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08 July 2022
Free State festival

The Vrystaat Arts Festival celebrates its twenty-second birthday this year, a remarkable achievement! After two challenging years of lockdown restrictions, the festival team is excited to work towards various in-person events again, including the first ever mini-MARK in July, the traditional arts festival with all the familiar faces in October, and the second instalment of the festival's classical music festival, Vrystaat Klank & Klassik, in November.

From 12-16 July, the festival will launch the inaugural Mini-MARK on the Bloemfontein campus of the University of the Free State (UFS). This smaller arts and crafts market will mostly be concentrated around the Callie Human Hall and the Exam Rooms on the UFS-campus and will involve only curated, unique, handmade, high quality, authentic South African products and food stalls, and an open stage for entertainment.

The mini-MARK will also include a selection of theatre, music, and dance productions. A definite highlight on the theatre program is the debut comedy, Laerskool Noord, with Margit Meyer-Rödenbeck, Marion Holm, and Ilne Fourie. Something special on the menu for the little ones is Liewe Heksie en die Rolskaate. Several local musicians will perform at the Vulture Club during the festival week and the contemporary dance production, POP, with Bloemfontein-based dancer, Thami Majela, and French choreographer, Matthieu Nieto will also be on the stage.

Two productions hosted in collaboration with the UFS’s Drama and Theatre Arts Department are The dressing room and Hoe Later, Hoe Kwater. The dressing room is based on the real antics of backstage life during the production of a community theatre musical. The show is not a musical, but a very relatable comedy to anyone who has been through the hustle of being backstage during a production.

Hoe Later, Hoe Kwater is an Afrikaans translation by Pierre van Pletzen of Michael Pertwee and John Chapman's Holiday Snap, and stars Barend Kriel, Mark Dobson, Jané Schnetler, DJ Kruger, Danielle Doubell, Amira-Xandria van Biljon, Paquot.

From 2-8 October 2022, the customary Vrystaat Arts Festival, with a full program including theatre productions, literature festival, film festival, visual and experimental art, as well as a much larger arts market, will also be presented on the UFS campus. Keep an eye out in the press and the arts festival's social media platforms for more information on the October program.

Entrance tickets to the festival grounds and to the theatre productions are already for sale at https://www.webtickets.co.za/.

For more information about this year's Vrystaat Arts Festival, please email mark@vrystaatkunstefees.co.za or alternatively send a WhatsApp to 063 584 4379.

News Archive

Discovery in Scorpius constellation may signify clean energy for Earth
2017-01-23

 Description: Discovery in Scorpius constellation may signify clean energy for Earth Tags: Discovery in Scorpius constellation may signify clean energy for Earth

Earlier this year, a group of international astronomers
announced the discovery of an exotic binary star system,
AR Scorpii. The system is in the Scorpius constellation.
Photos: Supplied

See article on Nature’s website 

In future, stargazers and astronomers will look at the Scorpius constellation near the Milky Way with new eyes. Earlier this year, a group of international astronomers announced the discovery of an exotic binary star system, AR Scorpii. The system is in the Scorpius constellation.

Prof Pieter Meintjes, researcher in the Department of Physics at the University of the Free State (UFS), worked with four colleagues on what he describes as a “wonderful discovery”. This sensational discovery, which could lead to the production of cleaner energy on Earth, will be published in the research journal, Nature, early in 2017.

Model developed to interpret new set of measurements
The exotic binary star which was discovered consists of a red dwarf and a white dwarf revolving around each other every 3,5 hours. The binary system showed very prominent pulsations of 117 and 118 seconds respectively. The pulsations can be explained by a bundle radiation produced by the white dwarf star.

“These new observations have shown that the radiation is strongly polarised, a sign that we are dealing with synchrotron radiation here. Synchrotron radiation is produced by electrons accelerated to extremely high energy levels in the magnetic field of the white dwarf star,” says Prof Meintjes.

He developed a theoretical model to interpret a new set of measurements that was taken by the 1,9 m telescope and the 10 m SALT telescope at the South African Astronomical Observatory (SAA0).

Totally unique phenomenon could contribute to energy production on Earth
“I further indicated that the interaction between the magnetic fields of the white dwarf star and the red dwarf star induces secondary processes that specifically describe the behaviour of the radiation in the radio band and infrared band accurately. AR Sco is the first white-red dwarf binary system of which all the pulsated radiation could be explained by the synchrotron process, which is totally unique,” says Prof Meintjes.

According to Prof Meintjes, the value of the model lies in the fact that the processes which produce the radiation in AR Sco, can also be applied to produce energy on Earth.

 

Plasma reactors are based on roughly the same processes which apply in AR Sco, and with refining, it could be utilised to generate electricity in future. This will be much cleaner than nuclear energy.

 

The model developed by Prof Meintjes explains all the radiation in the system – from radio waves to X-rays – in terms of electrons accelerated to extremely high energy levels by electric fields in the system, which then produce synchrotron radiation over a very wide band of the electromagnetic spectrum.

Prof Meintjes is currently working on a follow-up article examining the evolution of the AR Sco, in other words, the origin of such a unique system and the final state towards which it is evolving. “My vision for the immediate future is therefore to develop a model for the evolution of the source concerned,” he says.

 

 

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