Researchers have developed a coordinate‑aware Mamba2 framework (CA‑Mamba2) for predicting the remaining useful life of lithium‑ion batteries. By integrating a coordinate feature attention network and a swiGLU‑gated residual network with the state‑space Mamba2 backbone, the model effectively captures both long‑term degradation trends and local fluctuation patterns. On the NASA, Tongji University, and Xi’an Jiaotong University datasets under single‑variable, multivariate, and cross‑dataset generalization settings, the model achieved mean absolute error values below 0.0098, 0.0016, and 0.0083, respectively, with superior computational efficiency and robustness across different prediction starting points.

Older adults living in homes with electrical or plumbing problems, insufficient space, or poor lighting are more likely to experience a fall, according to a new study published August 5, 2026 in the open access journal PLOS One by Javiera Cartagena-Farías of the London School of Economics and Political Science, UK, and colleagues.

SUMMARY: The U.S. National Science Foundation National Solar Observatory (NSF NSO) announced today a major breakthrough in solar physics. Using the world's most powerful solar telescope, the NSF Daniel K. Inouye Solar Telescope near the summit of Maui’s Haleakalā, combined with computer simulations, an international team of scientists from the NSO, NSF NCAR High Altitude Observatory (HAO), and the Max Planck Institute for Solar System Research (MPS) found the signature of Kelvin-Helmholtz instability (KHI), tiny swirling patterns like small whirlpools, on the Sun's surface. Researchers suggest that KHI might be a key reason why the Sun's outer atmosphere gets so hot, and why magnetic energy builds up and moves around on the Sun. Magnetic energy fuels solar flares and eruptions—the kind of solar activity that can send bursts of energy toward Earth and affect satellites, power grids, and other technology. The discovery opens a new window into the fundamental physics of the Sun and other stars while underscoring the unmatched capabilities of the Inouye Solar Telescope.

SAN ANTONIO — August 5, 2026 — A new study led by Southwest Research Institute (SwRI) provides evidence that liquid nitrogen is rising to Pluto’s surface through cracks in the northern edge of the Sputnik Planitia, part of the massive heart-shaped glacier on the dwarf planet’s surface. This is the first evidence of liquid recently flowing on Pluto. The study is based on data from NASA’s New Horizons spacecraft and is led by SwRI Associate Vice President Dr. Alan Stern, the principal investigator of the New Horizons mission.

The occurrence of fires in the Arctic is linked not only to warming temperatures and increasingly dry conditions, but also human activity in the region. An international research team led by the University of Zurich found that fires occurred 2.5 times more often in lit areas associated with human activity than in climatically similar unlit areas. Effective fire prevention and response can help reduce risks whose impacts extend far beyond the Arctic.

Physicists at the University of Würzburg and the Würzburg-Dresden Cluster of Excellence ctd.qmat have realized the world’s first continuously operating maser based on the semiconductor silicon carbide. This new technology could pave the way for compact microwave sources, low-noise amplifiers, and highly sensitive magnetic field sensors – and may even find future applications in space technology.

An international team of researchers has succeeded in producing atomic quantum gas mixtures with an unprecedented particle flux. In the journal Nature Communications, the scientists report on experiments conducted with the MAIUS-B apparatus, in which Bose-Einstein condensates consisting of two different atomic species – rubidium and potassium – were generated and studied under microgravity conditions in the Einstein Elevator at Leibniz University Hannover, Germany. A key contribution to this achievement came from a technological development at Johannes Gutenberg University Mainz: the highly sophisticated and compact optical system used to control the atoms.

In hub-filament systems, radially converging filaments are known to channel dense gas into hubs where massive stars form, but the contribution of inter-filamentary diffuse gas has remained unclear. In this study, researchers mapped gas motions in the Monoceros R2 star-forming region using carbon monoxide observations. They found that diffuse inter-filamentary gas not only flows directly toward the central hub but also replenishes dense filaments, substantially increasing the total gas reservoir available for massive star formation.