Hydrogen abundance estimation and distribution on (101955) Bennu
International audience Asteroids were likely a major source of volatiles and water to early Earth. Quantifying the hydration of asteroids is necessary to constrain models of the formation and evolution of the Solar System and the origin of Life on Earth. The OSIRIS-REx (Origins, Spectral Interpretat...
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Online Access: | https://hal.science/hal-03502255 https://hal.science/hal-03502255/document https://hal.science/hal-03502255/file/S0019103521001111.pdf https://doi.org/10.1016/j.icarus.2021.114427 |
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ftinsu:oai:HAL:hal-03502255v1 2023-11-05T03:45:19+01:00 Hydrogen abundance estimation and distribution on (101955) Bennu Praet, A. Barucci, M. A. Clark, B. E. Kaplan, H. H. Simon, A. A. Hamilton, V. E. Emery, J. P. Howell, E. S. Lim, L. F. Zou, X. -D. Li, J. -Y. Reuter, D. C. Merlin, F. Deshapriya, J. D. P. Fornasier, S. Hasselmann, P. H. Poggiali, G. Ferrone, S. Brucato, J. R. Takir, D. Cloutis, E. Connolly, H. C. Fulchignoni, M. Lauretta, D. S. Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA) Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité) Institut Universitaire de France (IUF) Ministère de l'Education nationale, de l’Enseignement supérieur et de la Recherche (M.E.N.E.S.R.) 2021 https://hal.science/hal-03502255 https://hal.science/hal-03502255/document https://hal.science/hal-03502255/file/S0019103521001111.pdf https://doi.org/10.1016/j.icarus.2021.114427 en eng HAL CCSD Elsevier info:eu-repo/semantics/altIdentifier/doi/10.1016/j.icarus.2021.114427 hal-03502255 https://hal.science/hal-03502255 https://hal.science/hal-03502255/document https://hal.science/hal-03502255/file/S0019103521001111.pdf BIBCODE: 2021Icar.36314427P doi:10.1016/j.icarus.2021.114427 PII: S0019-1035(21)00111-1 http://creativecommons.org/licenses/by-nc/ info:eu-repo/semantics/OpenAccess ISSN: 0019-1035 EISSN: 1090-2643 Icarus https://hal.science/hal-03502255 Icarus, 2021, 363, pp.4123-4142. ⟨10.1016/j.icarus.2021.114427⟩ Asteroid Bennu Asteroid surfaces Asteroid composition Meteorites Spectroscopy [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/article Journal articles 2021 ftinsu https://doi.org/10.1016/j.icarus.2021.114427 2023-10-11T16:24:47Z International audience Asteroids were likely a major source of volatiles and water to early Earth. Quantifying the hydration of asteroids is necessary to constrain models of the formation and evolution of the Solar System and the origin of Life on Earth. The OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer) mission showed that near-Earth asteroid (101955) Bennu contains widespread, abundant hydrated phyllosilicates, indicated by a ubiquitous absorption at ~ 2.7 μm. The objective of this work is to quantify the hydration-that is, the hydrogen content-of phyllosilicates on Bennu's surface and investigate how this hydration varies spatially. We analyse spectral parameters (normalized optical path length, NOPL; effective single-scattering albedo, ESPAT; and Gaussian modeling) computed from the hydrated phyllosilicate absorption band of spatially resolved visible-near-infrared spectra acquired by OVIRS (the OSIRIS-REx Visible and InfraRed Spectrometer). We also computed the same spectral parameters using laboratory-measured spectra of meteorites including CMs, CIs, and the ungrouped C2 Tagish Lake. We estimate the mean hydrogen content of water and hydroxyl groups in hydrated phyllosilicates on Bennu's surface to be 0.71 ± 0.16 wt%. This value is consistent with the hydration range of some aqueously altered meteorites (CMs, C2 Tagish Lake), but not the most aqueously altered group (CIs). The sample collection site of the OSIRIS-REx mission has slightly higher hydrogen content than average. Spatial variations in hydrogen content on Bennu's surface are linked to geomorphology, and may have been partially inherited from its parent body. Article in Journal/Newspaper Tagish Institut national des sciences de l'Univers: HAL-INSU Icarus 363 114427 |
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Open Polar |
collection |
Institut national des sciences de l'Univers: HAL-INSU |
op_collection_id |
ftinsu |
language |
English |
topic |
Asteroid Bennu Asteroid surfaces Asteroid composition Meteorites Spectroscopy [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
spellingShingle |
Asteroid Bennu Asteroid surfaces Asteroid composition Meteorites Spectroscopy [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] Praet, A. Barucci, M. A. Clark, B. E. Kaplan, H. H. Simon, A. A. Hamilton, V. E. Emery, J. P. Howell, E. S. Lim, L. F. Zou, X. -D. Li, J. -Y. Reuter, D. C. Merlin, F. Deshapriya, J. D. P. Fornasier, S. Hasselmann, P. H. Poggiali, G. Ferrone, S. Brucato, J. R. Takir, D. Cloutis, E. Connolly, H. C. Fulchignoni, M. Lauretta, D. S. Hydrogen abundance estimation and distribution on (101955) Bennu |
