
Copernical Team
A touch of sun heats up material scieces at ESTEC

NASA orders satellite container and trolley from RUAG Space

Exercise bike in space helps keep crew fit

Homemade spacesuits ensure safety of Chinese astronauts in space

Thousands of galaxies classified in a blink of an eye

New clues to why there's so little antimatter in the universe

Billionaire Blastoff: Rich riding own rockets into space

LHAASO measures Crab Nebula brightness, yields new UHE gamma-ray standard

The Large High Altitude Air Shower Observatory (LHAASO), one of China's key national science and technology infrastructure facilities, has accurately measured the brightness over 3.5 orders of magnitude of the standard candle in high-energy astronomy, thus calibrating a new standard for ultra-high-energy (UHE) gamma-ray sources. The standard candle is the famous Crab Nebula, which evolved from the "guest star" recorded by the imperial astronomers of China's Song Dynasty.
LHAASO has also discovered a photon with an energy of 1.1 PeV (1 PeV = one quadrillion electronvolts), indicating the presence of an extremely powerful electron accelerator—about one-tenth the size of the solar system—located in the core region of the Crab Nebula. The accelerator can energize electrons to a level 20,000 times greater than what CERN's Large Electron-Positron Collider (LEP) can ever achieve, thus approaching the absolute theoretical limit posed by classical electrodynamics and ideal magnetohydrodynamics.
Meet the open-source software powering NASA's Ingenuity Mars Helicopter

When NASA's Ingenuity Mars Helicopter hovered above the Red Planet April 19 on its maiden voyage, the moment was hailed as the first instance of powered, controlled flight on another planet. Figuring out how to fly on Mars, where the air is thin but gravity is about a third of that on Earth, took years of work. Along with the challenge of developing a craft that was up to the task, the mission needed software to make the unprecedented flights possible.
Image: Protecting the Meteosat Third Generation–Imaging satellite from the sun

From ESA's Materials and Electrical Components Laboratory—one of a suite of labs based at the ESTEC technical center in Noordwijk, the Netherlands—a view from an intricate test campaign for the next generation of European weather satellites.
The near infrared detector assembly of the Flexible Combined Instrument (FCI) imager aboard the Meteosat Third Generation—Imaging (MTG—I) satellite was found to be susceptible to unwanted "stray light" from the sun.
A solution was proposed to reduce this vulnerability: a very thin metal mask would be glued atop the assembly, with carefully designed slits that would allow light to penetrate only in the desired areas, minimizing the entry of stray light.
But the feasibility of this solution needed to be tested, in order to demonstrate if the alloy cover would remain securely in place as incoming direct sunlight heats it up repeatedly during moments of sun intrusion.
Accordingly, a new feature was added to the Electrostatic Discharge (ESD) facility, part of the Materials and Electrical Components Lab. Originally designed as a vacuum chamber to expose samples to mono-energetic electrons down to cryogenic temperature, the ESD was upgraded to host an optical rack to hold a light source to simulate sunlight exposure onto the sample.