Exploring the link between star and planet formation with Ariel
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Published:2021-10-15
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ISSN:0922-6435
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Container-title:Experimental Astronomy
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language:en
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Short-container-title:Exp Astron
Author:
Turrini DiegoORCID, Codella Claudio, Danielski CamillaORCID, Fedele Davide, Fonte Sergio, Garufi Antonio, Guarcello Mario Giuseppe, Helled Ravit, Ikoma Masahiro, Kama Mihkel, Kimura Tadahiro, Kruijssen J. M. Diederik, Maldonado Jesus, Miguel YamilaORCID, Molinari Sergio, Nikolaou Athanasia, Oliva Fabrizio, Panić Olja, Pignatari Marco, Podio Linda, Rickman Hans, Schisano Eugenio, Shibata Sho, Vazan Allona, Wolkenberg Paulina
Abstract
AbstractThe 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.
Funder
Agenzia Spaziale Italiana Istituto Nazionale di Astrofisica University of Tartu Deutsche Forschungsgemeinschaft Deutsche Forschungsgemeinschaft Sachbeihilfe European Research Council Hungarian Academy of Sciences National Science Foundation Japan Society for the Promotion of Science London Royal Society Dorothy Hodgkin Fellowship
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
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