TY - JOUR
T1 - Exploring the link between star and planet formation with Ariel
AU - Turrini, Diego
AU - Codella, Claudio
AU - Danielski, Camilla
AU - Fedele, Davide
AU - Fonte, Sergio
AU - Garufi, Antonio
AU - Guarcello, Mario Giuseppe
AU - Helled, Ravit
AU - Ikoma, Masahiro
AU - Kama, Mihkel
AU - Kimura, Tadahiro
AU - Kruijssen, J. M.Diederik
AU - Maldonado, Jesus
AU - Miguel, Yamila
AU - Molinari, Sergio
AU - Nikolaou, Athanasia
AU - Oliva, Fabrizio
AU - Panić, Olja
AU - Pignatari, Marco
AU - Podio, Linda
AU - Rickman, Hans
AU - Schisano, Eugenio
AU - Shibata, Sho
AU - Vazan, Allona
AU - Wolkenberg, Paulina
N1 - Publisher Copyright:
© 2021, The Author(s).
PY - 2022/4
Y1 - 2022/4
N2 - 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.
AB - 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.
KW - Ariel
KW - Galactic environment
KW - Planet formation
KW - Protoplanetary discs
KW - Star formation
KW - Stellar characterization
UR - http://www.scopus.com/inward/record.url?scp=85110468067&partnerID=8YFLogxK
U2 - 10.1007/s10686-021-09754-4
DO - 10.1007/s10686-021-09754-4
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C2 - 35673554
AN - SCOPUS:85110468067
SN - 0922-6435
VL - 53
SP - 225
EP - 278
JO - Experimental Astronomy
JF - Experimental Astronomy
IS - 2
ER -