Solid State Astrochemistry

The fundamentals of astrochemistry in the gas phase are relatively well established, in contrast to the special relevance attributed to processes involving interstellar dust grains - the solid component of matter diffused among the stars.
This book presents the state of the art in relation to the ways grains interact with gases, the catalytic role played by dust that allows key molecular species (H2 as well as many complex, possibly prebiotic species) to be formed on its surface - which cannot be obtained efficiently by any other mechanisms, and the interaction between solids (dust grains, icy mantles, cometary nuclei, satellites of the giant planets and minor bodies in the Solar system) in space and energetic agents such as UV photons and fast particles.
The presence and importance of PAH, which may represent the smallest component of the grains, is considered in relation to possible astrobiological pathways and the ever-present mystery of the ubiquitous presence of Diffuse Interstellar Bands and their carriers.

The astrochemical interaction of interstellar dust grains (the "solid component of matter diffused among the stars") with other grains and with gases in stars and interstellar clouds was the subject of the fifth course of the International School of Space Chemistry held in June of 2000. Fifteen papers from the gathering are presented here by Krelowski (Center for Astronomy, N. Copernicus U., Poland) and his colleagues Pirronello and Manic<`o> (both of DMFCI Università di Catania, Italy). Among the topics discussed are a review of the cosmic silicates, the identification of diffuse band carriers, chemical reactions on solid surfaces of astrophysical interest, ice chemistry in space, ion interactions with solids, trans-Neptunian objects, and a model of the chemical composition of Halley dust particles. Annotation ©2004 Book News, Inc., Portland, OR