Brine residues and organics in the Urvara basin on Ceres.

Λεπτομέρειες βιβλιογραφικής εγγραφής
Τίτλος: Brine residues and organics in the Urvara basin on Ceres.
Συγγραφείς: Nathues A; Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077, Goettingen, Germany. nathues@mps.mpg.de., Hoffmann M; Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077, Goettingen, Germany., Schmedemann N; Institut für Planetologie, WWU Münster, Münster, Germany., Sarkar R; Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077, Goettingen, Germany., Thangjam G; School of Earth and Planetary Sciences, National Institute of Science Education and Research, NISER, HBNI, Bhubaneswar, India., Mengel K; Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077, Goettingen, Germany., Hernandez J; Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077, Goettingen, Germany., Hiesinger H; Institut für Planetologie, WWU Münster, Münster, Germany., Pasckert JH; Institut für Planetologie, WWU Münster, Münster, Germany.
Πηγή: Nature communications [Nat Commun] 2022 Feb 22; Vol. 13 (1), pp. 927. Date of Electronic Publication: 2022 Feb 22.
Τύπος έκδοσης: Journal Article; Research Support, Non-U.S. Gov't
Γλώσσα: English
Στοιχεία περιοδικού: Publisher: Nature Pub. Group Country of Publication: England NLM ID: 101528555 Publication Model: Electronic Cited Medium: Internet ISSN: 2041-1723 (Electronic) Linking ISSN: 20411723 NLM ISO Abbreviation: Nat Commun Subsets: MEDLINE
Imprint Name(s): Original Publication: [London] : Nature Pub. Group
Ιατρικοί όροι (MeSH): Evolution, Planetary* , Salts*, Earth, Planet ; Geology
Περίληψη: Ceres is a partially differentiated dwarf planet, as confirmed by NASA's Dawn mission. The Urvara basin (diameter ~170 km) is its third-largest impact feature, enabling insights into the cerean crust. Urvara's geology and mineralogy suggest a potential brine layer at the crust-mantle transition. Here we report new findings that help in understanding the structure and composition of the cerean crust. These results were derived by using the highest-resolution Framing Camera images acquired by Dawn at Ceres. Unexpectedly, we found meter-scale concentrated exposures of bright material (salts) along the crater's upper central ridge, which originate from an enormous depth, possibly from a deep-seated brine or salt reservoir. An extended resurfacing modified the southern floor ~100 Myr after crater formation (~250 Myr), long after the dissipation of the impact-generated heat. In this resurfaced area, one floor scarp shows a granular flow pattern of bright material, showing spectra consistent with the presence of organic material, the first such finding on Ceres beyond the vast Ernutet area. Our results strengthen the hypothesis that Ceres is and has been a geologically active world even in recent epochs, with salts and organic-rich material playing a major role in its evolution.
(© 2022. The Author(s).)
References: Science. 2012 May 11;336(6082):700-4. (PMID: 22582258)
Nature. 2015 Dec 10;528(7581):241-4. (PMID: 26659184)
Nature. 2015 Dec 10;528(7581):237-40. (PMID: 26659183)
Science. 2016 Sep 2;353(6303):1008-1010. (PMID: 27701107)
Science. 2017 Feb 17;355(6326):719-722. (PMID: 28209893)
Science. 2016 Sep 2;353(6303):. (PMID: 27701089)
Nature. 2016 Aug 4;536(7614):54-7. (PMID: 27362221)
Geophys Res Lett. 2017 Jul 16;44(13):6570-6578. (PMID: 28989206)
Substance Nomenclature: 0 (Salts)
0 (brine)
Entry Date(s): Date Created: 20220223 Date Completed: 20220412 Latest Revision: 20220412
Update Code: 20260130
PubMed Central ID: PMC8863799
DOI: 10.1038/s41467-022-28570-8
PMID: 35194036
Βάση Δεδομένων: MEDLINE
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  – Url: https://dx.doi.org/doi:10.1038/s41467-022-28570-8
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  Data: Brine residues and organics in the Urvara basin on Ceres.
