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RETRO DIRK BACH
Fotoprobe von Kein Pardon - Das Musical im Capitol Theater, DŸsseldorf - Dirk Bach (als Heinz WŠscher), die Showgirls und der lustige GlŸckshase
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder, Barbara Wussow bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder, Barbara Wussow bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder, Sascha Gluth bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Barbara Wussow bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Barbara Wussow bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Brigitte Grothum, Tochter Debora Weigert bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Peter Sattmann bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Peter Sattmann bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder, Debora Weigert und Brigitte Grothum bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder, Debora Weigert bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder, Debora Weigert bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder, Ilja Richter bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder, Sascha Gluth bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder, Sascha Gluth bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder und Barbara Wussow bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder, Barbara Wussow und Sascha Gluth bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder und Barbara Wussow bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder und Barbara Wussow bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder und Barbara Wussow bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder und Barbara Wussow bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Barbara Wussow bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Barbara Wussow bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Brigitte Grothum bei der Jedermann Fotoprobe in Berlin
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Jedermann Fotoprobe in Berlin
Sascha Gluth bei der Jedermann Fotoprobe in Berlin / 181011 (FOTO: DUKAS/ACTIONPRESS)
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Jedermann Fotoprobe in Berlin
Sascha Gluth bei der Jedermann Fotoprobe in Berlin / 181011 (FOTO: DUKAS/ACTIONPRESS)
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Jedermann Fotoprobe in Berlin
Winfried Glatzeder und Herbert Köfer bei der Jedermann Fotoprobe in Berlin / 181011 (FOTO: DUKAS/ACTIONPRESS)
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Jedermann Fotoprobe in Berlin
Sascha Gluth bei der Jedermann Fotoprobe in Berlin / 181011 (FOTO: DUKAS/ACTIONPRESS)
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Bepi before space.
Bepi before space.
Launched in 2018, the BepiColombo spacecraft is due to make its flyby of Earth this Friday 10 April, helping it slow down to allow the SunÕs gravity to pull it closer to Mercury. This picture comes from 2014, showing its main Mercury Planetary Orbiter module bathed in simulated sunlight during ground testing, to give an idea of how the spacecraft will be illuminated in space as it passes its homeworld.
BepiColombo is actually made up of three spacecraft modules: ESAÕs MPO seen here, the Japan Aerospace Exploration AgencyÕs Mercury Magnetosphere Orbiter and the Mercury Transfer Module transporting the other two modules on their way to the innermost planet. They are due to arrive in December 2025 after two Venus flybys and six Mercury flybys.
The full BepiColombo stack was too big for ESAÕs Large Space Simulator, so thermal vacuum testing of the three modules took place separately. Within this cavernous 10-m wide, 15-m high chamber, they were subjected to orbital-quality vacuum as well the temperature extremes prevailing in space.
Credit: ESA / eyevine
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(FOTO: DUKAS/EYEVINE)
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Wenn die Musi spielt
Sänger Hansi Hinterseer bei der Generalprobe der ZDF Sendung Wenn die Musi spielt in Bad Kleinkirchheim
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Wenn die Musi spielt
Sänger Hansi Hinterseer bei der Generalprobe der ZDF Sendung Wenn die Musi spielt in Bad Kleinkirchheim
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Aarhus Mars Simulation Wind Tunnel
Aarhus Mars Simulation Wind Tunnel.
Part of Aarhus University’s Mars Simulation Laboratory in Denmark, this wind tunnel has been specially designed to simulate the dusty surface of planet Mars.
Constructed within an 8-m long, 2.5-m wide pressure chamber, the Aarhus Mars Simulation Wind Tunnel has attracted researchers from all over Europe and the United States, to test instruments and equipment for a wide range of Mars missions, including ESA’s ExoMars and NASA’s Mars 2020 rovers.
The air pressure within the wind tunnel can be taken down to less than one hundredth of terrestrial sea level and the temperature reduced to as low as -170°C using liquid nitrogen. Fans then blow the scanty atmosphere that remains at up to 30 m/s, along with Mars-style dust.
