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WFRF:(Pirani A.)
 

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LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00004590naa a2200553 4500
001oai:lup.lub.lu.se:6929d2a2-ad40-4675-9922-c3d74854763a
003SwePub
008180208s2018 | |||||||||||000 ||eng|
024a https://lup.lub.lu.se/record/6929d2a2-ad40-4675-9922-c3d74854763a2 URI
024a https://doi.org/10.1007/s10686-017-9570-12 DOI
040 a (SwePub)lu
041 a engb eng
042 9 SwePub
072 7a art2 swepub-publicationtype
072 7a ref2 swepub-contenttype
100a Turrini, D.u University of Atacama,Institute for Space Astrophysics and Planetology4 aut
2451 0a The contribution of the ARIEL space mission to the study of planetary formation
264 c 2018-01-29
264 1b Springer Science and Business Media LLC,c 2018
520 a The study of extrasolar planets and of the Solar System provides complementary pieces of the mosaic represented by the process of planetary formation. Exoplanets are essential to fully grasp the huge diversity of outcomes that planetary formation and the subsequent evolution of the planetary systems can produce. The orbital and basic physical data we currently possess for the bulk of the exoplanetary population, however, do not provide enough information to break the intrinsic degeneracy of their histories, as different evolutionary tracks can result in the same final configurations. The lessons learned from the Solar System indicate us that the solution to this problem lies in the information contained in the composition of planets. The goal of the Atmospheric Remote-Sensing Infrared Exoplanet Large-survey (ARIEL), one of the three candidates as ESA M4 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. ARIEL will focus on warm and hot planets to take advantage of their well-mixed atmospheres, which should show minimal condensation and sequestration of high-Z materials and thus reveal their bulk composition across all main cosmochemical elements. In this work we will review the most outstanding open questions concerning the way planets form and the mechanisms that contribute to create habitable environments that the compositional information gathered by ARIEL will allow to tackle.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
653 a ARIEL
653 a Astrochemistry
653 a Atmospheric remote-sensing infrared exoplanet large-survey
653 a Exoplanets
653 a Planetary formation
653 a Space missions
700a Miguel, Y.u Leiden University4 aut
700a Zingales, T.u INAF Palermo Astronomical Observatory,University College London4 aut
700a Piccialli, A.u Belgian Institute for Space Aeronomy4 aut
700a Helled, R.u University of Zurich4 aut
700a Vazan, A.u University of Amsterdam4 aut
700a Oliva, F.u Institute for Space Astrophysics and Planetology4 aut
700a Sindoni, G.u Institute for Space Astrophysics and Planetology4 aut
700a Panić, O.u University of Leeds4 aut
700a Leconte, J.u Bordeaux Observatory4 aut
700a Min, M.u University of Amsterdam4 aut
700a Pirani, S.u Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science4 aut0 (Swepub:lu)astr-smp
700a Selsis, F.u Bordeaux Observatory4 aut
700a Coudé du Foresto, V.u Paris Observatory4 aut
700a Mura, A.u Institute for Space Astrophysics and Planetology4 aut
700a Wolkenberg, P.u Institute for Space Astrophysics and Planetology,Space Research Centre4 aut
710a University of Atacamab Institute for Space Astrophysics and Planetology4 org
773t Experimental Astronomyd : Springer Science and Business Media LLCg 46:1, s. 45-65q 46:1<45-65x 0922-6435x 1572-9508
856u http://dx.doi.org/10.1007/s10686-017-9570-1y FULLTEXT
856u http://eprints.whiterose.ac.uk/127812/8/1804.06179.pdf
8564 8u https://lup.lub.lu.se/record/6929d2a2-ad40-4675-9922-c3d74854763a
8564 8u https://doi.org/10.1007/s10686-017-9570-1

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