“ESA’s CryoSat and the Copernicus Sentinel-1 missions have been used to measure subtle changes in the elevation and flow of ice shelves that, in turn, reveals how huge canyons are forming underneath. Warm bottom ocean water is entering the cavity under Antarctica’s Dotson ice shelf and is stirred by Earth’s rotation. This is causing one side of the ice shelf to melt. The canyon, which has formed over 25 years, is now 200 m deep in places and the ice just above it is heavily crevassed, affecting the shelf’s future ability to buttress the ice on land.”
Video credit: ESA/University of Edinburgh–N. Gourmelen/Planetary Visions
“A series of nighttime photos were taken by ESA astronaut Paolo Nespoli to create this time-lapse of the Earth as seen from the International Space Station. “
“This timelapse video shows Sentinel-5P satellite, from final preparations to liftoff on a Rockot launcher, from the Plesetsk Cosmodrome in northern Russia, on 13 October 2017.
The Sentinels are a fleet of satellites designed to deliver the wealth of data and imagery that are central to the European Commission’s Copernicus programme. This unique environmental monitoring programme is providing a step change in the way we view and manage our environment, understand and tackle the effects of climate change and safeguard everyday lives.
Sentinel-5 Precursor – also known as Sentinel-5P – is the first Copernicus mission dedicated to monitoring our atmosphere. The satellite carries the state-of-the-art Tropomi instrument to map a multitude of trace gases such as nitrogen dioxide, ozone, formaldehyde, sulphur dioxide, methane, carbon monoxide and aerosols – all of which affect the air we breathe and therefore our health, and our climate.
With a swath width of 2600 km, it will map the entire planet every day. Information from this new mission will be used through the Copernicus Atmosphere Monitoring Service for air quality forecasts and for decision-making. The mission will also contribute to services such as volcanic ash monitoring for aviation safety and for services that warn of high levels of UV radiation, which can cause skin damage. In addition, scientists will also use the data to improve our knowledge of important processes in the atmosphere related to the climate and to the formation of holes in the ozone layer.
Sentinel-5P was developed to reduce data gaps between the Envisat satellite – in particular the Sciamachy instrument – and the launch of Sentinel-5, and to complement GOME-2 on MetOp. In the future, both the geostationary Sentinel-4 and polar-orbiting Sentinel-5 missions will monitor the composition of the atmosphere for Copernicus Atmosphere Services. Both missions will be carried on meteorological satellites operated by Eumetsat. Until then, the Sentinel-5P mission will play a key role in monitoring and tracking air pollution.”
“[This is a] Video showing a test of the mechanisms steering the four solar electric propulsion thrusters on BepiColombo’s Mercury Transfer Module (speeded up by 20 times). The module will use a combination of electric propulsion and multiple gravity assists at Earth, Venus and Mercury to carry BepiColombo’s two scientificorbiters – ESA’s Mercury Planetary Orbiter and Japan’s Mercury Magnetospheric Orbiter – to the innermost planet in our Solar System.
The test is designed to demonstrate that the mechanisms can reach their full steering range. The thruster mechanisms control the steering of the spacecraft during the long thrust arcs of the 7.2 year cruise to Mercury and as such are used for navigation, attitude control, and reaction wheel off-loading. Together with the onboard software, the mechanisms will update the direction of the thrust vector every five minutes relative to the spacecraft’s evolving centre of gravity. The thrusters will be fired for several months at a time between the gravity assist flybys.
This particular test was conducted in April 2017, before the spacecraft was put into the composite stack configuration. The same test will be repeated again later in the year to verify performance after the stack level vibration test campaign.”
“The high performance of ESA’s new generation ‘Planetary and Asteroid Natural scene Generation Utility’ or Pangu software enables real-time testing of both landing algorithms and hardware. Entry, descent and landing on a planetary body is an extremely risky move: decelerating from orbital velocities of multiple km per second down to zero, at just the right moment to put down softly on an unknown surface, while avoiding craters, boulders and other unpredictable hazards.
But Pangu can generate realistic images of planets and asteroids on a real-time basis, as if approaching a landing site during an actual mission. This allows the testing of landing algorithms, or dedicated microprocessors or entire landing cameras or other hardware ‘in the loop’ – plugged directly into the simulation – or run thousands of simulations one after the other on a ‘Monte Carlo’ basis, to test all eventualities.
Seen here is a Pangu recreation of the Mars Curiosity’s rover’s approach to Mars, using original telemetry, and then a view of Mars moon Phobos. This is followed by another recreation the Japanese Hayabusa probe’s encounter with the rubble-strewn Itokawa near-Earth asteroid, and finally a telemetry-based recreation of the field of view of the New Horizons mission as it performed its rapid flyby of Pluto.
This new generation of Pangu was developed for ESA by the University of Dundee in Scotland.”
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