Evidence map›Paper›PMID 37285429›Full record

ArticleScience advances2023

Complex organosulfur molecules on comet 67P: Evidence from the ROSINA measurements and insights from laboratory simulations.

Ahmed Mahjoub, Kathrin Altwegg, Michael J Poston, Martin Rubin, Robert Hodyss, Mathieu Choukroun, Bethany L Ehlmann, Nora Hänni, Michael E Brown, Jordana Blacksberg and 2 more

Open access · goldAbstract read
In one paragraph

Article in Science advances, 2023. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 4 papers.

0numbers the graph read from it
0cells of the map it votes in
4citing papers in PubMed
2.7field-weighted citation impact, top 10% 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

4 citing papers in PubMed, 15 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 5 institutions in 2 countries.

Ahmed MahjoubJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.ORCID 0000-0003-1229-5208
Kathrin AltweggPhysikalisches Institut, University of Bern, Bern, Switzerland.ORCID 0000-0002-2677-8238
Michael J PostonSWRI, San Antonio, TX 78238, USA.ORCID 0000-0001-5113-1017
Martin RubinPhysikalisches Institut, University of Bern, Bern, Switzerland.ORCID 0000-0001-6549-3318
Robert HodyssJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.ORCID 0000-0002-6523-3660
Mathieu ChoukrounJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.ORCID 0000-0001-7447-9139
Bethany L EhlmannDivision of Planetary and Space Sciences, Caltech, Pasadena, CA 91125, USA.ORCID 0000-0002-2745-3240
Nora HänniPhysikalisches Institut, University of Bern, Bern, Switzerland.ORCID 0000-0002-8253-6436
Michael E BrownDivision of Planetary and Space Sciences, Caltech, Pasadena, CA 91125, USA.ORCID 0000-0002-8255-0545
Jordana BlacksbergJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
John M EilerDivision of Planetary and Space Sciences, Caltech, Pasadena, CA 91125, USA.
Kevin P HandJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.ORCID 0000-0002-3225-9426
Jet Propulsion Laboratory · USCalifornia Institute of Technology · USUniversity of Bern · CHSouthwest Research Institute · USSpace Science Institute · US

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

The ROSINA (Rosetta Orbiter Spectrometer for Ion and Neutral Analysis) instrument aboard the Rosetta mission revolutionized our understanding of cometary material composition. One of Rosetta's key findings is the complexity of the composition of comet 67P/Churyumov-Gerasimenko. Here, we used ROSINA data to analyze dust particles that were volatilized during a dust event in September 2016 and report the detection of large organosulfur species and an increase in the abundances of sulfurous species previously detected in the coma. Our data support the presence of complex sulfur-bearing organics on the surface of the comet. In addition, we conducted laboratory simulations that show that this material may have formed from chemical reactions that were initiated by the irradiation of mixed ices containing H

Identifiers

PMID37285429
PMCPMC10246891
OpenAlexW4379621699

What OpenQuestion holds

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LicenceCC BY-NC
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.