Researchers can evaluate how items such as sensors, solar panels and mechanical parts stand up to the clingy, abrasive particles, sourced from Mars-like, oxide-rich soil found in central Denmark.
“We’ve been in operation all through this decade,” comments Jonathan Merrison of Aarhus University’s Department of Physics and Astronomy, overseeing the facility. “We’re the only wind tunnel that not only reproduces the low pressure and low temperatures of Mars, but also allows the introduction of particulates of sand and dust.
“Probably about a third of the testing carried out here has been ExoMars related, then there have been users related to other Mars missions, as well as industrial testing of high altitude terrestrial equipment.
“We are also a member of the Europlanet network, a grouping of planetary scientists supported by the European Union, supporting the usage of various planetary simulation facilities and analogues.”
The Aarhus Mars Simulation Wind Tunnel was based on a smaller, earlier version, which remains in use. Its development was supported by ESA’s Technology Development Element programme for promising new technologies as well as the philanthropic Villum Kann Rasmussen Founda
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European launcher family
Artist's view of the European launcher family.
Shown from left to right: Ariane 5, Vega, the two-booster Ariane 6 (A62), Vega-C, the four-booster Ariane 6 (A64).
Ariane 5 and Vega are operated from Europe's Spaceport in Kourou, French Guiana.
Vega-C is set to debut in 2020, increasing performance from VegaÕs current 1.5 t to about 2.2 t in a reference 700 km polar orbit, covering identified European institutional usersÕ mission needs, with no increase in launch service and operating costs.
The first flight of Ariane 6 is planned for 2020. Ariane 6 provides a modular architecture using either two boosters (Ariane 62) or four boosters (Ariane 64), depending on the required performance. The P120C solid-propellant boosters will be common with Vega-C.
Credit: ESA / eyevine
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(FOTO: DUKAS/EYEVINE)
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Proben zum Finale des Eurovision Song Contest 2011 in DŸsseldorf
Anna Rossinelli fŸr die Schweiz bei den Proben zum Finale des Eurovision Song Contest 2011 in DŸsseldorf
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*** Last rehearsals of the Eurovision Song Contest in Dusseldorf / Germany on may, 13th, 2011*** (FOTO: DUKAS/ACTIONPRESS)
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Proben zum Finale des Eurovision Song Contest 2011 in DŸsseldorf
Anna Rossinelli fŸr die Schweiz bei den Proben zum Finale des Eurovision Song Contest 2011 in DŸsseldorf
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*** Last rehearsals of the Eurovision Song Contest in Dusseldorf / Germany on may, 13th, 2011*** (FOTO: DUKAS/ACTIONPRESS)
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Proben zum Finale des Eurovision Song Contest 2011 in DŸsseldorf
Anna Rossinelli fŸr die Schweiz bei den Proben zum Finale des Eurovision Song Contest 2011 in DŸsseldorf
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*** Last rehearsals of the Eurovision Song Contest in Dusseldorf / Germany on may, 13th, 2011*** (FOTO: DUKAS/ACTIONPRESS)
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Teilnehmer proben fŸr den Eurovision Song Contest 2011 in DŸsseldorf
Anna Rossinelli aus der Schweiz bei der Probe zum 1. Halbfinale fŸr den Eurovision Song Contest 2011 in DŸsseldorf
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Teilnehmer proben fŸr den Eurovision Song Contest 2011 in DŸsseldorf
Anna Rossinelli aus der Schweiz bei der Probe zum 1. Halbfinale fŸr den Eurovision Song Contest 2011 in DŸsseldorf
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Earth’s evil twin
EarthÕs evil twin. Appearances can be deceiving. This thick, cloud-rich atmosphere rains sulphuric acid and below lie not oceans but a baked and barren lava-strewn surface. Welcome to Venus.
The second planet from the Sun is often coined EarthÕs Ôevil twinÕ on account of it being almost the same size but instead plagued with a poisonous atmosphere of carbon dioxide and a sweltering 470¼C surface. Its high pressure and temperature is hot enough to melt lead and destroy the spacecraft that dare to land on it. Thanks to its dense atmosphere, it is even hotter than planet Mercury, which orbits closer to the Sun.
