Unique thermal expansion properties of water key to the formation of sea ice on Earth

International audience The formation of sea ice in polar regions is possible because a salinity gradient or halocline keeps the water column stable despite intense cooling. Here, we demonstrate that a unique water property is central to the maintenance of the polar halocline, namely, that the therma...

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Published in:Science Advances
Main Authors: Roquet, Fabien, Ferreira, David, Caneill, Romain, Schlesinger, Daniel, Madec, Gurvan
Other Authors: Department of Marine Sciences Gothenburg, Göteborgs Universitet = University of Gothenburg (GU), Department of Meteorology Reading, University of Reading (UOR), Department of Applied Environmental Science Stockholm (ITM), Stockholm University, Bolin Centre for Climate Research, Nucleus for European Modeling of the Ocean (LOCEAN-NEMO R&D), Laboratoire d'Océanographie et du Climat : Expérimentations et Approches Numériques (LOCEAN), Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636)), École normale supérieure - Paris (ENS-PSL), Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X), Institut Polytechnique de Paris (IP Paris)-Institut Polytechnique de Paris (IP Paris)-Centre National d'Études Spatiales Toulouse (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-École normale supérieure - Paris (ENS-PSL), Institut Polytechnique de Paris (IP Paris)-Institut Polytechnique de Paris (IP Paris)-Centre National d'Études Spatiales Toulouse (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636)), Institut Polytechnique de Paris (IP Paris)-Institut Polytechnique de Paris (IP Paris)-Centre National d'Études Spatiales Toulouse (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Format: Article in Journal/Newspaper
Language:English
Published: CCSD 2022
Subjects:
Online Access:https://hal.science/hal-03952777
https://hal.science/hal-03952777v1/document
https://hal.science/hal-03952777v1/file/sciadv.abq0793.pdf
https://doi.org/10.1126/sciadv.abq0793
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author Roquet, Fabien
Ferreira, David
Caneill, Romain
Schlesinger, Daniel
Madec, Gurvan
author2 Department of Marine Sciences Gothenburg
Göteborgs Universitet = University of Gothenburg (GU)
Department of Meteorology Reading
University of Reading (UOR)
Department of Applied Environmental Science Stockholm (ITM)
Stockholm University
Bolin Centre for Climate Research
Nucleus for European Modeling of the Ocean (LOCEAN-NEMO R&D)
Laboratoire d'Océanographie et du Climat : Expérimentations et Approches Numériques (LOCEAN)
Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636))
École normale supérieure - Paris (ENS-PSL)
Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)
Institut Polytechnique de Paris (IP Paris)-Institut Polytechnique de Paris (IP Paris)-Centre National d'Études Spatiales Toulouse (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-École normale supérieure - Paris (ENS-PSL)
Institut Polytechnique de Paris (IP Paris)-Institut Polytechnique de Paris (IP Paris)-Centre National d'Études Spatiales Toulouse (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636))
Institut Polytechnique de Paris (IP Paris)-Institut Polytechnique de Paris (IP Paris)-Centre National d'Études Spatiales Toulouse (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
author_facet Roquet, Fabien
Ferreira, David
Caneill, Romain
Schlesinger, Daniel
Madec, Gurvan
author_sort Roquet, Fabien
collection HAL Sorbonne Université
container_issue 46
container_title Science Advances
container_volume 8
description International audience The formation of sea ice in polar regions is possible because a salinity gradient or halocline keeps the water column stable despite intense cooling. Here, we demonstrate that a unique water property is central to the maintenance of the polar halocline, namely, that the thermal expansion coefficient (TEC) of seawater increases by one order of magnitude between polar and tropical regions. Using a fully coupled climate model, it is shown that, even with excess precipitations, sea ice would not form at all if the near-freezing temperature TEC was not well below its ocean average value. The leading order dependence of the TEC on temperature is essential to the coexistence of the mid/low-latitude thermally stratified and the high-latitude sea ice–covered oceans that characterize our planet. A key implication is that nonlinearities of water properties have a first-order impact on the global climate of Earth and possibly exoplanets.
