Evidence map›Paper›PMID 35330631›Full record

ArticleACS earth & space chemistry2022

Experimental and Theoretical Constraints on Amino Acid Formation from PAHs in Asteroidal Settings.

Claudia-Corina Giese, Inge Loes Ten Kate, Martijn P A van den Ende, Mariette Wolthers, José C Aponte, Eloi Camprubi, Jason P Dworkin, Jamie E Elsila, Suzanne Hangx, Helen E King and 3 more

Abstract read
In one paragraph

Article in ACS earth & space chemistry, 2022. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 2 papers.

0numbers the graph read from it
0cells of the map it votes in
2citing 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

2 citing papers in PubMed.

  1. Article
  2. 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

13 authors.

Claudia-Corina GieseLeiden Observatory, Faculty of Science, Leiden University, 2300 RA Leiden, The Netherlands.ORCID https://orcid.org/0000-0001-9415-6345
Inge Loes Ten KateDepartment of Earth Sciences, Faculty of Geosciences, Utrecht University, 3584 CB Utrecht, The Netherlands.ORCID https://orcid.org/0000-0002-1135-1792
Martijn P A van den EndeUniversité Côte d'Azur, OCA, UMR Lagrange, 06000 Nice, France.
Mariette WolthersDepartment of Earth Sciences, Faculty of Geosciences, Utrecht University, 3584 CB Utrecht, The Netherlands.ORCID https://orcid.org/0000-0003-3908-5622
José C AponteSolar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, United States.ORCID https://orcid.org/0000-0002-0131-1981
Eloi CamprubiDepartment of Earth Sciences, Faculty of Geosciences, Utrecht University, 3584 CB Utrecht, The Netherlands.
Jason P DworkinSolar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, United States.ORCID https://orcid.org/0000-0002-3961-8997
Jamie E ElsilaSolar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, United States.ORCID https://orcid.org/0000-0002-0008-2590
Suzanne HangxDepartment of Earth Sciences, Faculty of Geosciences, Utrecht University, 3584 CB Utrecht, The Netherlands.
Helen E KingDepartment of Earth Sciences, Faculty of Geosciences, Utrecht University, 3584 CB Utrecht, The Netherlands.ORCID https://orcid.org/0000-0002-1825-782X
Hannah L MclainSolar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, United States.
Oliver PlümperDepartment of Earth Sciences, Faculty of Geosciences, Utrecht University, 3584 CB Utrecht, The Netherlands.ORCID https://orcid.org/0000-0001-9726-0885
Alexander G G M TielensLeiden Observatory, Faculty of Science, Leiden University, 2300 RA Leiden, The Netherlands.

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Amino acids and polycyclic aromatic hydrocarbons (PAHs) belong to the range of organic compounds detected in meteorites. In this study, we tested empirically and theoretically if PAHs are precursors for amino acids in carbonaceous chondrites, as previously suggested. We conducted experiments to synthesize amino acids from fluoranthene (PAH), with ammonium bicarbonate as a source for ammonia and carbon dioxide under mimicked asteroidal conditions. In our thermodynamic calculations, we extended our analysis to additional PAH-amino acid combinations. We explored 36 reactions involving the PAHs naphthalene, anthracene, fluoranthene, pyrene, triphenylene, and coronene and the amino acids glycine, alanine, valine, leucine, phenylalanine, and tyrosine. Our experiments do not show the formation of amino acids, whereas our theoretical results hint that PAHs could be precursors of amino acids in carbonaceous chondrites at low temperatures.

Identifiers

PMID35330631
PMCPMC8935471

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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.