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Dust is formed in stars and is then blown off in a slow wind or a massive star explosion. The dust is then 'recycled' in the clouds of gas between stars and some of it is consumed when the next generation of stars begins to form.
Cosmic dust traces a wide range of physical and chemical processes, ranging from the solar system to the high-redshift universe. Infrared and millimeter radiation from dust grains has served as the best tool to detect and characterize structures from proto-planetary discs around nearby brown dwarfs to distant quasars.
When a star dies, it sheds clouds of gas in strong stellar winds or in an explosion called a supernova. As the gas cools, minerals condense. Observations by our SOFIA mission suggest that in the wake of a supernova shockwave, dust may form more rapidly than scientists previously thought.
Cosmic dust consists of tiny particles of solid material floating around in the space between the stars. It is not the same as the dust you find in your house but more like smoke with small particles varying from collections of just a few molecules to grains of 0.1 mm in size.
Also called cosmic dust, a fleck of space dust is usually smaller than a grain of sand and is made of rock, ice, minerals, or organic compounds. Scientists can study cosmic dust to learn about how it formed and how the universe recycles material.
Cosmic dust can be divided in two categories: interstellar dust (ISD) — 'visible' as the dust blocking the light of the stars of the milky way — and interplanetary dust particles (IDPs) — visible as the zodiacal light, which is sunlight, scattered by interplanetary dust particles.
It's true that: about 86 per cent of our mass is “stardust”; almost certainly we each carry at least a few million atoms of gold inside us; and yes, the carbon atoms we carry are mostly many billions of years old.
In addition, cosmic dust particles are some of nature's most powerful detectors of electric and magnetic fields throughout the universe. For example, cosmic dust particles close to the center of the Milky Way's massive black hole are charged and align perpendicularly to the galaxy's magnetic field lines.

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Cosmic Dust – Near & Far 2008 is a scientific report or publication that discusses the origins, properties, and significance of cosmic dust both from nearby and distant astronomical sources.
Researchers, scientists, and institutions involved in studies of cosmic dust are typically required to file Cosmic Dust – Near & Far 2008, especially those who contribute new findings or data.
To fill out Cosmic Dust – Near & Far 2008, one must follow the guidelines provided in the publication, ensuring to include all relevant data, methodologies, and findings accurately.
The purpose of Cosmic Dust – Near & Far 2008 is to compile and disseminate research findings on cosmic dust to advance our understanding of its role in the universe.
Information that must be reported on Cosmic Dust – Near & Far 2008 includes observational data, analyses of dust composition, implications for astrophysics, and any new discoveries related to cosmic dust.
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