New research, out today, Tuesday, November 4, published in IOP Publishing’s Plasma Physics and Controlled Fusion, shows how knowledge gained from the pursuit of nuclear fusion research may reduce the threat to acceptable levels, making man’s first mission to Mars a much greater possibility.
The solar energetic particles, although just part of the ‘cosmic rays’ spectrum, are of greatest concern because they are the most likely to cause deadly radiation damage to the astronauts.
Large numbers of these energetic particles occur intermittently as “storms” with little warning and are already known to pose the greatest threat to man. Nature helps protect the Earth by having a giant “magnetic bubble” around the planet called the magnetosphere.
The Apollo astronauts of the 1960’s and 70’s who walked upon the Moon are the only humans to have travelled beyond the Earth’s natural “force field” – the Earth’s magnetosphere. With typical journeys on the Apollo missions lasting only about 8 days, it was possible to miss an encounter with such a storm; a journey to Mars, however, would take about eighteen months, during which time it is almost certain that astronauts would be enveloped by such a “solar storm”.
Space craft visiting the Moon or Mars could maintain some of this protection by taking along their very own portable “mini”-magnetosphere. The idea has been around since the 1960’s but it was thought impractical because it was believed that only a very large (more than 100km wide) magnetic bubble could possibly work.
Researchers at the Science and Technology Facilities Council’s Rutherford Appleton Laboratory, the Universities of York, Strathclyde and IST Lisbon, have undertaken experiments, using know-how from 50 years of research into nuclear fusion, to show that it is possible for astronauts to shield their spacecrafts with a portable magnetosphere - scattering the highly charged, ionised particles of the solar wind and flares away from their space craft.
Computer simulations done by a team in Lisbon with scientists at Rutherford Appleton last year showed that theoretically a very much smaller “magnetic bubble” of only several hundred meters across would be enough to protect a spacecraft.
Now this has been confirmed in the laboratory in the UK using apparatus originally built to work on fusion. By recreating in miniature a tiny piece of the Solar Wind, scientists working in the laboratory were able to confirm that a small “hole” in the Solar Wind is all that would be needed to keep the astronauts safe on their journey to our nearest neighbours.
Dr. Ruth Bamford, one of the lead researchers at the Rutherford Appleton Laboratory, said, “These initial experiments have shown promise and that it may be possible to shield astronauts from deadly space weather”.
Joe Winters | alfa
NASA's Fermi catches gamma-ray flashes from tropical storms
25.04.2017 | NASA/Goddard Space Flight Center
DGIST develops 20 times faster biosensor
24.04.2017 | DGIST (Daegu Gyeongbuk Institute of Science and Technology)
More and more automobile companies are focusing on body parts made of carbon fiber reinforced plastics (CFRP). However, manufacturing and repair costs must be further reduced in order to make CFRP more economical in use. Together with the Volkswagen AG and five other partners in the project HolQueSt 3D, the Laser Zentrum Hannover e.V. (LZH) has developed laser processes for the automatic trimming, drilling and repair of three-dimensional components.
Automated manufacturing processes are the basis for ultimately establishing the series production of CFRP components. In the project HolQueSt 3D, the LZH has...
Reflecting the structure of composites found in nature and the ancient world, researchers at the University of Illinois at Urbana-Champaign have synthesized thin carbon nanotube (CNT) textiles that exhibit both high electrical conductivity and a level of toughness that is about fifty times higher than copper films, currently used in electronics.
"The structural robustness of thin metal films has significant importance for the reliable operation of smart skin and flexible electronics including...
The nearby, giant radio galaxy M87 hosts a supermassive black hole (BH) and is well-known for its bright jet dominating the spectrum over ten orders of magnitude in frequency. Due to its proximity, jet prominence, and the large black hole mass, M87 is the best laboratory for investigating the formation, acceleration, and collimation of relativistic jets. A research team led by Silke Britzen from the Max Planck Institute for Radio Astronomy in Bonn, Germany, has found strong indication for turbulent processes connecting the accretion disk and the jet of that galaxy providing insights into the longstanding problem of the origin of astrophysical jets.
Supermassive black holes form some of the most enigmatic phenomena in astrophysics. Their enormous energy output is supposed to be generated by the...
The probability to find a certain number of photons inside a laser pulse usually corresponds to a classical distribution of independent events, the so-called...
Microprocessors based on atomically thin materials hold the promise of the evolution of traditional processors as well as new applications in the field of flexible electronics. Now, a TU Wien research team led by Thomas Müller has made a breakthrough in this field as part of an ongoing research project.
Two-dimensional materials, or 2D materials for short, are extremely versatile, although – or often more precisely because – they are made up of just one or a...
20.04.2017 | Event News
18.04.2017 | Event News
03.04.2017 | Event News
25.04.2017 | Physics and Astronomy
25.04.2017 | Materials Sciences
25.04.2017 | Life Sciences