Evidence map›Paper›PMID 36932072›Full record

ArticleNature communications2023

Insights into the formation and evolution of extraterrestrial amino acids from the asteroid Ryugu.

Christian Potiszil, Tsutomu Ota, Masahiro Yamanaka, Chie Sakaguchi, Katsura Kobayashi, Ryoji Tanaka, Tak Kunihiro, Hiroshi Kitagawa, Masanao Abe, Akiko Miyazaki and 14 more

Full text read
In one paragraph

Article in Nature communications, 2023. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 13 papers.

0numbers the graph read from it
0cells of the map it votes in
13citing 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

13 citing papers in PubMed.

  1. Article
  2. Interstellar Stereoisomerism.ACS earth & space chemistry · 2026
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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

24 authors.

Christian PotiszilPheasant Memorial Laboratory, Institute for Planetary Materials, Okayama University, Yamada 827, Misasa, Tottori, 682-0193, Japan. cpotiszil@okayama-u.ac.jp.ORCID http://orcid.org/0000-0001-9420-4220
Tsutomu OtaPheasant Memorial Laboratory, Institute for Planetary Materials, Okayama University, Yamada 827, Misasa, Tottori, 682-0193, Japan.ORCID http://orcid.org/0000-0003-4801-1609
Masahiro YamanakaPheasant Memorial Laboratory, Institute for Planetary Materials, Okayama University, Yamada 827, Misasa, Tottori, 682-0193, Japan.ORCID http://orcid.org/0000-0002-7414-3616
Chie SakaguchiPheasant Memorial Laboratory, Institute for Planetary Materials, Okayama University, Yamada 827, Misasa, Tottori, 682-0193, Japan.ORCID http://orcid.org/0000-0003-0817-0365
Katsura KobayashiPheasant Memorial Laboratory, Institute for Planetary Materials, Okayama University, Yamada 827, Misasa, Tottori, 682-0193, Japan.ORCID http://orcid.org/0000-0002-1696-1418
Ryoji TanakaPheasant Memorial Laboratory, Institute for Planetary Materials, Okayama University, Yamada 827, Misasa, Tottori, 682-0193, Japan.
Tak KunihiroPheasant Memorial Laboratory, Institute for Planetary Materials, Okayama University, Yamada 827, Misasa, Tottori, 682-0193, Japan.
Hiroshi KitagawaPheasant Memorial Laboratory, Institute for Planetary Materials, Okayama University, Yamada 827, Misasa, Tottori, 682-0193, Japan.
Masanao AbeInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.
Akiko MiyazakiInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.ORCID http://orcid.org/0000-0001-7427-2285
Aiko NakatoInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.
Satoru NakazawaInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.ORCID http://orcid.org/0000-0003-4250-1826
Masahiro NishimuraInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.
Tatsuaki OkadaInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.ORCID http://orcid.org/0000-0001-6381-8107
Takanao SaikiInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.
Satoshi TanakaInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.
Fuyuto TeruiInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.
Yuichi TsudaInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.
Tomohiro UsuiInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.ORCID http://orcid.org/0000-0002-4653-293X
Sei-Ichiro WatanabeNagoya University, Nagoya, Japan.ORCID http://orcid.org/0000-0002-5820-2102
Toru YadaInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.ORCID http://orcid.org/0000-0002-7971-510X
Kasumi YogataInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.ORCID http://orcid.org/0000-0002-3717-9185
Makoto YoshikawaInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.
Eizo NakamuraPheasant Memorial Laboratory, Institute for Planetary Materials, Okayama University, Yamada 827, Misasa, Tottori, 682-0193, Japan.ORCID http://orcid.org/0000-0003-4399-9443

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

All life on Earth contains amino acids and carbonaceous chondrite meteorites have been suggested as their source at the origin of life on Earth. While many meteoritic amino acids are considered indigenous, deciphering the extent of terrestrial contamination remains an issue. The Ryugu asteroid fragments (JAXA Hayabusa2 mission), represent the most uncontaminated primitive extraterrestrial material available. Here, the concentrations of amino acids from two particles from different touchdown sites (TD1 and TD2) are reported. The concentrations show that N,N-dimethylglycine (DMG) is the most abundant amino acid in the TD1 particle, but below detection limit in the other. The TD1 particle mineral components indicate it experienced more aqueous alteration. Furthermore, the relationships between the amino acids and the geochemistry suggest that DMG formed on the Ryugu progenitor body during aqueous alteration. The findings highlight the importance of aqueous chemistry for defining the ultimate concentrations of amino acids in primitive extraterrestrial samples.

Identifiers

PMID36932072
PMCPMC10023693

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