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Globular clusters are relics of the early Universe and they hold clues tomany aspects of stellar and galactic evolution. We propose to point the RomanSpace Telescope at one or more clusters either as a part of or as an extensionof the Galactic Bulge Time Domain Survey. This would provide a uniqueopportunity to apply the powerful toolkit of asteroseismology to a globularcluster, an observation that is largely out of reach for any other time-domainphotometric missions. In this white paper we present the possible targets inthe vicinity of the notional survey fields. Potential science cases includeprecise determination of stellar parameters throughout the cluster, accurateestimation of the integrated mass loss for metal-poor and metal-rich clusters,asteroseismic analysis and mass estimation for RR Lyrae stars, anddetermination of the seismic ages of clusters. We provide comparisons withother photometric missions and recommendations for maximizing the scientificreturn from a dedicated globular cluster observing run.

Asteroseismic sounding of bulge globular clusters with the Roman Space Telescope