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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

References

Blanco, A., Bussoletti, E., Colangeli, L., Fonti, S., Orofino, V., & Stephens, J. R. 1991, in Origin and Evolution of Interplanetary Dust, Levasseur-Regourd, A. C. & H. Hasegawa, Dordrecht: Kluwer, 125Google Scholar
Buss, R.H., Lamers, H., & Snow, T.P. 1989, ApJ, 347, 977 Google Scholar
Bussoletti, E., Colangeli, L., & Mennella, V. Eds. 1995, Planet Spa. Sci., Vol. 43.Google Scholar
Colangeli, L., Mennella, V., Palumbo, P., Rotundi, A., & Bussoletti, E. 1995, A&AS, 113, 561 Google Scholar
Fitzpatrick, E. L., & Massa, D. 1988, ApJ, 328, 734 Google Scholar
Hanner, M. S., Lynch, D. K., & Russell, R. W. 1994, ApJ, 425, 274 Google Scholar
Hanner, M. S., Brooke, T. Y., & Tokunanga, A. T. 1995, ApJ, 438, 250 Google Scholar
V., Mennella, Colangeli, L., Blanco, A., Bussoletti, E., Fonti, S., Palumbo, P., & Mertins, H. C. 1995a, ApJ, 444, 288Google Scholar
Mennella, V., , Colangeli, L., Bussoletti, E., Monaco, G., Palumbo, P., & Rotundi, A. 1995b ApJS, 100, 149Google Scholar
Stephens, J. R., Blanco, A., Bussoletti, E., Colangeli, L., Fonti, S., Mennella, V., & Orofino, V. 1995, Planet Spa. Sci, 43, in pressGoogle Scholar
Tokunaga, A. T., & Brooke, T. Y. 1990, Icarus, 86, 208 Google Scholar