ESAÕs Venus Express studied the planet from orbit between 2006 and 2014, providing the most in-depth studies of its atmospheric circulation to date. This false-colour image was taken in ultraviolet light with the Venus Monitoring Camera on 23 July 2007. It shows a view of the southern hemisphere from equator (right) to the pole (left) from a distance of 35 000 km from the surface of the planet.
Scientists think that Venus once looked a lot like Earth, but underwent an irreversible climate change that is often used as an extreme example of what happens in a runaway greenhouse effect.
The main source of heat in the Solar System is the SunÕs energy, which warms a planetÕs surface up, and then the planet radiates energy back into space. An atmosphere traps some of the outgoing energy, retaining heat Ð the so-called greenhouse effect. It is a natural phenomenon that helps regulate a planetÕs temperature. If it werenÕt for greenhouse gases like water vapour, carbon dioxide, methane and ozone, EarthÕs surface temperature would be about 30 degrees cooler than its present +15¼C average.
Over the past centuries, humans have altered this natural balance on Earth, strengthening the greenhouse effect since the dawn of industrial activity by contributing additional carbon dioxide (FOTO: DUKAS/EYEVINE)
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ESA’s wandering eye.
ESAÕs wandering eye. Sitting 2400 m above sea level on the volcanic island of Tenerife, Spain, ESAÕs Optical Ground Station keeps watch on the skies.
The 1-m telescope nestled within the dome on the left of this image, spends its time surveying EarthÕs local environment for artificial debris objects, testing different strategies for observing risky asteroids (near-Earth objects) as well as testing and commissioning optical communication satellites. (The telescope is also used for quantum key distribution and feeder-link experiments.)
Part of the larger Teide Observatory, the optical ground station can detect artificial debris objects as small as 10-cm travelling in the Ôgeostationary ringÕ Ð a volume of space that comprises all geostationary orbits suitable for practical use, and one of the most valuable regions in space for telecommunications and Earth observation.
The search for fragments in the geostationary ring and a better knowledge of the current debris population are crucial to understand its future evolution, to assess the risk of collisions, and to define suitable and cost-efficient mitigation measures.
ESAÕs Space Safety activities are underpinned by such accurate data from observatories around the globe, not only on space debris and asteroids but on our energetic Sun.
Credit: ESO / eyevine
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Credit: ESA / eyevine
Contact eyevine for more information about using this image:
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(FOTO: DUKAS/EYEVINE)
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Dragon fire
Dragon fire.
SpaceXÕs Falcon 9 rocket carrying the Crew Dragon spits fire as it lifts off from Kennedy Space Center in Florida, 23 April at 05:49 local time. On board are ESA astronaut Thomas Pesquet, NASA astronauts Megan McArthur and Shane Kimbrough, and JAXA (Japan Aerospace Exploration Agency) astronaut Akihiko Hoshide.
The crew of four spent around 23 hours orbiting Earth and catching up with the International Space Station after their launch before docking to the Node-2 Harmony module, marking the start of ESAÕs six-month mission Alpha.
Thomas is the first European to be launched to space on a US spacecraft in over a decade. The new Crew Dragon ships four astronauts at a time, allowing more people to live and work on the International Space Station doing more research for scientists on Earth.
Alpha is ThomasÕ second space mission, and everything is set to be bigger and brighter. A Russian laboratory module, scheduled to arrive in the summer with a European robotic arm, will offer more ways of maintaining the International Space Station and supporting spacewalkers as they work outside. Thomas will help set up this arm and prepare it for use during the Alpha mission.
Over 200 international experiments are planned during ThomasÕ time in space. Of the 40 European ones, 12 are new experiments led by the French space agency CNES.
At the end of the Alpha mission in October, Thomas will take over commander of the International Space Station for a brief period and welcome ESA astronaut Matthias Maurer on his first flight to space.
Credit: ESA / eyevine
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(FOTO: DUKAS/EYEVINE)
ESA / eyevine