Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/28285
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Krohn, K. | en_US |
dc.contributor.author | Neesemann, A. | en_US |
dc.contributor.author | Jaumann, R. | en_US |
dc.contributor.author | Otto, K. A. | en_US |
dc.contributor.author | Stephan, K. | en_US |
dc.contributor.author | Wagner, R. J. | en_US |
dc.contributor.author | TOSI, Federico | en_US |
dc.contributor.author | ZAMBON, Francesca | en_US |
dc.contributor.author | Ruesch, O. | en_US |
dc.contributor.author | Williams, D. A. | en_US |
dc.contributor.author | Raymond, C. A. | en_US |
dc.contributor.author | Russell, C. T. | en_US |
dc.date.accessioned | 2020-11-12T11:13:48Z | - |
dc.date.available | 2020-11-12T11:13:48Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 0094-8276 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/28285 | - |
dc.description.abstract | One of the main tasks of the Dawn mission is to characterize the potentially ice-rich crust of the dwarf planet Ceres. Ongoing studies reveal morphological features related to ice-rich material such as pits or particular landslides. Here we report the identification of ring-mold craters within the huge impact crater Occator. The Cerean ring-mold craters exhibit strong morphological similarities to the ring-mold craters on Mars, where ice-rich material is thought to be involved in such crater development. We discuss the occurrence of water ice reservoirs in the subsurface and assume that ice-rich material likely plays an important role in the development of ring-mold craters on Ceres. The occurrence of ring-mold craters on the surface of Ceres is not only a sign of water ice reservoirs in the subsurface but can also be used for the study of habitable zones on planetary bodies. | en_US |
dc.language.iso | eng | en_US |
dc.title | Ring-Mold Craters on Ceres: Evidence for Shallow Subsurface Water Ice Sources | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1029/2018GL078697 | en_US |
dc.identifier.scopus | 2-s2.0-85053210048 | en_US |
dc.identifier.isi | 000445612500028 | en_US |
dc.identifier.url | https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2018GL078697 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 45 | en_US |
dc.relation.issue | 16 | en_US |
dc.relation.firstpage | 8121 | en_US |
dc.relation.lastpage | 8128 | en_US |
dc.relation.numberofpages | 8 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 12 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | DEU | en_US |
dc.relation.scientificsector | FIS/06 - FISICA PER IL SISTEMA TERRA E IL MEZZO CIRCUMTERRESTRE | en_US |
dc.relation.journal | GEOPHYSICAL RESEARCH LETTERS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2018GeoRL..45.8121K | 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 | IAPS Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.orcid | 0000-0003-4002-2434 | - |
crisitem.author.orcid | 0000-0002-4190-6592 | - |
crisitem.journal.journalissn | 0094-8276 | - |
crisitem.journal.ance | E070238 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
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Krohn_GRL_2018.pdf | postprint | 4.23 MB | Adobe PDF | Visualizza/apri |
114_Krohn_GRL_2018.pdf | Pdf editoriale | 4.62 MB | Adobe PDF | Visualizza/apri |
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