Space weathering influence on Ryugu’s IR ...
Document type :
Autre communication scientifique (congrès sans actes - poster - séminaire...): Communication dans un congrès sans actes
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Title :
Space weathering influence on Ryugu’s IR signature: insights from nanoscale vibrational spectroscopy in the STEM
Author(s) :
Laforet, Sylvain [Auteur]
Unité Matériaux et Transformations (UMET) - UMR 8207
Leroux, Hugues [Auteur]
Unité Matériaux et Transformations (UMET) - UMR 8207
Le Guillou, Corentin [Auteur]
Unité Matériaux et Transformations (UMET) - UMR 8207
de la Peña, Francisco [Auteur]
Unité Matériaux et Transformations (UMET) - UMR 8207
Marinova, Maya [Auteur]
Institut Chevreul - FR2638
Jacob, Damien [Auteur]
Unité Matériaux et Transformations (UMET) - UMR 8207
Viennet, Jean-Christophe [Auteur]
Mouloud, Bahae-Eddine [Auteur]
Unité Matériaux et Transformations (UMET) - UMR 8207
Hallatt, Daniel [Auteur]
Unité Matériaux et Transformations (UMET) - UMR 8207
Teurtrie, Adrien [Auteur]
Unité Matériaux et Transformations (UMET) - UMR 8207
Pelaez Fernandez, Mario [Auteur]
Unité Matériaux et Transformations (UMET) - UMR 8207
Walls, Mike [Auteur]
Galvao-Tizei, L. [Auteur]
Troadec, david [Auteur]
Institut d'Électronique, de Microélectronique et de Nanotechnologie (IEMN) - UMR 8520
Unité Matériaux et Transformations (UMET) - UMR 8207
Leroux, Hugues [Auteur]
Unité Matériaux et Transformations (UMET) - UMR 8207
Le Guillou, Corentin [Auteur]
Unité Matériaux et Transformations (UMET) - UMR 8207
de la Peña, Francisco [Auteur]
Unité Matériaux et Transformations (UMET) - UMR 8207
Marinova, Maya [Auteur]
Institut Chevreul - FR2638
Jacob, Damien [Auteur]
Unité Matériaux et Transformations (UMET) - UMR 8207
Viennet, Jean-Christophe [Auteur]
Mouloud, Bahae-Eddine [Auteur]
Unité Matériaux et Transformations (UMET) - UMR 8207
Hallatt, Daniel [Auteur]
Unité Matériaux et Transformations (UMET) - UMR 8207
Teurtrie, Adrien [Auteur]
Unité Matériaux et Transformations (UMET) - UMR 8207
Pelaez Fernandez, Mario [Auteur]
Unité Matériaux et Transformations (UMET) - UMR 8207
Walls, Mike [Auteur]
Galvao-Tizei, L. [Auteur]
Troadec, david [Auteur]
Institut d'Électronique, de Microélectronique et de Nanotechnologie (IEMN) - UMR 8520
Conference title :
Goldschmidt 2023
City :
LYON
Country :
France
Start date of the conference :
2023-07
HAL domain(s) :
Chimie/Matériaux
Physique [physics]/Matière Condensée [cond-mat]/Science des matériaux [cond-mat.mtrl-sci]
Physique [physics]/Physique [physics]/Géophysique [physics.geo-ph]
Physique [physics]/Astrophysique [astro-ph]
Planète et Univers [physics]/Astrophysique [astro-ph]
Planète et Univers [physics]/Sciences de la Terre
Physique [physics]/Matière Condensée [cond-mat]/Science des matériaux [cond-mat.mtrl-sci]
Physique [physics]/Physique [physics]/Géophysique [physics.geo-ph]
Physique [physics]/Astrophysique [astro-ph]
Planète et Univers [physics]/Astrophysique [astro-ph]
Planète et Univers [physics]/Sciences de la Terre
English abstract : [en]
JAXA’s Hayabusa2 mission brought back 5.4 g of material from the surface of the carbonaceous asteroid Ryugu. Some grains show evidence of a modified surface attributed to space-weathering effects [1], which result from ...
