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Hidden morphology of Shackleton Crater, lunar South Pole

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/
Document Type:Article
Title:Hidden morphology of Shackleton Crater, lunar South Pole
Authors:
AuthorsInstitution or Email of AuthorsAuthor's ORCID iDORCID Put Code
Mitusov, Andrey V.You Tube channel “Land and Water CA”, Berlin, GermanyUNSPECIFIEDUNSPECIFIED
Stark, AlexanderUNSPECIFIEDhttps://orcid.org/0000-0001-9110-1138UNSPECIFIED
Khrisanov, Vladislav R.Department of Landscape Ecology, Institute of Basic Biological Problems RAS (IBBP RAS), Institutskaya st. 2, 142290, Moscow region, Pushchino, RussiaUNSPECIFIEDUNSPECIFIED
Oberst, JürgenInstitute of Geodesy and Geoinformation Science, Technische Universität Berlin, Berlin, GermanyUNSPECIFIEDUNSPECIFIED
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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