MASCOT’s in situ analysis of asteroid Ryugu in the context of regolith samples and remote sensing data returned by Hayabusa2
Abstract The Hayabusa2 mission provided a unique data set of asteroid Ryugu that covers a wide range of spatial scale from the orbiter remote sensing instruments to the returned samples. The MASCOT lander that was delivered onto the surface of Ryugu aimed to provide context for these data sets by pr...
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Format: | Article |
Language: | English |
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SpringerOpen
2023-04-01
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Series: | Earth, Planets and Space |
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Online Access: | https://doi.org/10.1186/s40623-023-01805-8 |
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author | Katharina Otto Tra-Mi Ho Stephan Ulamec Jean-Pierre Bibring Jens Biele Matthias Grott Maximilian Hamm David Hercik Ralf Jaumann Masahiko Sato Stefan E. Schröder Satoshi Tanaka Ulrich Auster Kohei Kitazato Jörg Knollenberg Aurelie Moussi Tomoki Nakamura Tatsuaki Okada Cedric Pilorget Nicole Schmitz Seiji Sugita Koji Wada Hikaru Yabuta |
author_facet | Katharina Otto Tra-Mi Ho Stephan Ulamec Jean-Pierre Bibring Jens Biele Matthias Grott Maximilian Hamm David Hercik Ralf Jaumann Masahiko Sato Stefan E. Schröder Satoshi Tanaka Ulrich Auster Kohei Kitazato Jörg Knollenberg Aurelie Moussi Tomoki Nakamura Tatsuaki Okada Cedric Pilorget Nicole Schmitz Seiji Sugita Koji Wada Hikaru Yabuta |
author_sort | Katharina Otto |
collection | DOAJ |
description | Abstract The Hayabusa2 mission provided a unique data set of asteroid Ryugu that covers a wide range of spatial scale from the orbiter remote sensing instruments to the returned samples. The MASCOT lander that was delivered onto the surface of Ryugu aimed to provide context for these data sets by producing in situ data collected by a camera (MasCam), a radiometer (MARA), a magnetometer (MasMag) and a spectrometer (MicrOmega). In this work, we evaluate the success of MASCOT as an integrated lander to bridge the gap between orbiter and returned sample analysis. We find that MASCOT’s measurements and derivatives thereof, including the rock morphology, colour in the visible wavelengths, possible meteorite analogue, density, and porosity of the rock at the landing site are in good agreement with those of the orbiter and the returned samples. However, it also provides information on the spatial scale (sub-millimetres to centimetres) at which some physical properties such as the thermal inertia and reflectance undergo scale-dependent changes. Some of the in situ observations such as the presence of clast/inclusions in rocks and the absence of fine particles at the landing site was uniquely identified by MASCOT. Thus, we conclude that the delivery of an in situ instrument like MASCOT provides a valuable data set that complements and provides context for remote sensing and returned sample analyses. Graphical Abstract |
first_indexed | 2024-04-09T18:55:39Z |
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id | doaj.art-1db573e7411a49008a7b52d35bce2048 |
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issn | 1880-5981 |
language | English |
last_indexed | 2024-04-09T18:55:39Z |
publishDate | 2023-04-01 |
publisher | SpringerOpen |
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series | Earth, Planets and Space |
spelling | doaj.art-1db573e7411a49008a7b52d35bce20482023-04-09T11:10:24ZengSpringerOpenEarth, Planets and Space1880-59812023-04-0175111610.1186/s40623-023-01805-8MASCOT’s in situ analysis of asteroid Ryugu in the context of regolith samples and remote sensing data returned by Hayabusa2Katharina Otto0Tra-Mi Ho1Stephan Ulamec2Jean-Pierre Bibring3Jens Biele4Matthias Grott5Maximilian Hamm6David Hercik7Ralf Jaumann8Masahiko Sato9Stefan E. Schröder10Satoshi Tanaka11Ulrich Auster12Kohei Kitazato13Jörg Knollenberg14Aurelie Moussi15Tomoki Nakamura16Tatsuaki Okada17Cedric Pilorget18Nicole Schmitz19Seiji Sugita20Koji Wada21Hikaru Yabuta22German Aerospace Center (DLR), Institute of Planetary ResearchGerman Aerospace Center (DLR), Institute of Space SystemsGerman Aerospace Center (DLR), Space Operations and Astronaut TrainingInstitute d’Astrophysique SpatialeGerman Aerospace Center (DLR), Space Operations and Astronaut TrainingGerman Aerospace Center (DLR), Institute of