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Boulder Morphology on Asteroid Bennu

Svanström, Evelina and Otto, Katharina A. and Schröder, Stefan (2024) Boulder Morphology on Asteroid Bennu. Europlanet Science Congress, 2024-09-09 - 2024-09-13, Berlin, Deutschland. doi: 10.5194/epsc2024-505.

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Official URL: https://meetingorganizer.copernicus.org/EPSC2024/EPSC2024-505.html

Abstract

NASA’s Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer (OSIRIS-REx) spacecraft arrived at the near-Earth rubble pile asteroid (101955) Bennu in December 2018, and took high resolution images of the surface (3). The images revealed that the surface is covered with boulders of various sizes (6). The morphology and orientation of these boulders can provide valuable information about the body’s history and mechanical properties (1,4). In this work, we use images taken by the OSIRIS-Rex Camera Suite (OCAMS) (6) to map the outline of boulders on Bennu in two different geologic units: a rugged unit and a smooth unit (2). This work was implemented using the open-source software QGIS (5). The parameters we found in QGIS are show in Figure 1. We compare the two units’ boulder morphology in terms of boulder roughness by looking at the shape factors solidity (to what extent a boulder is convex) and circularity (to what extent a boulder’s perimeter is similar to the perimeter of a circle with the same area). The solidity plotted against the circularity can be seen in Figure 2. We also looked at the boulder shape by studying the shape factors elongation (how elongated a boulder is) and roundness (to what extent the area of the boulder resembles the area of a circle with its radius equal to the boulder’s semi-major axis). The elongation plotted against the roundness can be seen in Figure 3. Despite the geologic differences of the smooth and rugged units, we find no significant difference in boulder roughness and shape between these two units. Both regions’ boulders possess a large variation of values that overlap significantly. However, we do find that the smooth unit tends to have smaller boulders (0.579±0.35) m with more boulders mapped (total 2426) than the rugged unit ((0.711±0.48) m, total 1774 boulders mapped). Finally, we found that smaller boulders tend to be rounder and less rough than larger boulders in both units, however, this may be an effect of the image resolution. This work implies that boulder morphology is relatively uniform over the surface of Bennu, also indicating that the mechanical material properties are similar in the two units. Although the units are geologically distinct, the material they are made of seems to be homogenous.

Item URL in elib:https://elib.dlr.de/209671/
Document Type:Conference or Workshop Item (Poster)
Title:Boulder Morphology on Asteroid Bennu
Authors:
AuthorsInstitution or Email of AuthorsAuthor's ORCID iDORCID Put Code
Svanström, Evelinasvanstromevelina (at) gmail.comUNSPECIFIEDUNSPECIFIED
Otto, Katharina A.Katharina.Otto (at) dlr.dehttps://orcid.org/0000-0002-0675-1177UNSPECIFIED
Schröder, StefanLuleå University of Technology, 98128 Kiruna, Swedenhttps://orcid.org/0000-0003-0323-8324UNSPECIFIED
Date:September 2024
Refereed publication:No
Open Access:Yes
Gold Open Access:No
In SCOPUS:No
In ISI Web of Science:No
Volume:17
DOI:10.5194/epsc2024-505
Page Range:EPSC2024-505
Series Name:EPSC Abstracts
Status:Published
Keywords:Boulders, morphology, morphometry, mapping, Osiris-Rex, NASA mission, Asteroid Bennu
Event Title:Europlanet Science Congress
Event Location:Berlin, Deutschland
Event Type:international Conference
Event Start Date:9 September 2024
Event End Date:13 September 2024
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 - CO-I Participations
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Planetary Geology
Deposited By: Otto, Dr. Katharina A.
Deposited On:02 Dec 2024 13:07
Last Modified:09 Jan 2025 08:35

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