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11 May 2023 | Story Leonie Bolleurs | Photo Supplied
Eco-vehicle Race
Join the UFS on 13 May 2023 at 09:00 (student performances at 09:00 and race at 10:15) on the road around the UFS Odeion School of Music for the annual Kovsie ACT Eco-Vehicle Race. Don't miss out on this incredible display of endurance; support your favourite team to victory!

Kovsie ACT at the University of the Free State (UFS) is presenting the sixth Kovsie Eco-Vehicle Race this year.

Come and show your support for our students who will be representing our colleges and three campuses, along with the Central University of Technology. Be a part of the action:

Date: Saturday 13 May 2023
Time: 09:00 Performances by student artists
Time: 10:15 Official start of Eco-Vehicle Race
Venue: UFS Odeion School of Music parking area

The Eco-Vehicle Race represents the last phase of a nine-month co-curricular skills programme, providing our students with a set of skills that prepare them for the world of work. 

In this programme where students are equipped with basic knowledge and skills on sustainable energy, they get the opportunity not only to race the eco-vehicles, but to also understand the workings of the vehicle, which is critical for repairs done by the team during the race. 

Our students will be competing in three events:

  • Obstacle course: Teams will be challenged by obstacles to test their control over the car.
  • Smart lap: A timed lap in which the drivers take the main track for the first time.
  • Endurance race: The teams need to finish as many laps as possible using the least amount of energy in 45 minutes. 
The winners of the three events will each receive a trophy. There will be a trophy for the best pit stop as well as a spirit cup for the team with the best energy and support from the audience.

Come and support our students as they showcase their ingenuity and endurance. Don't miss out on the action! For more information, click here to contact Jady Carelse.

Car manufacturers will also exhibit hybrid/electric vehicles; come and view the exhibition and learn more about how these cars work and their benefits.

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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