Planetary ResearchGerman Aerospace Center (DLR), Institute of Planetary ResearchInstitute of Atmospheric Physics (CAS)Free University Berlin, Institute of Geological SciencesUniversity of Tokyo, Department of Earth and Planetary ScienceLuleå University of Technology, Department of Computer Science, Electrical and Space EngineeringJapan Aerospace Exploration Agency (JAXA), Institute of Space and Astronautical Science (ISAS)Technical University Braunschweig, Institute of Geophysics and Extraterrestrial PhysicsUniversity of Aizu, Center for Advanced Information Science and Technology (CAIST)German Aerospace Center (DLR), Institute of Planetary ResearchCentre National d’Etudes Spatiales (CNES)Tohoku University, Department of Earth SciencesJapan Aerospace Exploration Agency (JAXA), Institute of Space and Astronautical Science (ISAS)Institute d’Astrophysique SpatialeGerman Aerospace Center (DLR), Institute of Planetary ResearchUniversity of Tokyo, Department of Earth and Planetary SciencePlanetary Exploration Research Center, Chiba Institute of TechnologyHiroshima University, Department of Earth and Planetary Systems ScienceAbstract The Hayabusa2 mission provided a unique data set of asteroid Ryugu that covers a wide range of spatial scale from the orbiter remote sensing instruments to the returned samples. The MASCOT lander that was delivered onto the surface of Ryugu aimed to provide context for these data sets by producing in situ data collected by a camera (MasCam), a radiometer (MARA), a magnetometer (MasMag) and a spectrometer (MicrOmega). In this work, we evaluate the success of MASCOT as an integrated lander to bridge the gap between orbiter and returned sample analysis. We find that MASCOT’s measurements and derivatives thereof, including the rock morphology, colour in the visible wavelengths, possible meteorite analogue, density, and porosity of the rock at the landing site are in good agreement with those of the orbiter and the returned samples. However, it also provides information on the spatial scale (sub-millimetres to centimetres) at which some physical properties such as the thermal inertia and reflectance undergo scale-dependent changes. Some of the in situ observations such as the presence of clast/inclusions in rocks and the absence of fine particles at the landing site was uniquely identified by MASCOT. Thus, we conclude that the delivery of an in situ instrument like MASCOT provides a valuable data set that complements and provides context for remote sensing and returned sample analyses. Graphical Abstracthttps://doi.org/10.1186/s40623-023-01805-8Asteroid RyuguIn situ analysesAsteroid sample returnMulti-scale analysisAsteroid regolith propertiesAsteroid regolith |
spellingShingle | Katharina Otto Tra-Mi Ho Stephan Ulamec Jean-Pierre Bibring Jens Biele Matthias Grott Maximilian Hamm David Hercik Ralf Jaumann Masahiko Sato Stefan E. Schröder Satoshi Tanaka Ulrich Auster Kohei Kitazato Jörg Knollenberg Aurelie Moussi Tomoki Nakamura Tatsuaki Okada Cedric Pilorget Nicole Schmitz Seiji Sugita Koji Wada Hikaru Yabuta MASCOT’s in situ analysis of asteroid Ryugu in the context of regolith samples and remote sensing data returned by Hayabusa2 Earth, Planets and Space Asteroid Ryugu In situ analyses Asteroid sample return Multi-scale analysis Asteroid regolith properties Asteroid regolith |
title | MASCOT’s in situ analysis of asteroid Ryugu in the context of regolith samples and remote sensing data returned by Hayabusa2 |
title_full | MASCOT’s in situ analysis of asteroid Ryugu in the context of regolith samples and remote sensing data returned by Hayabusa2 |
title_fullStr | MASCOT’s in situ analysis of asteroid Ryugu in the context of regolith samples and remote sensing data returned by Hayabusa2 |
title_full_unstemmed | MASCOT’s in situ analysis of asteroid Ryugu in the context of regolith samples and remote sensing data returned by Hayabusa2 |
title_short | MASCOT’s in situ analysis of asteroid Ryugu in the context of regolith samples and remote sensing data returned by Hayabusa2 |
title_sort | mascot s in situ analysis of asteroid ryugu in the context of regolith samples and remote sensing data returned by hayabusa2 |
topic | Asteroid Ryugu In situ analyses Asteroid sample return Multi-scale analysis Asteroid regolith properties Asteroid regolith |
url | https://doi.org/10.1186/s40623-023-01805-8 |
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