With the accelerated advancement of lunar and Mars exploration programs, long-term human habitation on extraterrestrial bodies faces the severe challenge of extreme diurnal temperature variations. Phase change materials (PCMs), owing to their ability to store or release substantial latent heat during solid–liquid phase transitions while maintaining a nearly constant temperature, have become an ideal solution for space thermal control systems. However, in the microgravity environment of space, the ground-dominant natural convection tends to disappear, and thermocapillary convection may become the prevailing heat transfer mechanism; in low-gravity environments such as those on the Moon and Mars, the coexistence and competition between these two convective regimes remain unclear. Existing studies have predominantly focused on either Earth's gravity or pure microgravity conditions, with a notable scarcity of research on the coupled effects of thermocapillary and natural convection at intermediate gravity levels. The melting dynamics of two typical organic PCMs, succinonitrile and n-octadecane, under low-gravity conditions have not yet been systematically elucidated. Therefore, clarifying the roles of thermocapillary convection under varying gravity levels and container geometries holds significant engineering guidance for the design of efficient space thermal control systems.

Mars once had abundant liquid water, yet orbiters and rovers have found far less carbonate rock than expected for a planet that may have had a thick, carbon dioxide-rich atmosphere. A new geochemical modelling study led by Chang-Chin Wang, with Professor Tomohiro Usui at JAXA and the University of Tokyo, and Associate Professor Mohit Melwani Daswani at ELSI, shows that the type of rock water reacts with, not just water itself, controls whether calcium/iron-rich or magnesium-rich carbonates form. Feldspar-rich rocks, increasingly detected on the Martian surface, readily produce the calcium/iron-rich carbonates seen in many locations. The simulations also show how percolating groundwater could be quietly burying carbonates underground, helping explain their apparent scarcity on the surface.

With the advancement of long-term crewed deep-space exploration missions, the effects of the microgravity environment on astronauts' brain function have become an important topic in aerospace medicine. The disappearance of the hydrostatic pressure gradient during spaceflight induces cephalad fluid shifts, which can alter cerebral blood flow (CBF) and are closely associated with visual impairment, spatial disorientation, and cognitive decline. However, existing studies have predominantly focused on the steady-state phase during the middle and late stages of microgravity exposure, with insufficient understanding of the characteristics of CBF fluctuations during the early phase of postural transitions. Moreover, as an indicator of terminal perfusion in the cerebral microcirculation, the coupling relationship between CBF and the upstream hemodynamics of the internal carotid and vertebral arteries has not been systematically investigated. In addition, magnetic resonance imaging (MRI) cannot be applied in real time during spaceflight due to its bulky equipment, whereas ultrasound offers the advantages of portability, real-time capability, and radiation-free operation. Therefore, elucidating the association between early macrovascular hemodynamic changes under simulated microgravity and regional CBF alterations, and evaluating the feasibility of using ultrasound parameters as portable predictors of CBF, holds significant scientific importance and application value.

With the increasing scale of space infrastructure such as large space telescopes, antenna arrays, and solar power stations, the payload fairing size of launch vehicles has become a critical bottleneck constraining their development. On-orbit autonomous assembly via deployable modules has emerged as an important technical approach to overcome this limitation. Deployable modules typically exhibit high packaging ratios; however, the geometric deviations caused by residual strain, assembly tolerances, and dynamic coupling effects after deployment can significantly affect docking accuracy and structural stability, and may even lead to assembly failure. Nevertheless, existing studies have mostly focused on post-deployment final configuration accuracy optimization, with insufficient attention paid to the cooperative strategies between real-time deformation control and motion control during the assembly process. Moreover, a dynamic modeling method capable of accurately describing the coupling between variable-length flexible components and rigid bodies is still lacking. Therefore, how to achieve active configuration correction and coordinated position–attitude control of deployable modules on orbit has become a key challenge in the autonomous assembly of large space structures.

Want to cut reliance on Earth supplies for Mars colonies? A new Engineering review explores mild-temperature CO₂ conversion tech ECO2R, a lighter, stabler alternative to NASA’s high-heat MOXIE oxygen generator. It turns Mars’ thick carbon dioxide atmosphere into rocket fuel and breathable oxygen via tailored electrodes and catalysts. Researchers also use CFD simulations and machine learning to fix space-specific hurdles like microgravity mass transport, mapping step-by-step plans to build fully self-sustaining Martian habitats down the line.

Dr. Deanna Kennedy of the Department of Kinesiology and Sport Management and Drs. Ana Diaz Artiles and Bonnie Dunbar from the Department of Aerospace Engineering have partnered to investigate how differences in gravity influence coordination and movement control. Their latest work looks into how the body performs in altered gravity conditions to identify challenges astronauts encounter in space and how the human body adapts when environmental surroundings shift.

“On Earth, we spend our entire lives moving in a 1G environment, where the gravitational force feels natural,” Kennedy said. “But when that changes, the way our body controls movement changes too and understanding that helps us predict where performance may begin to break down.”