Evidence map›Paper›PMID 34255549›Full record

ArticleAstrobiology2021

Exobiology of the Venusian Clouds: New Insights into Habitability through Terrestrial Models and Methods of Detection.

Oleg R Kotsyurbenko, Jaime A Cordova, Andrey A Belov, Vladimir S Cheptsov, Denise Kölbl, Yuliya Y Khrunyk, Margarita O Kryuchkova, Tetyana Milojevic, Rakesh Mogul, Satoshi Sasaki and 3 more

Abstract read
In one paragraph

Article in Astrobiology, 2021. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 14 papers.

0numbers the graph read from it
0cells of the map it votes in
14citing 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

14 citing papers in PubMed.

  1. Article
  2. Review
  3. Article
  4. Article
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  6. Article
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  9. Review
  10. Article
  11. Article
  12. Stability of nucleic acid bases in concentrated sulfuric acid: Implications for the habitability of Venus' clouds.Proceedings of the National Academy of Sciences of the United States of America · 2023
    Article
  13. Review
  14. 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.

Oleg R KotsyurbenkoYugra State University, The Institute of Oil and Gas, School of Ecology, Khanty-Mansiysk, Russian Federation.
Jaime A CordovaLaboratory of Genetics, University of Wisconsin, Madison, Wisconsin, USA.
Andrey A BelovNetwork of Researchers on the Chemical Evolution of Life, Leeds, UK.
Vladimir S CheptsovNetwork of Researchers on the Chemical Evolution of Life, Leeds, UK.
Denise KölblSpace Biochemistry Group, Department of Biophysical Chemistry, University of Vienna, Vienna, Austria.
Yuliya Y KhrunykDepartment of Heat Treatment and Physics of Metal, Ural Federal University, Ekaterinburg, Russian Federation.
Margarita O KryuchkovaNetwork of Researchers on the Chemical Evolution of Life, Leeds, UK.
Tetyana MilojevicSpace Biochemistry Group, Department of Biophysical Chemistry, University of Vienna, Vienna, Austria.
Rakesh MogulChemistry and Biochemistry Department, California State Polytechnic University, Pomona, California, USA.
Satoshi SasakiSchool of Biosciences and Biotechnology/School of Health Sciences, Tokyo University of Technology, Hachioji, Tokyo, Japan.
Grzegorz P SłowikInstitute of Materials and Biomedical Engineering, Faculty of Mechanical Engineering, University of Zielona Góra, Zielona Góra, Poland.
Valery SnytnikovBoreskov Institute of Catalysis, Siberian Branch of the Russian Academy of Sciences, Novosibirsk, Russian Federation.
Elena A VorobyovaNetwork of Researchers on the Chemical Evolution of Life, Leeds, UK.

Funding

PREDOCTORAL TRAINING PROGRAM IN GENETICST32GM007133 · NIGMS · UNIVERSITY OF WISCONSIN-MADISON · PI PERNA, NICOLE T · 1985 to 2023
$16.5M
NIGMS NIH HHS T32 GM007133
6 · The paper itself

Abstract

The search for life beyond Earth has focused on Mars and the icy moons Europa and Enceladus, all of which are considered a safe haven for life due to evidence of current or past water. The surface of Venus, on the other hand, has extreme conditions that make it a nonhabitable environment to life as we know it. This is in contrast, however, to its cloud layer, which, while still an extreme environment, may prove to be a safe haven for some extreme forms of life similar to extremophiles on Earth. We consider the venusian clouds a habitable environment based on the presence of (1) a solvent for biochemical reactions, (2) appropriate physicochemical conditions, (3) available energy, and (4) biologically relevant elements. The diversity of extreme microbial ecosystems on Earth has allowed us to identify terrestrial chemolithoautotrophic microorganisms that may be analogs to putative venusian organisms. Here, we hypothesize and describe biological processes that may be performed by such organisms in the venusian clouds. To detect putative venusian organisms, we describe potential biosignature detection methods, which include metal-microbial interactions and optical methods. Finally, we describe currently available technology that can potentially be used for modeling and simulation experiments.

Indexed as

JupiterVenusEcosystemExobiologyExtraterrestrial EnvironmentAstrobiologyCloudsHabitabilityPolyextremophilesTerrestrial modelsVenus

Identifiers

PMID34255549
PMCPMC9545807

What OpenQuestion holds

Textmetadata
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.