Evidence map›Paper›PMID 35673554›Full record

ArticleExperimental astronomy2022

Exploring the link between star and planet formation with Ariel.

Diego Turrini, Claudio Codella, Camilla Danielski, Davide Fedele, Sergio Fonte, Antonio Garufi, Mario Giuseppe Guarcello, Ravit Helled, Masahiro Ikoma, Mihkel Kama and 15 more

Abstract read
PubMed Full text at PMC Publisher
In one paragraph

Article in Experimental astronomy, 2022. 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

25 authors.

Diego TurriniInstitute of Space Astrophysics and Planetology INAF-IAPS, Via Fosso del Cavaliere 100, I-00133 Rome, Italy.ORCID 0000-0002-1923-7740
Claudio CodellaINAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50127 Firenze, Italy.
Camilla DanielskiInstituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía s/n, 18008 Granada, Spain.ORCID 0000-0002-3729-2663
Davide FedeleINAF - Osservatorio Astrofisico di Torino, Via Osservatorio 20, I-10025 Pino Torinese, Italy.
Sergio FonteInstitute of Space Astrophysics and Planetology INAF-IAPS, Via Fosso del Cavaliere 100, I-00133 Rome, Italy.
Antonio GarufiINAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50127 Firenze, Italy.
Mario Giuseppe GuarcelloINAF - Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, I-90134 Palermo, Italy.
Ravit HelledInstitute for Computational Science, Center for Theoretical Astrophysics and Cosmology, University of Zurich, CH-8057 Zurich, Switzerland.
Masahiro IkomaDepartment of Earth and Planetary Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033 Japan.
Mihkel KamaDepartment of Physics and Astronomy, University College London, London, WC1E 6BT UK.
Tadahiro KimuraDepartment of Earth and Planetary Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033 Japan.
J M Diederik KruijssenAstronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstraße 12-14, 69120 Heidelberg, Germany.
Jesus MaldonadoINAF - Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, I-90134 Palermo, Italy.
Yamila MiguelLeiden Observatory, Leiden University, Niels Bohrweg 2, 2333CA Leiden, The Netherlands.ORCID 0000-0002-0747-8862
Sergio MolinariInstitute of Space Astrophysics and Planetology INAF-IAPS, Via Fosso del Cavaliere 100, I-00133 Rome, Italy.
Athanasia NikolaouSapienza University of Rome, Piazzale Aldo Moro 2, Rome, 00185 Italy.
Fabrizio OlivaInstitute of Space Astrophysics and Planetology INAF-IAPS, Via Fosso del Cavaliere 100, I-00133 Rome, Italy.
Olja PanićSchool of Physics and Astronomy, E. C. Stoner Building, University of Leeds, Leeds, LS2 9JT UK.
Marco PignatariE.A. Milne Centre for Astrophysics, Department of Physics, Mathematics, University of Hull, Hull, HU6 7RX UK.
Linda PodioINAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50127 Firenze, Italy.
Hans RickmanCentrum Badań Kosmicznykh Polskiej Akademii Nauk (CBK PAN), Bartycka 18A, 00-716 Warszawa, Poland.
Eugenio SchisanoInstitute of Space Astrophysics and Planetology INAF-IAPS, Via Fosso del Cavaliere 100, I-00133 Rome, Italy.
Sho ShibataDepartment of Earth and Planetary Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033 Japan.
Allona VazanDepartment of Natural Sciences and Astrophysics Research Center of the Open university (ARCO), The Open University of Israel, 4353701 Raanana, Israel.
Paulina WolkenbergInstitute of Space Astrophysics and Planetology INAF-IAPS, Via Fosso del Cavaliere 100, I-00133 Rome, Italy.

Funding

European Research Council 714907
6 · The paper itself

Abstract

The goal of the Ariel space mission is to observe a large and diversified population of transiting planets around a range of host star types to collect information on their atmospheric composition. The planetary bulk and atmospheric compositions bear the marks of the way the planets formed: Ariel's observations will therefore provide an unprecedented wealth of data to advance our understanding of planet formation in our Galaxy. A number of environmental and evolutionary factors, however, can affect the final atmospheric composition. Here we provide a concise overview of which factors and effects of the star and planet formation processes can shape the atmospheric compositions that will be observed by Ariel, and highlight how Ariel's characteristics make this mission optimally suited to address this very complex problem.

Indexed as

ArielGalactic environmentPlanet formationProtoplanetary discsStar formationStellar characterization

Identifiers

PMID35673554
PMCPMC9166885

What OpenQuestion holds

Textmetadata
LicenceCC BY
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.