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Laboratory Astrophysics of Cosmic Dust Analogues

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Astromineralogy

Part of the book series: Lecture Notes in Physics ((LNP,volume 815))

Abstract

In this chapter, the main techniques for producing and characterizing cosmic dust analogues in the laboratory will be discussed. It will be shown how optical data of astronomically relevant materials can be measured and how such data can be applied to interpret astronomical spectra. The identification of minerals in space from infrared spectroscopy will be summarized.

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Acknowledgement

I thank my collaborators from the Jena Laboratory Astrophysics Group for many discussions about cosmic dust analogues and Drs. J. Dorschner, J. Gürtler, and H. Mutschke for critically reading of the paper.

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Correspondence to T. Henning .

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Henning, T. (2010). Laboratory Astrophysics of Cosmic Dust Analogues. In: Henning, T. (eds) Astromineralogy. Lecture Notes in Physics, vol 815. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-13259-9_8

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  • DOI: https://doi.org/10.1007/978-3-642-13259-9_8

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