New observation method improves outlook for lithium metal battery
Peer-Reviewed Publication
In honor of Global Astronomy Month, we’re exploring the science of space. Learn how astronomy connects us through curiosity, discovery, and a shared wonder for what lies beyond.
Updates every hour. Last Updated: 27-Oct-2025 20:11 ET (28-Oct-2025 00:11 GMT/UTC)
Recently, a research team led by Prof. XU Yigang and Prof. LIN Mang from the Guangzhou Institute of Geochemistry of the Chinese Academy of Sciences identified seven olivine-bearing clasts from two grams of lunar regolith returned by the Chang'e-6 mission. Their findings were published in Proceedings of the National Academy of Sciences (PNAS) on Oct. 20.
The ability to get detailed views of distant objects in space is limited by the telescope size, so the sharpest details are usually obtained by linking telescopes together. A UCLA-led team of astronomers has used a device called a photonic lantern on a single telescope to get the most detailed view yet of star beta Canis Minoris. The photonic lantern splits light collected by the telescope into multiple channels based on spatial “mode,” then computational techniques are used to reconstruct a high-resolution image from the photonic lantern outputs. The new approach to imaging will allow astronomers and astrophysicists to view objects that are smaller and more distant than ever before, unlocking answers to some mysteries.
Researchers discovered a previously unknown solar radio pattern — periodic beaded stripes — using the Chashan Broadband Solar Radio Spectrometer during a 2024 flare. These narrow, drifting radio bands, dotted with rhythmic “beads”, reveal rapid plasma processes in the Sun’s corona. The team attributes their formation to the double plasma resonance effect, modulated by magnetohydrodynamic waves. Observations suggest a weak magnetic field (~1 G) above the flaring loops in an active solar region.
The National Institute of Information and Communications Technology (NICT) and the Nagoya Institute of Technology (NITech), collaborated with the Japan Aerospace Exploration Agency (JAXA), have achieved the world’s first successful demonstration of next-generation error correction codes, mitigating the impact of atmospheric turbulence on ground-to-satellite laser communications.
Atmospheric turbulence in ground-to-satellite laser links is known to cause fading, resulting in burst data errors. Error correction codes are one of the key technologies to mitigate such effects. In this experiment, we transmitted next-generation error correction codes with high correction capability (5G NR LDPC and DVB-S2) and successfully corrected burst data errors caused by atmospheric turbulence in the laser link. This result confirmed that both codes can significantly improve communication quality compared to conventional schemes.
This achievement is expected to contribute to the practical implementation of ground-to-satellite laser communications by applying these codes.