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  5. Exploring the link between star and planet formation with Ariel
 

Exploring the link between star and planet formation with Ariel

Journal
EXPERIMENTAL ASTRONOMY  
Date Issued
2022
Author(s)
TURRINI, Diego  
•
CODELLA, Claudio  
•
DANIELSKI, Camilla  
•
FEDELE, Davide  
•
FONTE, SERGIO  
•
GARUFI, Antonio  
•
GUARCELLO, Mario Giuseppe  
•
Helled, Ravit
•
Ikoma, Masahiro
•
Kama, Mihkel
•
Kimura,Tadahiro
•
Kruijssen, J. M. Diederik
•
MALDONADO PRADO, Jesus  
•
Miguel, Yamila
•
MOLINARI, Sergio  
•
Nikolaou, Athanasia
•
OLIVA, Fabrizio  
•
Panić, Olja
•
Pignatari, Marco
•
PODIO, Linda  
•
Rickman, Hans
•
SCHISANO, EUGENIO  
•
Shibata, Sho
•
Vazan, Allona
•
WOLKENBERG, Paulina Maria  
DOI
10.1007/s10686-021-09754-4
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.
Volume
53
Issue
2
Start page
225
Uri
http://hdl.handle.net/20.500.12386/36140
Url
https://link.springer.com/article/10.1007/s10686-021-09754-4
Issn Identifier
0922-6435
Ads BibCode
2022ExA....53..225T
Rights
open.access
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