Show more >JAXA’s Hayabusa2 mission brought back 5.4 g of material from the surface of the carbonaceous asteroid Ryugu. Some grains show evidence of a modified surface attributed to space-weathering effects [1], which result from solar-wind irradiation and/or micrometeoroid bombardment. In collaboration with the Hayabusa2-Initial-Analysis Min-Pet Fine Team and the Hayabusa2-Initial-Analysis core, their study should allow to investigate, for the first time, how a C-type, hydrated asteroid surface evolves when subjected to space weathering. Alongside, the recent development of monochromated electron microscopes dedicated to high resolution EELS makes it possible to reach the Mid-IR spectral range (~40 cm-1 spectral resolution at best) [2]. It thus opens the possibility for comparison with bulk IR studies with the advantage of the TEM spatial resolution. Here, we study the modified surfaces and underlying matrix of several small Ryugu grains, originating from both touchdown A and C [3]. Surfaces modified by space weathering were first identified by SEM and FIB sections were prepared. The main product of space weathering is glassy and vesiculated layer likely resulting from the melting of Ryugu materials due to micrometeorite impacts. Our results show that it is possible to distinguish the spectral signature of both space weathered melt layers and underlying preserved matrix. In particular, we evidence the loss of the H2O and -OH vibrational modes in the melt layers. It could explain why the 2.7 µm band, corresponding to hydroxyl groups in phyllosilicates, is twice less intense in NIRS3 spectra than in the returned samples ones [4]. We also observe that the organic modes are absent in the melt layers, in agreement with the EDS data. We thus demonstrate that space weathering strongly modifies the IR signature of hydrated and C-rich airless bodies, and may lead to the underestimation of their water and carbon content when analyzed by remote sensing.Show less >
Show more >JAXA’s Hayabusa2 mission brought back 5.4 g of material from the surface of the carbonaceous asteroid Ryugu. Some grains show evidence of a modified surface attributed to space-weathering effects [1], which result from solar-wind irradiation and/or micrometeoroid bombardment. In collaboration with the Hayabusa2-Initial-Analysis Min-Pet Fine Team and the Hayabusa2-Initial-Analysis core, their study should allow to investigate, for the first time, how a C-type, hydrated asteroid surface evolves when subjected to space weathering. Alongside, the recent development of monochromated electron microscopes dedicated to high resolution EELS makes it possible to reach the Mid-IR spectral range (~40 cm-1 spectral resolution at best) [2]. It thus opens the possibility for comparison with bulk IR studies with the advantage of the TEM spatial resolution. Here, we study the modified surfaces and underlying matrix of several small Ryugu grains, originating from both touchdown A and C [3]. Surfaces modified by space weathering were first identified by SEM and FIB sections were prepared. The main product of space weathering is glassy and vesiculated layer likely resulting from the melting of Ryugu materials due to micrometeorite impacts. Our results show that it is possible to distinguish the spectral signature of both space weathered melt layers and underlying preserved matrix. In particular, we evidence the loss of the H2O and -OH vibrational modes in the melt layers. It could explain why the 2.7 µm band, corresponding to hydroxyl groups in phyllosilicates, is twice less intense in NIRS3 spectra than in the returned samples ones [4]. We also observe that the organic modes are absent in the melt layers, in agreement with the EDS data. We thus demonstrate that space weathering strongly modifies the IR signature of hydrated and C-rich airless bodies, and may lead to the underestimation of their water and carbon content when analyzed by remote sensing.Show less >
Language :
Anglais
Français
Français
Audience :
Internationale
Popular science :
Non
Administrative institution(s) :
Université de Lille
CNRS
INRAE
ENSCL
CNRS
INRAE
ENSCL
Collections :
Research team(s) :
Matériaux Terrestres et Planétaires
Submission date :
2023-10-27T12:47:15Z
2023-11-02T08:15:32Z
2023-12-09T01:56:04Z
2024-02-06T10:35:13Z
2023-11-02T08:15:32Z
2023-12-09T01:56:04Z
2024-02-06T10:35:13Z