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One of the primary mechanisms for inferring the dynamical history of planetsin our Solar System and in exoplanetary systems is through observation ofelemental ratios (i.e. C/O). The ability to effectively use these observationsrelies critically on a robust understanding of the chemistry and evolutionaryhistory of the observed abundances. Significant efforts have been devoted tothis area from within astrochemistry circles, and these efforts should besupported going forward by the larger exoplanetary science community. Inaddition, the construction of a next-generation radio interferometer will berequired to test many of these predictive models in situ, while simultaneouslyproviding the resolution necessary to pinpoint the location of planets information.

Science with an ngVLA: Observing the Effects of Chemistry on Exoplanets and Planet Formation