topic_facet |
Asteroid Bennu Asteroid surfaces Asteroid composition Meteorites Spectroscopy [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
description |
International audience Asteroids were likely a major source of volatiles and water to early Earth. Quantifying the hydration of asteroids is necessary to constrain models of the formation and evolution of the Solar System and the origin of Life on Earth. The OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer) mission showed that near-Earth asteroid (101955) Bennu contains widespread, abundant hydrated phyllosilicates, indicated by a ubiquitous absorption at ~ 2.7 μm. The objective of this work is to quantify the hydration-that is, the hydrogen content-of phyllosilicates on Bennu's surface and investigate how this hydration varies spatially. We analyse spectral parameters (normalized optical path length, NOPL; effective single-scattering albedo, ESPAT; and Gaussian modeling) computed from the hydrated phyllosilicate absorption band of spatially resolved visible-near-infrared spectra acquired by OVIRS (the OSIRIS-REx Visible and InfraRed Spectrometer). We also computed the same spectral parameters using laboratory-measured spectra of meteorites including CMs, CIs, and the ungrouped C2 Tagish Lake. We estimate the mean hydrogen content of water and hydroxyl groups in hydrated phyllosilicates on Bennu's surface to be 0.71 ± 0.16 wt%. This value is consistent with the hydration range of some aqueously altered meteorites (CMs, C2 Tagish Lake), but not the most aqueously altered group (CIs). The sample collection site of the OSIRIS-REx mission has slightly higher hydrogen content than average. Spatial variations in hydrogen content on Bennu's surface are linked to geomorphology, and may have been partially inherited from its parent body. |
author2 |
Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA) Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité) Institut Universitaire de France (IUF) Ministère de l'Education nationale, de l’Enseignement supérieur et de la Recherche (M.E.N.E.S.R.) |
format |
Article in Journal/Newspaper |
author |
Praet, A. Barucci, M. A. Clark, B. E. Kaplan, H. H. Simon, A. A. Hamilton, V. E. Emery, J. P. Howell, E. S. Lim, L. F. Zou, X. -D. Li, J. -Y. Reuter, D. C. Merlin, F. Deshapriya, J. D. P. Fornasier, S. Hasselmann, P. H. Poggiali, G. Ferrone, S. Brucato, J. R. Takir, D. Cloutis, E. Connolly, H. C. Fulchignoni, M. Lauretta, D. S. |
author_facet |
Praet, A. Barucci, M. A. Clark, B. E. Kaplan, H. H. Simon, A. A. Hamilton, V. E. Emery, J. P. Howell, E. S. Lim, L. F. Zou, X. -D. Li, J. -Y. Reuter, D. C. Merlin, F. Deshapriya, J. D. P. Fornasier, S. Hasselmann, P. H. Poggiali, G. Ferrone, S. Brucato, J. R. Takir, D. Cloutis, E. Connolly, H. C. Fulchignoni, M. Lauretta, D. S. |
author_sort |
Praet, A. |
title |
Hydrogen abundance estimation and distribution on (101955) Bennu |
title_short |
Hydrogen abundance estimation and distribution on (101955) Bennu |
title_full |
Hydrogen abundance estimation and distribution on (101955) Bennu |
title_fullStr |
Hydrogen abundance estimation and distribution on (101955) Bennu |
title_full_unstemmed |
Hydrogen abundance estimation and distribution on (101955) Bennu |
title_sort |
hydrogen abundance estimation and distribution on (101955) bennu |
publisher |
HAL CCSD |
publishDate |
2021 |
url |
https://hal.science/hal-03502255 https://hal.science/hal-03502255/document https://hal.science/hal-03502255/file/S0019103521001111.pdf https://doi.org/10.1016/j.icarus.2021.114427 |
genre |
Tagish |
genre_facet |
Tagish |
op_source |
ISSN: 0019-1035 EISSN: 1090-2643 Icarus https://hal.science/hal-03502255 Icarus, 2021, 363, pp.4123-4142. ⟨10.1016/j.icarus.2021.114427⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/doi/10.1016/j.icarus.2021.114427 hal-03502255 https://hal.science/hal-03502255 https://hal.science/hal-03502255/document https://hal.science/hal-03502255/file/S0019103521001111.pdf BIBCODE: 2021Icar.36314427P doi:10.1016/j.icarus.2021.114427 PII: S0019-1035(21)00111-1 |
op_rights |
http://creativecommons.org/licenses/by-nc/ info:eu-repo/semantics/OpenAccess |
op_doi |
https://doi.org/10.1016/j.icarus.2021.114427 |
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Icarus |
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363 |
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114427 |
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