Exploring the link between star and planet formation with Ariel.
Ariel
Galactic environment
Planet formation
Protoplanetary discs
Star formation
Stellar characterization
Journal
Experimental astronomy
ISSN: 1572-9508
Titre abrégé: Exp Astron (Dordr)
Pays: Netherlands
ID NLM: 101769314
Informations de publication
Date de publication:
2022
2022
Historique:
received:
30
06
2020
accepted:
13
04
2021
entrez:
8
6
2022
pubmed:
9
6
2022
medline:
9
6
2022
Statut:
ppublish
Résumé
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.
Identifiants
pubmed: 35673554
doi: 10.1007/s10686-021-09754-4
pii: 9754
pmc: PMC9166885
doi:
Types de publication
Journal Article
Langues
eng
Pagination
225-278Subventions
Organisme : European Research Council
ID : 714907
Pays : International
Informations de copyright
© The Author(s) 2021.
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