Ambiguity. Clarity. All phrases and words used by the most recent Sophia Gray laureate, Jon Jacobson from Metropolis Design in Cape Town, to describe aspects of his work.

He delivered the 31st Sophia Gray memorial lecture in Bloemfontein. The name of his lecture at this prestigious event, organised by the UUFS Department of Architecture, was in [de] finite. Jacobson is the first graduate in the department’s MArch with Design.

Nature plays a big role in many of his projects, with a blurred distinction between the inside and the outside of the structures he builds. His designs fulfil the desire of a union with nature. 

A detailed investigation

Jacobson creates places and spaces to celebrate being. “Architecture is undeniably art, but it is also embodied in the completeness of the lived moment,” he says. 

Every project starts with a detailed investigation. “What social theory will we engage with? How progressive is it? What attitude will we take to the environment, to the theory of family? What other personal concerns will we be worried about? It is important to engage critically with this information. Important to build a philosophical base for each project,” says Jacobson.

He also believes it is important to consciously ensure that form follows idea with the same intensity that it follows function and that it does not blindly follow other form. 

At Metropolis, Jon and his team are client centred in their approach to design. Jon explains the process: “Some of the content is brought from the client’s personal and social aspiration and some from contemporary architecture culture, but the most potent component is the hidden set of ideas that emerge from our own engagements with the living world such as popular science, geology, art, music, literature, philosophy, theology, mysticism, and many others. And this emerges in the hidden sense of the word, in its architecture content.”

Content approach to design

In house design, Jon categorises the content that informs the architecture of the house: content pertaining to the individual, their philosophy, values and beliefs, content derived from culture, architecture and the arts, passion, religion, politics, and content referring to the natural world and its processes. Content from each of these spheres is present in any of his work. 

Jon says a major implication of a content approach to design is that it requires a design framework that is largely operative at a level of idea rather than at the level of form. This contributes to creating architecture rather than just buildings. 

His design method allows conscious control over the relationship between the ideas, the forms, and the poetics of the projects. “And at any point in the building process, it is possible to trace back and to critically assess whether any particular form is aligning with the core ideas of the project,” Jon indicates. 

Jon’s first taste of grappling with the infinite of architecture was with a garden pavilion he built for rest and relaxation. “For the first time I felt that we integrated planning, content, sight, programme, structure, and materiality into one unified whole that was expressed with a minimum of means and that was more than just the sum of its part,” he states.

He strongly believes that the individual is at the centre of every architectural project. He says the belief systems, type of social needs, family dynamics, physical habits, and spatial practices of their clients need to be investigated in detail in order to facilitate a meaningful spatial experience.

He continues: “We see our role as designers to saturate the environment with the meaning that enhances our clients’ daily experience in every possible way – from the ergonomic and the practical to the spiritual. In the process, the logics and tradition of architecture and the ego of the architect sometimes need to make way for human need and aspiration.”


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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