T207 The Big Picture from Small Worlds: Dwarf Planets, Trans-Neptunian Objects, Asteroids, Comets, and More

Thursday, 29 October 2020
1:30 PM - 5:30 PM
Meeting Rooms

PIXELS AND PINGOS: UTILIZING COMPUTER VISION TO DETECT PINGOS ON EARTH, MARS, AND CERES

Paper number: T207-17
Program: Technical Sessions
Time: 5:02 PM – 5:12 PM

Authors

Abstract

Pingos are mound-like structures formed through the freezing of groundwater under specific periglacial hydrological conditions [1]. These dynamic water-based systems are of interest on other planetary bodies due to the implications of the existence of subsurface water ice resources. On Earth, these features are found in Canada, Alaska, Russia, and elsewhere where the necessary conditions exist. Similar landforms have been documented on Mars on Utopia Planitia [e.g. 2 & 3], and recent high-resolution images from NASA’s Dawn spacecraft revealed pingo-like morphologies on the dwarf planet Ceres in Occator and Urvara craters [4,5]. These potential hydrological systems on Mars and Ceres may be, or could have been, important habitats for life or nexus for pre-biotic chemistry. Additionally, identifying and characterizing the water resource potential of possible extraterrestrial pingos is relevant for future human space exploration.

This project is a combined effort between manually identifying potential pingo features on Earth, Mars, and Ceres, and developing a computational pipeline that can identify these features to a level of accuracy similar to human identification using computer vision and machine learning techniques. We examined these features on Earth on the Tuktoyaktuk peninsula at a scale of 1:10,000, on Mars within Utopia Planitia at a scale of 1:2,500, and on Ceres within Occator Crater at a scale of 1:10,000. Earth and Ceres imagery are both at a resolution of ~3m/pixel and Mars imagery is ~1m/pixel. Manually mapping these features allowed us to then check our code output for accuracy.

Currently, preliminary maps of pingo features on Mars, Ceres, and Earth have been completed manually. A code has been developed that successfully identifies pingo features on Earth with a high degree of accuracy and will be used to help map potential pingo-like features on Mars and Ceres.

References: [1] Mackay J. R. (1998) Geo. Phys et Quart., 52, 271-323. [2] Dundas C. M. & McEwen A. S. (2010) Icarus, 205, 244-258. [3] Soare R. J. et al. (2019) Icarus, in press. [4] Schmidt B. E. et al. (Accepted) Nat. Geo. [5] Hughson K. H. G. et al. (2020) LPSC LI.

Acknowledgments: Planet Team (2017). Planet Application Program Interface: In Space for Life on Earth., the Dawn Data Archive on the PDS SmallBodies Node, Mars HiRISE on the PDS Mars

Geological Society of America Abstracts with Programs. Vol. 52, No. 6

doi: 10.1130/abs/2020AM-358719

© Copyright 2020 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.