Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/23754
DC Field | Value | Language |
---|---|---|
dc.contributor.author | TURRINI, Diego | en_US |
dc.contributor.author | Nelson, R. P. | en_US |
dc.contributor.author | Barbieri, M. | en_US |
dc.date.accessioned | 2020-03-31T10:57:18Z | - |
dc.date.available | 2020-03-31T10:57:18Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.issn | 0922-6435 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/23754 | - |
dc.description.abstract | Over the last twenty years, the search for extrasolar planets has revealed the rich diversity of outcomes from the formation and evolution of planetary systems. In order to fully understand how these extrasolar planets came to be, however, the orbital and physical data we possess are not enough, and they need to be complemented with information about the composition of the exoplanets. Ground-based and space-based observations provided the first data on the atmospheric composition of a few extrasolar planets, but a larger and more detailed sample is required before we can fully take advantage of it. The primary goal of a dedicated space mission like the Exoplanet Characterization Observatory (EChO) proposal is to fill this gap and to expand the limited data we possess by performing a systematic survey of extrasolar planets. The full exploitation of the data that space-based and ground-based facilities will provide in the near future, however, requires knowledge about the sources and sinks of the chemical species and molecules that will be observed. Luckily, the study of the past history of the Solar System provides several indications about the effects of processes like migration, late accretion and secular impacts, and on the time they occur in the life of planetary systems. In this work we will review what is already known about the factors influencing the composition of planetary atmospheres, focusing on the case of gaseous giant planets, and what instead still need to be investigated. | en_US |
dc.language.iso | eng | en_US |
dc.title | The role of planetary formation and evolution in shaping the composition of exoplanetary atmospheres | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1007/s10686-014-9401-6 | en_US |
dc.identifier.scopus | 2-s2.0-84952978979 | en_US |
dc.identifier.isi | 000367627900008 | en_US |
dc.identifier.url | https://link.springer.com/article/10.1007%2Fs10686-014-9401-6 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 40 | en_US |
dc.relation.issue | 2-3 | en_US |
dc.relation.firstpage | 501 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | GBR | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | EXPERIMENTAL ASTRONOMY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2015ExA....40..501T | en_US |
dc.relation.ercsector | Scienze Fisiche Settori ERC (ERC) di riferimento::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegherò il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Torino | - |
crisitem.author.orcid | 0000-0002-1923-7740 | - |
crisitem.journal.journalissn | 0922-6435 | - |
crisitem.journal.ance | E061604 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
1401.5119.pdf | postprint | 726.44 kB | Adobe PDF | View/Open |
Turrini2015_Article_TheRoleOfPlanetaryFormationAnd.pdf | [Administrators only] | 1.06 MB | Adobe PDF |
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