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The Model of Chemical Composition of Halley Dust Particles

  • Conference paper
Book cover Solid State Astrochemistry

Part of the book series: NATO Science Series ((NAII,volume 120))

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Abstract

In this short paper we present a quick view of the composition of the nucleus of comet Halley deduced by the analysis of the dust particles detected by VEGA and GIOTTO spacecraft.

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References

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Author information

Authors and Affiliations

  1. Space Research Institute Russian Academy of Sciences, Moscow, Russia

    B. M. Andreichikov & G. G. Dolnikov

  2. Institute of Ore Deposits, Petrography, Mineralogy and Geochemistry Russian Academy of Sciences, Moscow, Russia

    Yu. P. Dikov

Authors
  1. B. M. Andreichikov
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  2. G. G. Dolnikov
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  3. Yu. P. Dikov
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Editor information

Editors and Affiliations

  1. DMFCI Università di Catania, Catania, Sicily, Italy

    Valerio Pirronello  & Giulio Manicò  & 

  2. Center for Astronomy, N. Copernicus University, Torun, Poland

    Jacek Krelowski

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© 2003 Springer Science+Business Media Dordrecht

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Andreichikov, B.M., Dolnikov, G.G., Dikov, Y.P. (2003). The Model of Chemical Composition of Halley Dust Particles. In: Pirronello, V., Krelowski, J., Manicò, G. (eds) Solid State Astrochemistry. NATO Science Series, vol 120. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0062-8_15

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  • DOI: https://doi.org/10.1007/978-94-010-0062-8_15

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-1-4020-1559-5

  • Online ISBN: 978-94-010-0062-8

  • eBook Packages: Springer Book Archive

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