Abstract: Analysis of Lunar Boulder Tracks: Implications for Trafficability of Pyroclastic Deposits and Permanently Shadowed Regions (AGU Fall Meeting 2018)

Analysis of Lunar Boulder Tracks: Implications for Trafficability of Pyroclastic Deposits and Permanently Shadowed Regions

Valentin Tertius Bickel^1,2, Casey I Honniball³, Sabrina Martinez⁴, Alexander Rogaski⁵, Hannah M. Sargeant⁶, Samantha K. Bell⁷, Ellen Czaplinski⁸, Benjamin E. Farrant⁷, Elise Michelle Harrington⁹, Gavin D. Tolometti⁹ and David A Kring^10,11, (1)University of Bern, Center for Space and Habitability, Bern, Switzerland, (2)ETH Zurich, Geological Institute, Zurich, Switzerland, (3)University of Hawaii at Manoa, Honolulu, HI, United States, (4)Tulane University of Louisiana, New Orleans, United States, (5)South Dakota School of Mines and Technology, Rapid City, SD, United States, (6)Open University, Milton Keynes, United Kingdom, (7)University of Manchester, Manchester, United Kingdom, (8)Honeybee Robotics, Pasadena, United States, (9)University of Western Ontario, London, Canada, (10)Lunar and Planetary Institute, Houston, TX, United States, (11)Center for Lunar Science and Exploration, Houston, United States

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