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Laboratory Experiments on Carbonaceous and Silicate Materials

Published online by Cambridge University Press:  27 February 2018

L. Colangeli ,
V. Mennella ,
A. Rotundi ,
E. Bussoletti  and
P. Palumbo
L. Colangeli
Affiliation:
Astronomical Observatory of Capodimonte, Via Moiariello 16, 80131 Napoli (Italy)
V. Mennella
Affiliation:
Astronomical Observatory of Capodimonte, Via Moiariello 16, 80131 Napoli (Italy)
A. Rotundi
Affiliation:
Astronomical Observatory of Capodimonte, Via Moiariello 16, 80131 Napoli (Italy)
E. Bussoletti
Affiliation:
Istituto Universitario Navale, Via A. De Gasperi 5, 80133 Napoli (Italy)
P. Palumbo
Affiliation:
Istituto Universitario Navale, Via A. De Gasperi 5, 80133 Napoli (Italy)

Abstract

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Ground-based, remote and “in situ” observations show that dust plays an important role in the evolution of interstellar, circumstellar and interplanetary media. Despite the wealth of available astronomical data, a main item to be clarified concerns the actual chemico-physical composition of cosmic dust. A correct interpretation of observations must rely on a systematic comparison with results coming from laboratory simulations. In this paper we present an overview of recent results, obtained in our laboratory, on various forms of carbon-based and silicate grains of possible astrophysical interest.

Type
XII. Physical Processes and Laboratory Analyses
Information
International Astronomical Union Colloquium , Volume 150: Physics, Chemistry and Dynamics of Interplanetary Dust , 1996 , pp. 463 - 468
Copyright
Copyright © Astronomical Society of the Pacific 1996

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