Mitusov, Andrey V. and Stark, Alexander and Khrisanov, Vladislav R. and Oberst, Jürgen (2023) Hidden morphology of Shackleton Crater, lunar South Pole. Planetary and Space Science, 238, p. 105795. Elsevier. doi: 10.1016/j.pss.2023.105795. ISSN 0032-0633.
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Official URL: https://www.sciencedirect.com/science/article/abs/pii/S0032063323001642
Abstract
The article's goal is the detailed description of geomorphologic structures on the floor and interior walls of Shackleton Crater and a reconstruction of their formation histories. A Digital Elevation Model (DEM) with 20 m grid was constructed for the area around the crater based on Lunar Orbiter Laser Altimeter (LOLA) data. The DEM was analysed for slope steepness, Maximal Catchment Area (MCA) and four curvatures: maximal (kmax), minimal (kmin), horizontal (kh) and vertical (kv). Using this extensive set of Morphometric Variables (MVs) for the first time for a detail lunar DEM revealed unknown structures in permanently shaded areas. The previously identified large elevated structures “A" and “C" are attributed to landslides. “A" is related to a relatively large meteoroid impact that produced a recognisable crater on the exterior slope of Shackleton. “C" is associated with a landslide scar affecting the rim of Shackleton Crater directly above it. Structure “B” is not related to landsliding, but without of additional high-resolution geophysical data, its origin remains unclear. The low number of small impact craters on the steep slopes and sediment fields indicates ongoing surface erosion due to migration of unconsolidated fine grains and their deposition downslope. The foot slope zone is characterised by multiple accumulations of debris flows in the form of thin strips, identified as local landforms with kh > 0. On the surface of elevated structures “A”, “B” and “C” the map of kh reveals tree-like structures – erosion forms previously unknown in lunar geomorphology. These structures are formed by branching spurs characterised by several orders. The spurs are located relatively perpendicularly to the altitude isolines. The thickest (up to 120 m) slope deposits form a relatively flat area between the elevated structure “B" and the crater wall. These deposits should be of the greatest interest for future investigations searching for buried volatiles mixed with slope deposits.
Item URL in elib: | https://elib.dlr.de/201861/ | ||||||||||||||||||||
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Document Type: | Article | ||||||||||||||||||||
Title: | Hidden morphology of Shackleton Crater, lunar South Pole | ||||||||||||||||||||
Authors: |
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Date: | 10 October 2023 | ||||||||||||||||||||
Journal or Publication Title: | Planetary and Space Science | ||||||||||||||||||||
Refereed publication: | Yes | ||||||||||||||||||||
Open Access: | No | ||||||||||||||||||||
Gold Open Access: | No | ||||||||||||||||||||
In SCOPUS: | Yes | ||||||||||||||||||||
In ISI Web of Science: | Yes | ||||||||||||||||||||
Volume: | 238 | ||||||||||||||||||||
DOI: | 10.1016/j.pss.2023.105795 | ||||||||||||||||||||
Page Range: | p. 105795 | ||||||||||||||||||||
Publisher: | Elsevier | ||||||||||||||||||||
ISSN: | 0032-0633 | ||||||||||||||||||||
Status: | Published | ||||||||||||||||||||
Keywords: | Shackelton, Morphology, Lunar Orbiter Laser Altimeter | ||||||||||||||||||||
HGF - Research field: | Aeronautics, Space and Transport | ||||||||||||||||||||
HGF - Program: | Space | ||||||||||||||||||||
HGF - Program Themes: | Space Exploration | ||||||||||||||||||||
DLR - Research area: | Raumfahrt | ||||||||||||||||||||
DLR - Program: | R EW - Space Exploration | ||||||||||||||||||||
DLR - Research theme (Project): | R - Project BepiColombo - MERTIS and BELA, R - Project JUICE - JANUS and GALA | ||||||||||||||||||||
Location: | Berlin-Adlershof | ||||||||||||||||||||
Institutes and Institutions: | Institute of Planetary Research > Planetary Geodesy | ||||||||||||||||||||
Deposited By: | Stark, Dr. Alexander | ||||||||||||||||||||
Deposited On: | 08 Jan 2024 10:45 | ||||||||||||||||||||
Last Modified: | 29 Jan 2024 12:51 |
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