format Article in Journal/Newspaper
genre Sea ice
genre_facet Sea ice
id ftsorbonneuniv:oai:HAL:hal-03952777v1
institution Open Polar
language English
op_collection_id ftsorbonneuniv
op_doi https://doi.org/10.1126/sciadv.abq0793
op_relation info:eu-repo/semantics/altIdentifier/doi/10.1126/sciadv.abq0793
doi:10.1126/sciadv.abq0793
PUBMEDCENTRAL: PMC9668305
WOS: 000890493500002
op_rights http://creativecommons.org/licenses/by/
info:eu-repo/semantics/OpenAccess
op_source ISSN: 2375-2548
Science Advances
https://hal.science/hal-03952777
Science Advances , 2022, 8 (46), ⟨10.1126/sciadv.abq0793⟩
publishDate 2022
publisher CCSD
record_format openpolar
spelling ftsorbonneuniv:oai:HAL:hal-03952777v1 2025-03-23T15:45:06+00:00 Unique thermal expansion properties of water key to the formation of sea ice on Earth Roquet, Fabien Ferreira, David Caneill, Romain Schlesinger, Daniel Madec, Gurvan Department of Marine Sciences Gothenburg Göteborgs Universitet = University of Gothenburg (GU) Department of Meteorology Reading University of Reading (UOR) Department of Applied Environmental Science Stockholm (ITM) Stockholm University Bolin Centre for Climate Research Nucleus for European Modeling of the Ocean (LOCEAN-NEMO R&D) Laboratoire d'Océanographie et du Climat : Expérimentations et Approches Numériques (LOCEAN) Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636)) École normale supérieure - Paris (ENS-PSL) Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X) Institut Polytechnique de Paris (IP Paris)-Institut Polytechnique de Paris (IP Paris)-Centre National d'Études Spatiales Toulouse (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-École normale supérieure - Paris (ENS-PSL) Institut Polytechnique de Paris (IP Paris)-Institut Polytechnique de Paris (IP Paris)-Centre National d'Études Spatiales Toulouse (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Muséum national d'Histoire naturelle (MNHN)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut Pierre-Simon-Laplace (IPSL (FR_636)) Institut Polytechnique de Paris (IP Paris)-Institut Polytechnique de Paris (IP Paris)-Centre National d'Études Spatiales Toulouse (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité) 2022-11-18 https://hal.science/hal-03952777 https://hal.science/hal-03952777v1/document https://hal.science/hal-03952777v1/file/sciadv.abq0793.pdf https://doi.org/10.1126/sciadv.abq0793 en eng CCSD American Association for the Advancement of Science (AAAS) info:eu-repo/semantics/altIdentifier/doi/10.1126/sciadv.abq0793 doi:10.1126/sciadv.abq0793 PUBMEDCENTRAL: PMC9668305 WOS: 000890493500002 http://creativecommons.org/licenses/by/ info:eu-repo/semantics/OpenAccess ISSN: 2375-2548 Science Advances https://hal.science/hal-03952777 Science Advances , 2022, 8 (46), ⟨10.1126/sciadv.abq0793⟩ [SDU]Sciences of the Universe [physics] info:eu-repo/semantics/article Journal articles 2022 ftsorbonneuniv https://doi.org/10.1126/sciadv.abq0793 2025-02-21T01:01:58Z International audience The formation of sea ice in polar regions is possible because a salinity gradient or halocline keeps the water column stable despite intense cooling. Here, we demonstrate that a unique water property is central to the maintenance of the polar halocline, namely, that the thermal expansion coefficient (TEC) of seawater increases by one order of magnitude between polar and tropical regions. Using a fully coupled climate model, it is shown that, even with excess precipitations, sea ice would not form at all if the near-freezing temperature TEC was not well below its ocean average value. The leading order dependence of the TEC on temperature is essential to the coexistence of the mid/low-latitude thermally stratified and the high-latitude sea ice–covered oceans that characterize our planet. A key implication is that nonlinearities of water properties have a first-order impact on the global climate of Earth and possibly exoplanets. Article in Journal/Newspaper Sea ice HAL Sorbonne Université Science Advances 8 46
spellingShingle [SDU]Sciences of the Universe [physics]
Roquet, Fabien
Ferreira, David
Caneill, Romain
Schlesinger, Daniel
Madec, Gurvan
Unique thermal expansion properties of water key to the formation of sea ice on Earth
title Unique thermal expansion properties of water key to the formation of sea ice on Earth
title_full Unique thermal expansion properties of water key to the formation of sea ice on Earth
title_fullStr Unique thermal expansion properties of water key to the formation of sea ice on Earth
title_full_unstemmed Unique thermal expansion properties of water key to the formation of sea ice on Earth
title_short Unique thermal expansion properties of water key to the formation of sea ice on Earth
title_sort unique thermal expansion properties of water key to the formation of sea ice on earth
topic [SDU]Sciences of the Universe [physics]
topic_facet [SDU]Sciences of the Universe [physics]
url https://hal.science/hal-03952777
https://hal.science/hal-03952777v1/document
https://hal.science/hal-03952777v1/file/sciadv.abq0793.pdf
https://doi.org/10.1126/sciadv.abq0793