Abstract
We consider the chemistry occurring in protoplanetary disks and its possible contribution to the organic inventory of primitive solar system bodies. First, we outline the main physical and chemical processes associated with the formation of solar-type stars and their accretion disks. We then summarise the current observational status of protoplanetary disks and review chemical models of them. Finally, we discuss possible signatures of nebular chemistry in primitive organic material, paying particular attention to those related to isotope fractionation in comets and meteorites.
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Markwickan, A., Charnley, S. (2004). Chemistry of Protoplanetary Disks. In: Ehrenfreund, P., et al. Astrobiology: Future Perspectives. Astrophysics and Space Science Library, vol 305. Springer, Dordrecht. https://doi.org/10.1007/1-4020-2305-7_3
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