Definition
Protoplanetary disks (PPDs) surrounding young stars are short-lived (∼1–10 Myr), compact (∼10–1,000 AU) rotating reservoirs of gas and dust. Disks are believed to be the birthplaces of planetary systems, where tiny grains are assembled into pebbles, planetesimals, and eventually planets, asteroids, and comets. The evolution of gas and grain growth in disks is related to the redistribution and transport of angular momentum, which is thought to be governed by magnetohydrodynamical turbulence. The intense high-energy radiation from one or more young stars and strong spatial and temporal variations in the physical conditions (accretion rate, temperature, density, grain sizes) make a variety of chemical processes active in protoplanetary disks. In PPDs, simple molecules are rapidly produced in the gas phase via ion-molecule and neutral-neutral reactions. The more complex (organic) species in disks are slowly synthesized on and in the icy mantles of dust grains and later are...
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Semenov, D. (2015). Protoplanetary Disk, Chemistry. In: Gargaud, M., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-44185-5_1300
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