Evidence map›Paper›PMID 33469027›Full record

ArticleNature communications2021

Jarosite formation in deep Antarctic ice provides a window into acidic, water-limited weathering on Mars.

Giovanni Baccolo, Barbara Delmonte, P B Niles, Giannantonio Cibin, Elena Di Stefano, Dariush Hampai, Lindsay Keller, Valter Maggi, Augusto Marcelli, Joseph Michalski and 2 more

Open access · goldAbstract read
In one paragraph

Article in Nature communications, 2021. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 10 papers.

0numbers the graph read from it
0cells of the map it votes in
10citing papers in PubMed
7.0field-weighted citation impact, top 3% of its field
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

10 citing papers in PubMed, 47 citations in OpenAlex.

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4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

12 authors at 8 institutions in 4 countries.

Giovanni BaccoloDepartment of Environmental and Earth Sciences, University of Milano-Bicocca, 20126, Milan, Italy. giovanni.baccolo@unimib.it.ORCID 0000-0002-1246-8968
Barbara DelmonteDepartment of Environmental and Earth Sciences, University of Milano-Bicocca, 20126, Milan, Italy.
P B NilesNASA Johnson Space Center, Houston, TX, 77058, USA.ORCID 0000-0001-7612-1421
Giannantonio CibinDiamond Light Source, Harwell Science and Innovation Campus, Didcot, OX11 0DE, UK.ORCID 0000-0001-5761-6760
Elena Di StefanoDepartment of Environmental and Earth Sciences, University of Milano-Bicocca, 20126, Milan, Italy.
Dariush HampaiLaboratori Nazionali di Frascati, Istituto Nazionale di Fisica Nucleare, 00044, Frascati, Italy.ORCID 0000-0002-8881-0520
Lindsay KellerNASA Johnson Space Center, Houston, TX, 77058, USA.
Valter MaggiDepartment of Environmental and Earth Sciences, University of Milano-Bicocca, 20126, Milan, Italy.
Augusto MarcelliLaboratori Nazionali di Frascati, Istituto Nazionale di Fisica Nucleare, 00044, Frascati, Italy.
Joseph MichalskiDepartment of Earth Sciences, University of Hong Kong, Hong Kong, Hong Kong.ORCID 0000-0002-4543-6452
Christopher SneadJacobs, NASA Johnson Space Center, Houston, TX, 77058, USA.
Massimo FrezzottiDepartment of Science, University Roma Tre, Rome, Italy.ORCID 0000-0002-2461-2883
Johnson Space Center · USIstituto Nazionale di Fisica Nucleare · ITIstituto Nazionale di Fisica Nucleare, Sezione di Milano Bicocca · ITDiamond Light Source · GBRoma Tre University · ITUniversity of Hong Kong · HKUniversity of Milano-Bicocca · ITUniversity of Siena · IT

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Many interpretations have been proposed to explain the presence of jarosite within Martian surficial sediments, including the possibility that it precipitated within paleo-ice deposits owing to englacial weathering of dust. However, until now a similar geochemical process was not observed on Earth nor in other planetary settings. We report a multi-analytical indication of jarosite formation within deep ice. Below 1000 m depth, jarosite crystals adhering on residual silica-rich particles have been identified in the Talos Dome ice core (East Antarctica) and interpreted as products of weathering involving aeolian dust and acidic atmospheric aerosols. The progressive increase of ice metamorphism and re-crystallization with depth, favours the relocation and concentration of dust and the formation of acidic brines in isolated environments, allowing chemical reactions and mineral neo-formation to occur. This is the first described englacial diagenetic mechanism occurring in deep Antarctic ice and supports the ice-weathering model for jarosite formation on Mars, highlighting the geologic importance of paleo ice-related processes on this planet. Additional implications concern the preservation of dust-related signals in deep ice cores with respect to paleoclimatic reconstructions and the englacial history of meteorites from Antarctic blue ice fields.

Identifiers

PMID33469027
PMCPMC7815727
OpenAlexW3125121564

What OpenQuestion holds

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LicenceCC BY
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Registered trials

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Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.