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14 December 2021 | Story Leonie Bolleurs | Photo Supplied
Ofhani Mavhungu was recently awarded the Professor Rob Gous Scholarship by the Animal Feed Manufacturers Association (AFMA) of South Africa.

From a very early age, Ofhani Mavhungu knew he wanted to be involved in agriculture one day. Fast forward a few decades and you find Ofhani enrolled for the MScAgric Animal Science degree at the University of the Free State (UFS).

As a goal-orientated person who is open to new ventures, he reckons this degree will broaden his knowledge and understanding of the industry. “I believe Animal Science is an interdisciplinary field of study that enables students like me to pursue various career opportunities, ranging from primary animal production to secondary product processing, retail, and quality assurance. This motivates me to be part of the team that will ensure food security for the future generation,” says Ofhani.

Opening doors to a career in Animal Science

The Professor Rob Gous Scholarship for 2020/2021 that was jointly awarded to him and Victor Makofane of the University of Limpopo by the Animal Feed Manufacturers Association (AFMA) of South Africa, is for Ofhani a step closer to realising his dreams. 

“Diligence and hard work have always been the driving force throughout my studies, and I am delighted that my hard work was rewarded. This award further reflects on the Department of Animal Science’s dedication and commitment to build and mentor strong candidates who are recognised by the industry,” he says.

With increasing animal feed costs, the search for more cost-effective feed utilisation techniques – without compromising the nutritive value or feed quality – becomes critically important for intensive broiler producers. 

Ofhani’s study, which aims to evaluate the effect of increasing levels of a nutritional fat emulsifier with a high HLB on the (i) diet digestibility and (ii) production performance of broilers, will provide some insight into the possible energy-saving effect of dietary emulsifiers with a high HBL in broiler diets with moderate lipid inclusion levels. 

“A digestibility study will give more information on the emulsifier effect at metabolic level, and a production study will provide information on growth characteristics and carcass composition.”

An opportunity to compete with other candidates in the industry

“Few studies have been conducted on lipid emulsifiers under South African conditions, which necessitates the need for further research in this field,” he says. 

Ofhani, whose motto in life is to stay humble and accept positive criticism – as it is meant to enlighten you – wants to pursue a career in the animal feed industry. “My qualification will give me an opportunity to compete with other candidates of our generation in the industry, as well as on a research/academic level. By completing my MScAgric, I will broaden my own skill set so that I can continue with industry-related research in the future and provide mentorship to prospective animal scientists,” he adds. 

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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