Dr. Angelo Vermeulen is a space systems researcher at Delft University of Technology in the Netherlands, where he explores advanced concepts for interstellar exploration. Over the past decade, he has collaborated closely with the European Space Agency's (ESA) MELiSSA program, developing concepts for bioregenerative life support systems for space. In such systems, a variety of microorganisms progressively break down human waste and the resulting compounds are harnessed by plants to produce oxygen and food for the crew.

Beyond his scientific pursuits, Dr Vermeulen is also an accomplished artist and a co-founder of the SEADS (Space Ecologies Art and Design) collective. SEADS creates artworks that seamlessly integrate concepts and technologies from a diverse array of scientific disciplines, including biology, neuroscience, computer science, and astrophysics.

He is the author of a recently published Frontiers in Astronomy and Space Sciences article in which he and his co-authors describe a new model that theoretically produces all required food and oxygen during long-duration and remote space missions, removing the necessity for resupply from Earth.

As the earthquake-strength Hydra shaker table simulates the vibration forces of a rocket launch for satellite testing, it is only this concrete block and the dampeners and springs supporting it that prevent the rest of the European Space Agency's ESTEC Test Center from also suffering the shakes.

The most powerful and precisely controllable of the shaker tables the ESA uses for satellite testing at its Test Center in Noordwijk, the Netherlands, is the multi-axis Hydra, which is capable of vibrating test items weighing many tons.

Seen from the cleanroom above, the hydraulically-powered Hydra appears to be simply a 5.5 x 5.5 m aluminum platform lying flush with the floor. But this plate is only the top of an 18 metric ton test table which is moveable using eight hydraulic actuators, in the same manner as a flight simulator machine.

This test table is enclosed within a 1,400 metric ton concrete 'seismic foundation' block. This block rests in turn on the set of springs and dampers, which isolate it, preventing potentially damaging vibrations from spreading through the rest of the building.

NASA's Lunar Trailblazer is nearing completion now that its second and final cutting-edge science instrument has been added to the small spacecraft. Built by the University of Oxford in England and contributed by the UK Space Agency, the Lunar Thermal Mapper (LTM) joins the High-resolution Volatiles and Minerals Moon Mapper (HVM3), which was integrated with the spacecraft late last year. Together, the instruments will enable scientists to determine the abundance, location, and form of the moon's water.

Led by Caltech in Pasadena, California, Lunar Trailblazer has a mass of about 440 pounds (200 kilograms) and measures only 11.5 feet (3.5 meters) wide with its solar panels fully deployed.

The upcoming XRISM (X-ray Imaging and Spectroscopy Mission, pronounced "crism") spacecraft will study the universe's hottest regions, largest structures, and objects with the strongest gravity.

Led by JAXA (Japan Aerospace Exploration Agency), XRISM will peer into these cosmic extremes using spectroscopy, the study of how light and matter interact. In this explainer, video producer Sophia Roberts from NASA's Goddard Space Flight Center walks us through how understanding spectroscopy deepens our knowledge of the universe.

"I think we all get excited for the beautiful images we get from missions like NASA's James Webb Space Telescope," Roberts said. "But after taking a deep dive into spectroscopy, I really appreciate the critical context it gives scientists about the story behind those pictures.