Mapping Titan's surface features within the visible spectrum via Cassini VIMS

► Global surface mapping of Titan using visible wavelength channels from Cassini VIMS. ► Methane windows at 0.637, 0.681, 0.754, 0.827, 0.937, and 1.046μm. ► The first global surface reflectance maps of Titan shortward of 0.938μm. ► We employ an empirically derived algorithm to remove haze layers from Titan.