The organic landscape of Saturn's moon Titan has the potential to host a plethora of solution caves and other access points into the subsurface resulting from karstic dissolution. When combined with the other speleogenic processes found on icy worlds (cryovolcanism, diapirism, and fissure formation), this makes Titan one of the best places in the solar system for planetary cave exploration. For Titan, subsurface access points, or SAPs (we use this term in lieu of "cave entrance" as the latter presupposes a cave actually exists), represent potential entrances to the subsurface that permit surface organics to be transported deeper into the interior, whether as solution or as suspended insoluble materials. For the purposes of our discussion, we are using the concept of subsurface access points (SAPs) provided by Wynne, Mylroie, et al. (2022) to imply remotely sensed features, that may or may not be connected to a subsurface void or cave, and thus potentially provide access to the subsurface of a planetary body. However, dissolution and transport of fluids to the subsurface occurs at a much smaller scale than what can be resolved via current remote sensing capabilities. Fissures, cracks, joints, and interconnected pore spaces <1 cm in size may be driving these processes at the micro-scale. These "microcaverns" (see Howarth, 1983) allow both dissolved and suspended insoluble organic materials access into the subsurface, a potential first step in delivering atmospherically-derived surface organics to warmer habitable zones in the deep ice, or possibly even into the subsurface ocean tens of kilometers below. While these features would be well below the resolution limit of current imaging of Titan's surface, we can nonetheless infer the existence of SAPs based on larger-scale phenomena associated with smaller conduit structures, such as volcanic edifices and inference of closed valleys suggesting transport of fluids and materials into the subsurface. Our work will inventory the locations where features of this size and larger could exist on Titan's surface and will detail the types of secondary mineralizations that could occur within these features.Titan is an ocean world with an icy crust covered with organic molecules. The thickness of the organic coating varies from location to location, with evidence of a 500 m thick layer in some areas, while other areas have little