We present results from a shape-based, rotationally-resolved thermophysical model of near-Earth asteroid (433) Eros, using reflected and near-IR spectra collected at the NASA Infrared Telescope Facility (IRTF) over 18 nights (25 disk-integrated in total) 2009 to 2019. The data sample variety viewing geometries, illumination angles, rotational phases therefore allow us characterize Eros's surfac...