Turrini, D;
Codella, C;
Danielski, C;
Fedele, D;
Fonte, S;
Garufi, A;
Guarcello, MG;
... Wolkenberg, P; + view all
(2021)
Exploring the link between star and planet formation with Ariel.
Experimental Astronomy
10.1007/s10686-021-09754-4.
(In press).
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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.
Type: | Article |
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Title: | Exploring the link between star and planet formation with Ariel |
Open access status: | An open access version is available from UCL Discovery |
DOI: | 10.1007/s10686-021-09754-4 |
Publisher version: | https://doi.org/10.1007/s10686-021-09754-4 |
Language: | English |
Additional information: | Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/. |
Keywords: | Ariel, Planet formation, Protoplanetary discs, Star formation, Galactic environment, Stellar characterization, GALACTIC CHEMICAL EVOLUTION, SOLAR-SYSTEM ABUNDANCES, PROTOPLANETARY DISK, GIANT PLANETS, EXTRASOLAR PLANETS, PARENT STARS, CONDENSATION TEMPERATURE, CHROMOSPHERIC ACTIVITY, REFRACTORY ELEMENTS, PROTOSTELLAR DISKS |
UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy |
URI: | https://discovery.ucl.ac.uk/id/eprint/10138001 |
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