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06 March 2020 | Story Ruan Bruwer | Photo Supplied
Nomsa Mathontsi
Nomsa Mathontsi has been training with the South African senior women’s football team since Monday (03/02).

Whether she takes to the field or not, being part of the senior national women’s soccer team is already an accomplishment, says Nomsa Mathontsi. 

The BAdmin student in Economic and Management Sciences has been chosen for the Banyana Banyana squad for the first time. They face Lesotho on Sunday, 8 March 2020 in an international friendly in Johannesburg. There could be two Kovsies on the field, as Mating Monokoane, another University of the Free State student, was selected for Lesotho’s team. Both of them are midfielders.

The 21-year-old Mathontsi, who has been part of the Kovsie football team since 2018, says it will be a dream come true for her to wear the national colours. “Even if I don't get to play, I will still be proud of myself for being able to take on the challenge of going to camp and giving myself a chance to show my talent.”

“We have been together since Monday, 2 March 2020 and it has been the best experience, especially the fact that football has put me in the high-performance centre (South African Football Association girls’ academy), and now I get an opportunity to be with Banyana for the first time.”

“I was shocked when I got the call, but excited to face the challenge because it's never easy to get a call-up to Banyana, you need to work for it,” she says.

According to Mathontsi, who grew up in Mamelodi, Pretoria, her first love was athletics, but that changed during the 2010 World Cup in South Africa.
“I was an athlete back in primary school and it just so happened that I was selected to play football, which I never really enjoyed. I also had the opportunity to be part of the 2010 FIFA World Cup ceremonies, where I developed a love for football.”

News Archive

Two scientists part of team that discovers the source of the highest energy cosmic rays at the centre of the Milky Way
2016-03-22

Description: Giant molecular clouds  Tags: Giant molecular clouds

Artist's impression of the giant molecular clouds surrounding the Galactic Centre, bombarded by very high energy protons accelerated in the vicinity of the central black hole and subsequently shining in gamma rays.
Artist's impression: © Dr Mark A. Garlick/ H.E.S.S. Collaboration

Spotlight photo:
Dr Brian van Soelen and Prof Pieter Meintjes of the UFS Department of Physics.
Photo: Charl Devenish

H.E.S.S. (High Energy Stereoscopic System) scientists publically revealed their latest galactic discovery in the international science journal, Nature, on 16 March 2016. These scientists were able to pinpoint the most powerful source of cosmic radiation – which, up to now, remained a mystery.

Part of this team of scientists are Prof Pieter Meintjes and Dr Brian van Soelen, both in the University of the Free State (UFS) Department of Physics. Dr Van Soelen explains that they have discovered a proton PeVatron – a source that can accelerate protons up to energies of ~1 PeV (10^15 eV) – at the centre of the Milky Way. The supermassive black hole called Sagittarius A has been identified as the most plausible source of this unprecedented acceleration of protons.

The protons are accelerated to Very High Energy (VHE) gamma rays. The energy of these protons are 100 times larger than those achieved by the Large Hadron Collider at CERN (the European Organization for Nuclear Research).

According to Dr Van Soelen, the fact that this research has been published in Nature demonstrates the importance and pioneering nature of the research conducted by H.E.S.S. The H.E.S.S. observatory – operational in Namibia – is a collaboration between 42 scientific institutions in 12 countries.

In 2006, H.E.S.S. was awarded the Descartes Prize of the European Commission – the highest recognition for collaborative research – and in 2010 the prestigious Rossi Prize of the American Astronomical Society. The extent of the observatory’s significance places it among the ranks of the Hubble Space Telescope and the telescopes of the European Southern Observatory in Chile.

“The next generation VHE gamma-ray telescope,” Dr Van Soelen says, “will be the Cherenkov Telescope Array (CTA), which is currently in the design and development stage.” Both Dr Van Soelen and Prof Meintjes are part of this project as well.

H.E.S.S. has issued a complete statement about the paper published in Nature.

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