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.

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 ...

How to watch the Orionid meteor shower, debris of Halley's comet

The Orionids—one of two major meteor showers caused by remnants from Halley's comet—will peak with the arrival of a new moon, providing an excellent opportunity to see shooting stars without interference from moonlight.

No collision, no life: Earth probably needed supplies from space

Earth is so far the only known planet on which life exists—with liquid water and a stable atmosphere. However, the conditions were not conducive to life when it formed. The gas-dust cloud from which all the planets in the ...

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