Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/24555
DC Field | Value | Language |
---|---|---|
dc.contributor.author | FULLE, Marco | en_US |
dc.contributor.author | Altobelli, N. | en_US |
dc.contributor.author | Buratti, B. | en_US |
dc.contributor.author | Choukroun, M. | en_US |
dc.contributor.author | Fulchignoni, M. | en_US |
dc.contributor.author | Grün, E. | en_US |
dc.contributor.author | Taylor, M. G. G. T. | en_US |
dc.contributor.author | Weissman, P. | en_US |
dc.date.accessioned | 2020-05-06T14:31:51Z | - |
dc.date.available | 2020-05-06T14:31:51Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/24555 | - |
dc.description.abstract | ESA's Rosetta Mission has followed Comet 67P/Churyumov-Gerasimenko from 3.6 au inbound to 3.6 au outbound. Many results are largely unexpected, as compared to previous models based on in situ and ground-based observations of Jupiter-family comets. The main topics discussed in this review are (1) the importance of the large concavities characterizing the 67P nucleus, that, (2) coupled to the nucleus obliquity, make seasons an unexpectedly important source of many phenomena observed in this and probably in most comets; (3) the mostly uniform distribution of ices over the nucleus surface; (4) the high dust-to-water mass ratio, which implies that much of the nucleus mass is in the form of minerals partly coming from the inner proto-solar nebula, thus making 67P very porous and less hydrated than primitive CI chondrites. 67P nucleus may have never experienced any collision at speeds larger than 1 m s<SUP>-1</SUP>. | en_US |
dc.language.iso | eng | en_US |
dc.title | Unexpected and significant findings in comet 67P/Churyumov-Gerasimenko: an interdisciplinary view | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stw1663 | en_US |
dc.identifier.scopus | 2-s2.0-85015855495 | en_US |
dc.identifier.isi | 000403172000002 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/462/Suppl_1/S2/2633355 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 462 | en_US |
dc.relation.issue | Suppl 1 | en_US |
dc.relation.firstpage | S2 | en_US |
dc.relation.lastpage | S8 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2016MNRAS.462S...2F | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare 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. Trieste | - |
crisitem.author.orcid | 0000-0001-8435-5287 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
Appears in Collections: | 1.01 Articoli in rivista |
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File | Description | Size | Format | |
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stw1663.pdf | PDF editoriale | 226.39 kB | Adobe PDF | View/Open |
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