The Dawn of Dust Astronomy

@article{Grun2019TheDO,
  title={The Dawn of Dust Astronomy},
  author={Eberhard Grun and Harald Kruger and Ralf Srama},
  journal={Space Science Reviews},
  year={2019}
}
We review the development of dust science from the first ground-based astronomical observations of dust in space to compositional analysis of individual dust particles and their source objects. A multitude of observational techniques is available for the scientific study of space dust: from meteors and interplanetary dust particles collected in the upper atmosphere to dust analyzed in situ or returned to Earth. In situ dust detectors have been developed from simple dust impact detectors… 
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References

SHOWING 1-10 OF 341 REFERENCES
2002 Kuiper prize lecture: Dust Astronomy
Interplanetary Dust, Meteoroids, Meteors and Meteorites
Interplanetary dust particles and meteoroids mostly originate from comets and asteroids. Understanding their distribution in the Solar system, their dynamical behavior and their properties, sheds
Dust Near The Sun
We review the current knowledge and understanding of dust in the inner solar system. The major sources of the dust population in the inner solar system are comets and asteroids, but the relative
Evidence for interstellar origin of seven dust particles collected by the Stardust spacecraft
TLDR
Seven particles captured by the Stardust Interstellar Dust Collector and returned to Earth for laboratory analysis have features consistent with an origin in the contemporary interstellar dust stream, and are diverse in elemental composition, crystal structure, and size.
The Galileo Dust Detector
The Galileo Dust Detector is intended to provide direct observations of dust grains with masses between 10-19 and 10-9 kg in interplanetary space and in the Jovian system, to investigate their
The flow of interstellar dust into the solar system
Context. Interstellar dust (ISD) is a major component in the formation and evolution of stars, stellar systems, and planets. Astronomical observations of interstellar extinction and polarization, and
Recent Origin of the Solar System Dust Bands
Infrared Astronomical Satellite (IRAS) observations in 1983 revealed the existence of several solar system dust bands. These dust bands are believed to be debris produced by recent disruption events
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