Matthias Maurer researches the hardening of concrete in zero gravity.
Climate protection through more efficient use of raw materials.
Experiments in space provide data for technical developments on earth.
Cooperation DLR with the universities of Cologne and Duisburg-Essen.
The experiment is part of the Cosmic Kiss mission.
COLOGNE, Germany (DLR PR) — How does freshly poured concrete behave in zero gravity? And how can this contribute to environmental protection on Earth? In early February 2022, the German ESA astronaut Matthias Maurer searched for answers to these questions on the International Space Station experiment “MASON/Concrete Hardening” is a joint project of the German Aerospace Center (DLR), the University of Cologne and the University Duisburg-Essenand takes place as part of the Cosmic Kiss mission.
On December 25, 2021 at 9:20 a.m. local time (1:20 p.m. CET), the James Webb Space Telescope, the largest space telescope of all time to date, took off from the spaceport of the European Space Agency on an Ariane 5 launcher.
A total of four instruments are housed on James Webb. Two of them come from Europe and have German shares.
The German Space Agency at DLR coordinates the German contributions for ESA and for an instrument in the national space program.
KOUROU, French Guiana (DLR PR) — James Webb Space Telescope – JWST for short – was launched from the European spaceport in Kourou (French Guiana) on its journey to Lagrange Point 2, 1.5 million kilometers away. James Webb is the largest and most expensive space telescope of all time, which has now started its long journey into the depths of space with an Ariane 5 upper stage ‘Made in Germany’. In addition, MIRI (Mid Infrared Iinstrument) and Near Infrared ( Near Infrared Spectrograph) – two of the four instruments on board – German parts: The near-infrared instrument NIRSpec was built by Airbus in Ottobrunn and Friedrichshafen. With this instrument, scientists from all over the world want to analyze the ‘hours of birth’ of the universe. NIRSpec is primarily intended to detect the radiation from the first galaxies that formed shortly after the Big Bang.