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.
Exploring the link between star and planet formation with Ariel.
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作者: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 Jesus, Miguel Yamila, Molinari Sergio, Nikolaou Athanasia, Oliva Fabrizio, PaniÄ Olja, Pignatari Marco, Podio Linda, Rickman Hans, Schisano Eugenio, Shibata Sho, Vazan Allona, Wolkenberg Paulina
| 期刊: | Exp Astron (Dordr) | 影响因子: | 0.000 |
| 时间: | 2022 | 起止号: | 2022;53(2):225-278 |
| doi: | 10.1007/s10686-021-09754-4 | ||
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