T226 Best Practices and Exciting Discoveries in Identifying, Mapping, and Analyzing Planetary Landforms and Terrestrial Analogues
Wednesday, 12 October 2022
8:00 AM - 12:00 PM
501
FRACTURE MAPPING LAVA TUBES: COMPARING VISUAL VERSUS INFRARED DATA SETS
Paper number: T226-7
Program: Technical Sessions
Time: 9:20 AM – 9:35 AM
Authors
-
Danielle Wyrick Presenting AuthorSouthwest Research Institute Space Science Division, San Antonio, TX
-
Debra BuczkowskiJHU Applied Physics Laboratory, Laurel, MD
-
Wenlu ZhuUniversity of Maryland, College Park, MD
-
Casey BracciaUniversity of Maryland, College Park, MD
-
Edward WilliamsUniversity of Maryland, College Park, MD
Abstract
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).
Geological Society of America Abstracts with Programs. Vol. 54, No. 6
doi: 10.1130/abs/2022AM-382413
© Copyright 2022 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.