
Copernical Team
Winchcombe meteorite is helping us to understand more about asteroids

Viasat receives $80M for Multi-Function AESAs across warfighting domains

Lockheed Martin opens facility for rapid development of small satellites

Impulse Space secures $45M in Series A Funding Round

DARPA seeks solutions to preserve bio-samples without cold storage

Lockheed Martin's NGI program completes all subsystem PDRs

Mars once had wet-dry climate conducive to supporting life: study

Russian cosmonauts perform spacewalk to attach debris shields to space station

Hera’s mini-radar will probe asteroid’s heart

The smallest radar to fly in space has been delivered to ESA for integration aboard the miniature Juventas CubeSat, part of ESA’s Hera mission for planetary defence. The radar will perform the first radar imaging of an asteroid, peering deep beneath the surface of Dimorphos – the Great Pyramid-sized body whose orbit was shifted last year by the impact of NASA’s DART spacecraft.
Video: The universe in a box: Preparing for Euclid's survey

ESA's Euclid mission will create a 3D-map of the universe that scientists will use to measure the properties of dark energy and dark matter and uncover the nature of these mysterious components. The map will contain a vast amount of data, it will cover more than a third of the sky and its third dimension will represent time spanning 10 billion years of cosmic history.
But dealing with the huge and detailed set of novel data that Euclid observations will produce is not an easy task. To prepare for this, scientists in the Euclid Consortium have developed one of the most accurate and comprehensive computer simulations of the large-scale structure of the universe ever produced. They named this the Euclid Flagship simulation.
Running on large banks of advanced processors, computer simulations provide a unique laboratory to model the formation and evolution of large-scale structures in the universe, such as galaxies, galaxy clusters, and the filamentary cosmic web they form. These state-of-the-art computational techniques allow astrophysicists to trace the motion and behavior of an extremely large number of dark-matter particles over cosmological volumes under the influence of their own gravitational pull.