Chemical and Isotopic Evolution of the Solar Nebula and Protoplanetary Disks

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Protoplanetary Disks, Proto-Solar Nebula, Molecules, Chemistry, Gas-Phase, Reactions, Line Emission, Planet Formation, Interferometry, Spectroscopy, Radiative Transfer, Chemical Networks

Scientific paper

In this chapter we review recent advances in our understanding of the chemical and isotopic evolution of protoplanetary disks and the solar nebula. Current observational and meteoritic constraints on physical conditions and chemical composition of gas and dust in these systems are presented. A variety of chemical and photochemical processes that occur in planet-forming zones and beyond, in both gas phase and on grain surfaces, are overviewed. The discussion is based upon radio-interferometric, meteoritic, space-born, and laboratory-based observations,measurements and theories. Linkage between cosmochemical and astrochemical data are presented, and interesting research puzzles are discussed.

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