Exploring the link between star and planet formation with Ariel View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2021-10-15

AUTHORS

Diego Turrini, Claudio Codella, Camilla Danielski, Davide Fedele, Sergio Fonte, Antonio Garufi, Mario Giuseppe Guarcello, Ravit Helled, Masahiro Ikoma, Mihkel Kama, Tadahiro Kimura, J. M. Diederik Kruijssen, Jesus Maldonado, Yamila Miguel, Sergio Molinari, Athanasia Nikolaou, Fabrizio Oliva, Olja Panić, Marco Pignatari, Linda Podio, Hans Rickman, Eugenio Schisano, Sho Shibata, Allona Vazan, Paulina Wolkenberg

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. More... »

PAGES

1-54

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  • Journal

    TITLE

    Experimental Astronomy

    ISSUE

    N/A

    VOLUME

    N/A

    Author Affiliations

  • INAF - Osservatorio Astrofisico di Torino, Via Osservatorio 20, I-10025, Pino Torinese, Italy
  • INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50127, Firenze, Italy
  • Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía s/n, 18008, Granada, Spain
  • Institute of Space Astrophysics and Planetology INAF-IAPS, Via Fosso del Cavaliere 100, I-00133, Rome, Italy
  • INAF - Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, I-90134, Palermo, Italy
  • Institute for Computational Science, Center for Theoretical Astrophysics and Cosmology, University of Zurich, CH-8057, Zurich, Switzerland
  • Department of Earth and Planetary Science, The University of Tokyo, 7-3-1 Hongo, 113-0033, Bunkyo-ku, Tokyo, Japan
  • Tartu Observatory, University of Tartu, Observatooriumi 1, 61602, Tõravere, Estonia
  • Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstraße 12-14, 69120, Heidelberg, Germany
  • SRON - Netherlands Institute for Space Research, Sorbonnelaan 2, NL-3584, CA Utrecht, The Netherlands
  • European Space Agency, ESRIN, ESA Φ-lab, Largo Galileo Galilei 1, 00044, Frascati, Italy
  • School of Physics and Astronomy, E. C. Stoner Building, University of Leeds, LS2 9JT, Leeds, UK
  • Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements & NuGrid Collaboration, www.nugridstars.org, Notre Dame, USA
  • Centrum Badań Kosmicznykh Polskiej Akademii Nauk (CBK PAN), Bartycka 18A, 00-716, Warszawa, Poland
  • Department of Natural Sciences and Astrophysics Research Center of the Open university (ARCO), The Open University of Israel, 4353701, Raanana, Israel
  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1007/s10686-021-09754-4

    DOI

    http://dx.doi.org/10.1007/s10686-021-09754-4

    DIMENSIONS

    https://app.dimensions.ai/details/publication/pub.1141917031


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