Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/28707
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Lam, K. W. F. | en_US |
dc.contributor.author | Santerne, A. | en_US |
dc.contributor.author | Sousa, S. G. | en_US |
dc.contributor.author | Vigan, A. | en_US |
dc.contributor.author | Armstrong, D. J. | en_US |
dc.contributor.author | Barros, S. C. C. | en_US |
dc.contributor.author | Brugger, B. | en_US |
dc.contributor.author | Adibekyan, V. | en_US |
dc.contributor.author | Almenara, J. -M. | en_US |
dc.contributor.author | Delgado Mena, E. | en_US |
dc.contributor.author | Dumusque, X. | en_US |
dc.contributor.author | Barrado, D. | en_US |
dc.contributor.author | Bayliss, D. | en_US |
dc.contributor.author | BONOMO, ALDO STEFANO | en_US |
dc.contributor.author | Bouchy, F. | en_US |
dc.contributor.author | Brown, D. J. A. | en_US |
dc.contributor.author | Ciardi, D. | en_US |
dc.contributor.author | Deleuil, M. | en_US |
dc.contributor.author | Demangeon, O. | en_US |
dc.contributor.author | Faedi, F. | en_US |
dc.contributor.author | Foxell, E. | en_US |
dc.contributor.author | Jackman, J. A. G. | en_US |
dc.contributor.author | King, G. W. | en_US |
dc.contributor.author | Kirk, J. | en_US |
dc.contributor.author | LIGI, ROXANNE | en_US |
dc.contributor.author | Lillo-Box, J. | en_US |
dc.contributor.author | Lopez, T. | en_US |
dc.contributor.author | Lovis, C. | en_US |
dc.contributor.author | Louden, T. | en_US |
dc.contributor.author | Nielsen, L. D. | en_US |
dc.contributor.author | McCormac, J. | en_US |
dc.contributor.author | Mousis, O. | en_US |
dc.contributor.author | Osborn, H. P. | en_US |
dc.contributor.author | Pollacco, D. | en_US |
dc.contributor.author | Santos, N. C. | en_US |
dc.contributor.author | Udry, S. | en_US |
dc.contributor.author | Wheatley, P. J. | en_US |
dc.date.accessioned | 2020-12-04T15:02:09Z | - |
dc.date.available | 2020-12-04T15:02:09Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 0004-6361 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/28707 | - |
dc.description.abstract | We report the discovery of the super-Earth K2-265 b detected with K2 photometry. The planet orbits a bright (V<SUB>mag</SUB> = 11.1) star of spectral type G8V with a period of 2.37 days. We obtained high-precision follow-up radial velocity measurements from HARPS, and the joint Bayesian analysis showed that K2-265 b has a radius of 1.71 ± 0.11 R<SUB>⊕</SUB> and a mass of 6.54 ± 0.84 M<SUB>⊕</SUB>, corresponding to a bulk density of 7.1 ± 1.8 g cm<SUP>-3</SUP>. Composition analysis of the planet reveals an Earth-like, rocky interior; this object has a rock mass fraction of 80%. The short orbital period and small radius of the planet puts it below the lower limit of the photoevaporation gap, where the envelope of the planet could have eroded owing to strong stellar irradiation, leaving behind an exposed core. Knowledge of the planet core composition allows us to infer the possible formation and evolution mechanism responsible for its current physical parameters. | en_US |
dc.language.iso | eng | en_US |
dc.title | K2-265 b: a transiting rocky super-Earth | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1051/0004-6361/201834073 | en_US |
dc.identifier.scopus | 2-s2.0-85057742875 | en_US |
dc.identifier.isi | 000452371100001 | en_US |
dc.identifier.url | https://www.aanda.org/articles/aa/full_html/2018/12/aa34073-18/aa34073-18.html | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 620 | en_US |
dc.relation.firstpage | A77 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | ASTRONOMY & ASTROPHYSICS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2018A&A...620A..77L | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_6 Stars and stellar systems | 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.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
crisitem.journal.journalissn | 0004-6361 | - |
crisitem.journal.ance | E016240 | - |
crisitem.author.dept | O.A. Torino | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.orcid | 0000-0002-6177-198X | - |
crisitem.author.orcid | 0000-0002-6257-6051 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Lametal_2018.pdf | PDF editoriale | 2.55 MB | Adobe PDF | View/Open |
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