Evidence map›Paper›PMID 29978041›Full record

ArticleScience advances2018

Krypton isotopes and noble gas abundances in the coma of comet 67P/Churyumov-Gerasimenko.

Martin Rubin, Kathrin Altwegg, Hans Balsiger, Akiva Bar-Nun, Jean-Jacques Berthelier, Christelle Briois, Ursina Calmonte, Michael Combi, Johan De Keyser, Björn Fiethe and 17 more

Open access · goldAbstract read
In one paragraph

Article in Science advances, 2018. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 5 papers.

0numbers the graph read from it
0cells of the map it votes in
5citing papers in PubMed
4.5field-weighted citation impact, top 5% 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

5 citing papers in PubMed, 66 citations in OpenAlex.

  1. Article
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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

27 authors at 10 institutions in 6 countries.

Martin RubinPhysikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland.ORCID 0000-0001-6549-3318
Kathrin AltweggPhysikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland.ORCID 0000-0002-2677-8238
Hans BalsigerPhysikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland.
Akiva Bar-NunDepartment of Geophysics, Tel Aviv University, Ramat-Aviv, Tel Aviv, Israel.
Jean-Jacques BerthelierLaboratoire Atmosphères, Milieux, Observations Spatiales, Institut Pierre Simon Laplace, CNRS, Université Pierre et Marie Curie, 4 Place Jussieu, 75252 Paris Cedex 05, France.
Christelle BrioisLaboratoire de Physique et Chimie de l'Environnement et de l'Espace, UMR 6115 CNRS-Université d'Orléans, Orléans, France.
Ursina CalmontePhysikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland.ORCID 0000-0002-0982-7501
Michael CombiDepartment of Climate and Space Sciences and Engineering, University of Michigan, 2455 Hayward, Ann Arbor, MI 48109, USA.ORCID 0000-0002-9805-0078
Johan De KeyserKoninklijk Belgisch Instituut voor Ruimte-Aeronomie-Institut Royal Belge d'Aéronomie Spatiale, Ringlaan 3, B-1180 Brussels, Belgium.ORCID 0000-0003-4805-5695
Björn FietheInstitute of Computer and Network Engineering, Technische Universität Braunschweig, Hans-Sommer-Straße 66, D-38106 Braunschweig, Germany.ORCID 0000-0002-7915-6723
Stephen A FuselierSpace Science Directorate, Southwest Research Institute, 6220 Culebra Road, San Antonio, TX 78228, USA.ORCID 0000-0003-4101-7901
Sebastien GascPhysikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland.ORCID 0000-0001-5956-4722
Tamas I GombosiDepartment of Climate and Space Sciences and Engineering, University of Michigan, 2455 Hayward, Ann Arbor, MI 48109, USA.ORCID 0000-0001-9360-4951
Kenneth C HansenDepartment of Climate and Space Sciences and Engineering, University of Michigan, 2455 Hayward, Ann Arbor, MI 48109, USA.ORCID 0000-0002-8502-1980
Ernest KoppPhysikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland.
Axel KorthMax-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany.
Diana LauferDepartment of Geophysics, Tel Aviv University, Ramat-Aviv, Tel Aviv, Israel.
Léna Le RoyPhysikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland.
Urs MallMax-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany.ORCID 0000-0003-0206-6196
Bernard MartyCentre de Recherches Pétrographiques et Géochimiques, CNRS, Université de Lorraine, 15 rue Notre Dame des Pauvres, BP 20, 54501 Vandoeuvre lès Nancy, France.
Olivier MousisLaboratoire d'Astrophysique de Marseille, CNRS, Aix-Marseille Université, 13388 Marseille, France.
Tobias OwenInstitute for Astronomy, University of Hawaii, Honolulu, HI 96822, USA.
Henri RèmeInstitut de Recherche en Astrophysique et Planétologie, CNRS, Université Paul Sabatier, Observatoire Midi-Pyrénées, 9 Avenue du Colonel Roche, 31028 Toulouse Cedex 4, France.ORCID 0000-0002-0173-882X
Thierry SémonPhysikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland.
Chia-Yu TzouPhysikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland.ORCID 0000-0002-1812-1201
Jack H WaiteInstitute of Computer and Network Engineering, Technische Universität Braunschweig, Hans-Sommer-Straße 66, D-38106 Braunschweig, Germany.ORCID 0000-0002-1978-1025
Peter WurzPhysikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland.ORCID 0000-0002-2603-1169
University of Bern · CHCentre National de la Recherche Scientifique · FRUniversity of Michigan · USMax Planck Institute for Solar System Research · DETechnische Universität Braunschweig · DETel Aviv University · ILRoyal Belgian Institute for Space Aeronomy · BESouthwest Research Institute · USUniversité d'Orléans · FRUniversity of Hawaii System · US

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

The Rosetta Orbiter Spectrometer for Ion and Neutral Analysis mass spectrometer Double Focusing Mass Spectrometer on board the European Space Agency's Rosetta spacecraft detected the major isotopes of the noble gases argon, krypton, and xenon in the coma of comet 67P/Churyumov-Gerasimenko. Earlier, it was found that xenon exhibits an isotopic composition distinct from anywhere else in the solar system. However, argon isotopes, within error, were shown to be consistent with solar isotope abundances. This discrepancy suggested an additional exotic component of xenon in comet 67P/Churyumov-Gerasimenko. We show that krypton also exhibits an isotopic composition close to solar. Furthermore, we found the argon to krypton and the krypton to xenon ratios in the comet to be lower than solar, which is a necessity to postulate an addition of exotic xenon in the comet.

Identifiers

PMID29978041
PMCPMC6031375
OpenAlexW2809807926

What OpenQuestion holds

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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.