Evidence map›Paper›PMID 32642055›Full record

ArticleInterface focus2020

Aluminosilicate haloes preserve complex life approximately 800 million years ago.

Ross P Anderson, Nicholas J Tosca, Gianfelice Cinque, Mark D Frogley, Ioannis Lekkas, Austin Akey, Gareth M Hughes, Kristin D Bergmann, Andrew H Knoll, Derek E G Briggs

Open access · bronzeAbstract read
In one paragraph

Article in Interface focus, 2020. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 7 papers.

0numbers the graph read from it
0cells of the map it votes in
7citing papers in PubMed
3.3field-weighted citation impact, top 8% 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

7 citing papers in PubMed, 35 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

10 authors at 5 institutions in 2 countries.

Ross P AndersonAll Souls College, University of Oxford, Oxford OX1 4AL, UK.ORCID 0000-0002-0558-7563
Nicholas J ToscaDepartment of Earth Sciences, University of Oxford, Oxford OX1 3AN, UK.ORCID 0000-0003-4415-4231
Gianfelice CinqueDiamond Light Source, Harwell Science and Innovation Campus, Didcot OX11 ODE, UK.
Mark D FrogleyDiamond Light Source, Harwell Science and Innovation Campus, Didcot OX11 ODE, UK.
Ioannis LekkasDiamond Light Source, Harwell Science and Innovation Campus, Didcot OX11 ODE, UK.
Austin AkeyCenter for Nanoscale Systems, Harvard University, Cambridge, MA 02138, USA.
Gareth M HughesDepartment of Materials, University of Oxford, Oxford OX1 3PH, UK.
Kristin D BergmannDepartment of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA.
Andrew H KnollDepartment of Organismic and Evolutionary Biology, Harvard University, Cambridge, MA 02138, USA.ORCID 0000-0003-1308-8585
Derek E G BriggsDepartment of Geology and Geophysics, Yale University, New Haven, CT 06511, USA.ORCID 0000-0003-0649-6417
Diamond Light Source · GBUniversity of Oxford · GBHarvard University · USMassachusetts Institute of Technology · USYale University · US

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Mudstone-hosted microfossils are a major component of the Proterozoic fossil record, particularly dominating the record of early eukaryotic life. Early organisms possessed no biomineralized parts to resist decay and controls on their fossilization in mudstones are poorly understood. Consequently, the Proterozoic fossil record is compromised-we do not know whether changing temporal/spatial patterns of microfossil occurrences reflect evolution or the distribution of favourable fossilization conditions. We investigated fossilization within the approximately 1000 Ma Lakhanda Group (Russia) and the approximately 800 Ma Svanbergfjellet and Wynniatt formations (Svalbard and Arctic Canada). Vertical sections of microfossils and surrounding matrices were extracted from thin sections by focused ion beam milling. Elemental mapping and synchrotron-based infrared microspectroscopy revealed that microfossils are surrounded by haloes rich in aluminium, probably hosted in kaolinite. Kaolinite has been implicated in Cambrian Burgess Shale-type (BST) fossilization and is known to slow the growth of degraders. The Neoproterozoic mudstone microfossil record may be biased to tropical settings conducive to kaolinite formation. These deposits lack metazoan fossils even though they share fossilization conditions with younger BST deposits that are capable of preserving non-mineralizing metazoans. Thus metazoans, at least those typically preserved in BST deposits, were probably absent from sedimentary environments before approximately 800 Ma.

Indexed as

clay mineralscomplex lifeearly eukaryotesmetazoan antiquityProterozoic eontaphonomy

Identifiers

PMID32642055
PMCPMC7333908
OpenAlexW3034662998

What OpenQuestion holds

Textmetadata
Read underepoch 390

Registered trials

None linked

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.