The contribution of the ARIEL space mission to the study of planetary formation View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2018-01-29

AUTHORS

D. Turrini, Y. Miguel, T. Zingales, A. Piccialli, R. Helled, A. Vazan, F. Oliva, G. Sindoni, O. Panić, J. Leconte, M. Min, S. Pirani, F. Selsis, V. Coudé du Foresto, A. Mura, P. Wolkenberg

ABSTRACT

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. More... »

PAGES

45-65

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/s10686-017-9570-1

DOI

http://dx.doi.org/10.1007/s10686-017-9570-1

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1100690156


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40 configuration
41 contribution
42 cosmochemical elements
43 data
44 degeneracy
45 different evolutionary tracks
46 diversified population
47 diversity
48 elements
49 enough information
50 environment
51 evolution
52 evolutionary tracks
53 exoplanetary population
54 exoplanets
55 extrasolar planets
56 final configuration
57 form
58 formation
59 goal
60 habitable environments
61 history
62 host star types
63 hot planets
64 huge diversity
65 information
66 intrinsic degeneracy
67 lessons
68 main cosmochemical elements
69 materials
70 mechanism
71 minimal condensation
72 mission
73 mosaic
74 open question
75 outcomes
76 outstanding open question
77 physical data
78 pieces
79 planetary formation
80 planetary systems
81 planets
82 planets form
83 population
84 problem
85 process
86 questions
87 range
88 remote
89 same final configurations
90 sequestration
91 solar system
92 solution
93 space missions
94 star type
95 study
96 subsequent evolution
97 system
98 track
99 types
100 way planets form
101 work
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