FRACTURE MAPPING LAVA TUBES: COMPARING VISUAL VERSUS INFRARED DATA SETS
Comparisons with in situ fracture mapping within the lava tube are ongoing. However, several observations were apparent between the visual and thermal cameras. Visual imagery is useful where there has been prior mineralization events, as the vein minerals are typically a different color than the surrounding basaltic host rock. Similarly, wet or large aperture fractures are often apparent in visual imagery. However, not all small or hairline fractures were easily identified. Also, visual imagery required a significant amount of light aimed at the cave wall to capture data. Infrared camera data shows that fractures can be seen in some of the thermal imagery. In particular, wet or large aperture fractures are often warmer than the surrounding rock. This effect was most notable close to the cave entrance, with the effect diminishing with depth into the lava tube. This is likely an effect of temperature homogenization within the cave, creating similar temperatures for the walls, air and water. Additionally, the resolution of the thermal imagery is coarser than the visual. However, the thermal data provided valuable information regarding which fractures were conducive and currently permeable by highlighting temperature differences of fractures with air or water flowing through them. This work was funded by the NASA GEODES project (N. Schmerr [UMD], PI).