Evidence map›Paper›PMID 39277576›Full record

ArticleNature communications2024

A primordial noble gas component discovered in the Ryugu asteroid and its implications.

Alexander B Verchovsky, Feargus A J Abernethy, Mahesh Anand, Ian A Franchi, Monica M Grady, Richard C Greenwood, Simeon J Barber, Martin Suttle, Motoo Ito, Naotaka Tomioka and 26 more

Abstract read
PubMed Full text at PMC Publisher
In one paragraph

Article in Nature communications, 2024. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 1 paper.

0numbers the graph read from it
0cells of the map it votes in
1citing papers in PubMed
–field-weighted citation impact
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

1 citing paper in PubMed.

  1. Article
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

36 authors.

Alexander B VerchovskyThe Open University, Milton Keynes, UK. sasha.verchovsky@open.ac.uk.ORCID http://orcid.org/0000-0002-3532-5003
Feargus A J AbernethyThe Open University, Milton Keynes, UK.ORCID http://orcid.org/0000-0001-7210-3058
Mahesh AnandThe Open University, Milton Keynes, UK.ORCID http://orcid.org/0000-0003-4026-4476
Ian A FranchiThe Open University, Milton Keynes, UK.ORCID http://orcid.org/0000-0003-4151-0480
Monica M GradyThe Open University, Milton Keynes, UK.ORCID http://orcid.org/0000-0002-4055-533X
Richard C GreenwoodThe Open University, Milton Keynes, UK.ORCID http://orcid.org/0000-0002-5544-8027
Simeon J BarberThe Open University, Milton Keynes, UK.
Martin SuttleThe Open University, Milton Keynes, UK.ORCID http://orcid.org/0000-0001-7165-2215
Motoo ItoKochi Institute for Core Sample Research, X-star, Japan Agency for Marine-Earth Science and Technology (JAMSTEC), Nankoku, Kochi, Japan.ORCID http://orcid.org/0000-0001-5686-0243
Naotaka TomiokaKochi Institute for Core Sample Research, X-star, Japan Agency for Marine-Earth Science and Technology (JAMSTEC), Nankoku, Kochi, Japan.ORCID http://orcid.org/0000-0001-5725-9513
Masayuki UesugiJapan Synchrotron Radiation Research Institute (JASRI/SPring-8), Sayo, Hyogo, Japan.ORCID http://orcid.org/0000-0001-6261-9034
Akira YamaguchiNational Institute of Polar Research (NIPR), Tachikawa, Tokyo, Japan.ORCID http://orcid.org/0000-0001-5140-7853
Makoto KimuraFaculty of Science, Kanagawa University, Yokohama, Kanagawa, Japan.ORCID http://orcid.org/0000-0003-3352-4989
Naoya ImaeUVSOR Synchrotron Facility, Institute for Molecular Science, Okazaki, Aichi, Japan.ORCID http://orcid.org/0000-0001-8160-4284
Naoki ShiraiInstitute of Materials Structure Science, High Energy Accelerator Research Organization, Tsukuba, Ibaraki, Japan.ORCID http://orcid.org/0000-0003-0988-8571
Takuji OhigashiUVSOR Synchrotron Facility, Institute for Molecular Science, Okazaki, Aichi, Japan.ORCID http://orcid.org/0000-0003-4778-5645
Ming-Chang LiuLawrence Livermore National Laboratory, Livermore, CA, USA.
Kentaro UesugiJapan Synchrotron Radiation Research Institute (JASRI/SPring-8), Sayo, Hyogo, Japan.ORCID http://orcid.org/0000-0003-2579-513X
Aiko NakatoNational Institute of Polar Research (NIPR), Tachikawa, Tokyo, Japan.ORCID http://orcid.org/0000-0003-2392-1497
Kasumi YogataInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Kanagawa, Japan.ORCID http://orcid.org/0000-0002-3717-9185
Hayato YuzawaUVSOR Synchrotron Facility, Institute for Molecular Science, Okazaki, Aichi, Japan.ORCID http://orcid.org/0000-0003-4129-4407
Yuzuru KaroujiCore Facility Center, Osaka University, 8-1 Mihogaoka, Ibaraki, Osaka, Japan.ORCID http://orcid.org/0000-0002-8540-2986
Satoru NakazawaInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Kanagawa, Japan.ORCID http://orcid.org/0000-0003-4250-1826
Tatsuaki OkadaInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Kanagawa, Japan.
Takanao SaikiInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Kanagawa, Japan.
Satoshi TanakaInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Kanagawa, Japan.
Fuyuto TeruiInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Kanagawa, Japan.
Makoto YoshikawaInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Kanagawa, Japan.ORCID http://orcid.org/0000-0002-3118-7475
Akiko MiyazakiInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Kanagawa, Japan.ORCID http://orcid.org/0000-0001-7427-2285
Masahiro NishimuraInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Kanagawa, Japan.
Toru YadaInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Kanagawa, Japan.
Masanao AbeInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Kanagawa, Japan.
Tomohiro UsuiInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Kanagawa, Japan.ORCID http://orcid.org/0000-0002-4653-293X
Sen-Ichiro WatanabeGraduate School of Environmental Studies, Nagoya University, Nagoya, Aichi, Japan.ORCID http://orcid.org/0000-0002-5820-2102
Yuichi TsudaInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Kanagawa, Japan.
Consortium Phase2 curation team Kochi

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Ryugu is the C-type asteroid from which material was brought to Earth by the Hayabusa2 mission. A number of individual grains and fine-grained samples analysed so far for noble gases have indicated that solar wind and planetary (known as P1) noble gases are present in Ryugu samples with concentrations higher than those observed in CIs, suggesting the former to be more primitive compared to the latter. Here we present results of analyses of three fine-grained samples from Ryugu, in one of which Xe concentration is an order of magnitude higher than determined so far in other samples from Ryugu. Isotopically, this Xe resembles P1, but with a much stronger isotopic fractionation relative to solar wind and significantly lower

Identifiers

PMID39277576
PMCPMC11401872

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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.