The 46th COSPAR Scientific Assembly brought together experts from astronomy, the satellite industry, policy and law to examine one of the most important challenges arising from the rapid growth of activities in space: how to preserve dark and quiet skies while enabling satellite systems to continue delivering valuable services to society. The meeting was chaired by Marco Tavani. 

Narrow jets of luminous matter may be emitted towards Earth from the nuclei of active galaxies, billions of light-years away. The galaxy then appears as a point source and is called a blazar. A Polish-German team of scientists has, for the first time, analysed the activity of one such blazar over a long period of time and instead of finding answers, they have been faced with an ever-increasing number of intriguing questions.

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.

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.