Research news on Interplanetary dust

Interplanetary dust as a research area focuses on the origin, composition, dynamics, and evolution of micron- to millimeter-sized solid particles distributed throughout the Solar System. Studies integrate in situ spacecraft measurements, zodiacal light observations, infrared and submillimeter astronomy, laboratory analysis of collected particles (e.g., micrometeorites), and dynamical modeling of dust production and transport. Key topics include dust sources (comets, asteroids, Kuiper Belt objects), Poynting–Robertson drag, radiation pressure, collisions, and interactions with the solar wind and planetary magnetospheres. This field constrains planetary system formation, surface weathering processes, and the distribution of organic and volatile materials in planetary environments.

Uranus's two outer rings show starkly different origins

Astronomers using the W. M. Keck Observatory on Maunakea, Hawaiʻi Island are revealing new insight into the composition and origins of Uranus's two outer rings. Using data from the Keck Observatory Archive (KOA), combined ...

The hidden danger of lunar micrometeoroid storms

The moon has no significant atmosphere, no weather, and no wind. Yet it faces an invisible bombardment more relentless than any terrestrial storm, a constant rain of micrometeoroids, tiny fragments of rock and metal traveling ...

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