Solar Neutrino Detection with the nEXO Experiment

nEXO aims to employ a 5-tonne liquid xenon time projection chamber enriched to 90% in ¹³⁶Xe. Thanks to recent observations of long-lived excited ¹³⁶Cs states, the nEXO detector has the potential to serve as a solar neutrino observatory in addition to its primary goal of neutrino-less double beta decay detection. In this talk, I will discuss the projected capabilities of nEXO to use charged-current (ν_e, ¹³⁶Xe) interactions to measure the CNO and pep solar-neutrino fluxes, as well as the energy of the ⁷Be solar-neutrinos. I will also contextualize the expected results of these measurements relative to the current measurements made by the Borexino and KamLAND collaborations.