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Copernical Team
Deloitte announces formal space practice for rapidly growing space industry
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Hubble unexpectedly finds double quasar in distant universe
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New interactive mosaic uses NASA imagery to show Mars in vivid detail
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Scoping out the next sampling stop for Perseverance
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A new measurement could change our understanding of the Universe
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NASA's Webb Scores Another Ringed World with New Image of Uranus
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Europe’s biggest test chamber for space antennas takes shape
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Antennas and radio frequency systems for space are growing larger and more powerful, so to keep pace ESA’s ground-based test facilities are scaling up too. A construction project underway beside the dunes of the North Sea marks the expansion of the ESTEC technical centre in the Netherlands with the addition of Europe’s largest antenna and radio-frequency payload test chamber – Hertz 2.0.
Jupiter’s radiation belts – and how to survive them
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ESA’s Jupiter Icy Moons Explorer, Juice, is headed to the largest structure in the Solar System – not the gas giant itself but the mammoth magnetic field that it generates. Its exact size varies with the solar wind, but Jupiter’s magnetosphere is on average 20 million kilometres across, which is about 150 times wider than its parent planet and almost 15 times the diameter of the Sun. But within that field lurks a clear and present danger to space missions – intense belts of radiation much more energetic and intense than Earth’s own Van Allen belts.
Juice mission to Jupiter testing—down to the wire
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Preparing the Juice mission to Jupiter has involved testing for all kinds of contingencies, down to the smallest of scales. This microscopic view shows surface damage to a tiny silver interconnector after being exposed to erosive atomic oxygen known to be found surrounding Jupiter's moon Ganymede.
Due to launch on April 13 to begin an eight-year journey to the largest planet in the solar system, ESA's Jupiter Icy Moons Explorer, Juice, will spend three and a half years in the Jupiter system, and in the final phase of its exploration will go into orbit around the largest Jovian moon, Ganymede.
However, previous observations by the Hubble Space Telescope have revealed auroral glows around Ganymede due to the presence of 'atomic oxygen'—individual atoms of oxygen at the fringes of the moon's scanty atmosphere, the result of standard oxygen molecules being broken apart by the powerful radiation belts surrounding Jupiter.
ESA materials engineer Adrian Tighe explains, "Atomic oxygen is also experienced in Earth orbit, due to oxygen molecules being dissociated by ultraviolet radiation from the Sun, and all Earth-orbiting missions below about 1000 km altitude are designed to resist it.
Improving astronaut vision in long-haul space flights