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  Data: <searchLink fieldCode="AU" term="%22Nathues+A%22">Nathues A</searchLink>; Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077, Goettingen, Germany. nathues@mps.mpg.de.<br /><searchLink fieldCode="AU" term="%22Hoffmann+M%22">Hoffmann M</searchLink>; Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077, Goettingen, Germany.<br /><searchLink fieldCode="AU" term="%22Schmedemann+N%22">Schmedemann N</searchLink>; Institut für Planetologie, WWU Münster, Münster, Germany.<br /><searchLink fieldCode="AU" term="%22Sarkar+R%22">Sarkar R</searchLink>; Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077, Goettingen, Germany.<br /><searchLink fieldCode="AU" term="%22Thangjam+G%22">Thangjam G</searchLink>; School of Earth and Planetary Sciences, National Institute of Science Education and Research, NISER, HBNI, Bhubaneswar, India.<br /><searchLink fieldCode="AU" term="%22Mengel+K%22">Mengel K</searchLink>; Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077, Goettingen, Germany.<br /><searchLink fieldCode="AU" term="%22Hernandez+J%22">Hernandez J</searchLink>; Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077, Goettingen, Germany.<br /><searchLink fieldCode="AU" term="%22Hiesinger+H%22">Hiesinger H</searchLink>; Institut für Planetologie, WWU Münster, Münster, Germany.<br /><searchLink fieldCode="AU" term="%22Pasckert+JH%22">Pasckert JH</searchLink>; Institut für Planetologie, WWU Münster, Münster, Germany.
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  Data: <searchLink fieldCode="JN" term="%22101528555%22">Nature communications</searchLink> [Nat Commun] 2022 Feb 22; Vol. 13 (1), pp. 927. <i>Date of Electronic Publication: </i>2022 Feb 22.
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  Label: Abstract
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  Data: Ceres is a partially differentiated dwarf planet, as confirmed by NASA's Dawn mission. The Urvara basin (diameter ~170 km) is its third-largest impact feature, enabling insights into the cerean crust. Urvara's geology and mineralogy suggest a potential brine layer at the crust-mantle transition. Here we report new findings that help in understanding the structure and composition of the cerean crust. These results were derived by using the highest-resolution Framing Camera images acquired by Dawn at Ceres. Unexpectedly, we found meter-scale concentrated exposures of bright material (salts) along the crater's upper central ridge, which originate from an enormous depth, possibly from a deep-seated brine or salt reservoir. An extended resurfacing modified the southern floor ~100 Myr after crater formation (~250 Myr), long after the dissipation of the impact-generated heat. In this resurfaced area, one floor scarp shows a granular flow pattern of bright material, showing spectra consistent with the presence of organic material, the first such finding on Ceres beyond the vast Ernutet area. Our results strengthen the hypothesis that Ceres is and has been a geologically active world even in recent epochs, with salts and organic-rich material playing a major role in its evolution.<br /> (© 2022. The Author(s).)
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  Data: Science. 2012 May 11;336(6082):700-4. (PMID: <searchLink fieldCode="PM" term="%2222582258%22">22582258)</searchLink><br />Nature. 2015 Dec 10;528(7581):241-4. (PMID: <searchLink fieldCode="PM" term="%2226659184%22">26659184)</searchLink><br />Nature. 2015 Dec 10;528(7581):237-40. (PMID: <searchLink fieldCode="PM" term="%2226659183%22">26659183)</searchLink><br />Science. 2016 Sep 2;353(6303):1008-1010. (PMID: <searchLink fieldCode="PM" term="%2227701107%22">27701107)</searchLink><br />Science. 2017 Feb 17;355(6326):719-722. (PMID: <searchLink fieldCode="PM" term="%2228209893%22">28209893)</searchLink><br />Science. 2016 Sep 2;353(6303):. (PMID: <searchLink fieldCode="PM" term="%2227701089%22">27701089)</searchLink><br />Nature. 2016 Aug 4;536(7614):54-7. (PMID: <searchLink fieldCode="PM" term="%2227362221%22">27362221)</searchLink><br />Geophys Res Lett. 2017 Jul 16;44(13):6570-6578. (PMID: <searchLink fieldCode="PM" term="%2228989206%22">28989206)</searchLink>
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